[meteorite-list] AD: Special: Extremely unusual Eucrite - NWA 5473

2010-11-10 Thread Chladnis Heirs
Dear Friends of truly unusual meteorites,


in a Quick-Special, we want to present to you a very uncommon and weird new
eucrite.

Just take a look and you'll agree, that we have here a HED of quite unique
appearance:

http://www.chladnis-heirs.com/special-nwa5473.html


It is a polymict eucrite, but extremely shocked. Instead of displaying as to
expect textureless impact melts,
the matrix consist of a large variety of grains and finest fragments,
looking almost like have been sprayed around. 
Very hard to cut material it is. Here and there large lighter clasts are
preserved.
A strange play of colours it has.

We had held back that stone for two years, 
usually if of new material somewhat more gets available, it will appear very
soon with different numbers.
Not so with that one, we are not aware of pairings since.

NWA 5473
Sahara, 2008
tkw 45.9g
polymict EUC
Shock level:  high
Weathering grade: moderate

Only a small stone it was;
with such fast-going exciting material of very limited availability,
we have always to vary a little bit, because of the different time zones, 
where to publish our Specials firstly, to be more fair. 
This time we offered NWA 5473 three hours earlier in the Germs forum,
and all slices went immediately.

But, the good news - the main mass of 23.2g is still free.

And the better news - we priced it fairly cheap for such a quite unique
material:   20$/g.

The polished cut face of the main mass is a little bit reflecting in the
photo,
it is looking as fine as the slices do.


So here you are!

Good luck!

Stefan Ralew  Martin Altmann


Chladni's Heirs
Munich - Berlin
Fine Meteorites for Science  Collectors

http://www.chladnis-heirs.com





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[meteorite-list] AD: Special: Especially r are EL4 - at an especially affordable rate - NWA 6 482

2010-12-01 Thread Chladnis Heirs
Dear meteorite friends,

Our newest Special shall be about an enstatite chondrite!

The enstatite chondrites, the most reduced chondrites, which have formed in
the inner solar system
and plot on the terrestrial fractionation line,
are a rare group and became only recently more widespread by the mega-find
of El Haggouina and pairings.

Unfortunately El Hagg is so strongly terrestrialized and altered, that
hardly and only in a very few pieces still chondrules were visible,
so that initially it was classified even as an aubrite.

Now we present with NWA 6482 more representative specimens of that
intriguing class,
showing a lot of nice and distinct chondrules
and it was still fresh  enough to emit a strange smell while cutting – most
probably from the exotic sulfide minerals, which are so typical for the
E-chondrites.
The material is somewhat crumbly, so that we let the slices unpolished.

And with NWA 6482, we’re able to offer an extremely rare petrologic
subtype:  It is classified as an  EL4.

The Bulletin database coughs out only 6 non-Antarctic  EL4s
(DaG 734, DaG 1031, HaH 317, NWA 4780, NWA 5409, SaU 188).
with a somewhat modest combined tkw of  2.8 kg.

..and additionally 5 Antarctic finds, totalling to a 0.2kg.

So we think, that our offer should be an excellent opportunity for the
systematical collector (and of course for all others too!).

We have to confess, that we had difficulties to set a price for this new
meteorite.
Enstatite chondrites, besides the fossil El Hagg, are traditionally a
somewhat costly affair,
well and now we have here an almost unobtainable subtype.
A web-research, if you like to do, results for EL4s always in a few offers
of the remainders of the Dar al Ganis, at prices around 150$/g.

You know, what we did? We sat down, looked out in the fairy-tale-snowscape
and said – Christmas is coming soon  


10$ a gram, as long as stock lasts


http://www.chladnis-heirs.com/special-nwa6482.html


And hope to make you happy with that!

All the Best!
Stefan  Martin

Chladni's Heirs
Munich - Berlin
Fine Meteorites for Science  Collectors

http://www.chladnis-heirs.com





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Re: [meteorite-list] AD: Special: NWA 6349 prov. - a PRIME Brachinite at a low preferential price

2011-01-18 Thread Chladnis Heirs

Dear meteorite friends,

As a starter for our new meteoritical year, we chose for our Special a truly
especially convincing offer:

An excellent brachinite.


The class of the brachinites comprises quite heterogeneous members and their
genesis and the kind and history of their possible parent body isn't fully
understood yet, which makes that type so thrilling for the actual research.

To avoid iteration of former discussions and explanations on the
brachinite-group here on the list and in our specials and in fully
recognizing, that no one could better present the different types in such an
up-to-date and comprehensive manner than him, we recommend to consult David
Weir's famous meteorite studies homepage to get an insight into the
brachinite-topic.

With NWA 6349 today an attractive and very elegant representative of its
class climbs in the ring.

As you see already on the pictures, NWA 6349 lacks the brownish tint and
color, which other brachinites commonly share and which you connect with
that type, remembering the illustrations in the books of the classic one,
Eagles Nest.

It is, because NWA 6349 isn't so weathered like the others, but of a still
good freshness.


With several new numbers in the recent 2-3 years - and also the Bulletin
database not yet fully updated with the newer ones, (but also the holders of
samples of them being somewhat scrooge in loading up photos of their
specimens in the EoM), the situation with the brachinites is currently still
somewhat opaque.

We personally believe to see actually  4 complexes:

- NWA 3151, highlighted as the first true BRA from NWA + pairings.
- NWA 5471  possible pairings
- The stones around NWA 4882  NWA 5969, the latter the freshest of all
- And let us add, although no brachinites, the recent brachinite-like
numbers NWA 5400 et seqq.


There are indications, that our NWA 6349 with its 730g tkw may be a pairing
of NWA 4882.


Here are coming now the slices, as always with one polished side:

http://www.chladnis-heirs.com/special-nwa6349.html


Despite the recent numbers and nevertheless, a glimpse in the Bulletin
Database shows, how shockingly rare that type is (and of what for a crucial
importance the NWA finds are for research);

The quality of the NWA 6349 material is evident, the price of the alleged
possible pairings maybe here and there in the back of your mind, so that we
finally think, 
that our pricing of 40$ a gram
will make NWA 6349 for the collector  curator 
to an especially joyful brachinite.

With our best wishes,

Stefan  Martin

Chladni's Heirs
Munich - Berlin
Fine Meteorites for Science  Collectors 

http://www.chladnis-heirs.com




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[meteorite-list] AD: Special: NWA 6021 - a very pretty CO3

2011-01-26 Thread Chladnis Heirs
Dear fellow enthusiasts,


Here in our actual Special, we want to introduce a carbonaceous beauty, a
new CO3:  NWA 6021.


CO3s were and are still a little bit underestimated in the favorableness of
the collectors.
They never got the popularity of the CVs and CMs, most probably, because
they hadn’t these massive falls like Allende and Murchison
of the direct Apollo-period, which consequently were not only easily
available, but discussed at length and pictured in each and every popular
book. While the most important CO3-fall, Kainsaz, was locked away for the
collector behind the iron curtain, else there were only Lancé, Ornans, Isna
and Colony – all with very modest tkws, museum stuff, with limited
opportunities to gather a small cut – and so costly, that the whole class
was something only for the very experienced and specialized connoisseur. 
Really available the CO3s became not before the 2nd half of the 1990ies,
when the finds of the larger pairing group of the DaGs in Libya were made.
Additionally another reason might have been, that CO3s are of not so
striking first appeal, but CO3s require a closer look.
Though that attitude has already changed a bit with the fall of Moss.

And do you know what?
The novercal neglecting of the CO3s by the collectors is absolutely
undeserved.
One has to examine these rocks only a little bit en detail, if you allow
them to come only a little bit closer to your eyes,
an incredible cosmos will open to you, richer than in any other of the
carbonaceous types!

CO-chondrites have chondrules to excess, sharply defined and not very
metamorphosed.
Their matrix is similar to that of the CV3s, as well as the chondrules
composition, they’re only much more smaller, so small like those in the
CM2s,
but they have three times more chondrules than the CMs – and they have many
more olivine aggregates than the CV3s.
And yes, they contain CAIs too, the reason, why you bought once your first
Allende.

One has it all and more than that – but on a miniature stage.
Take a magnifying glass and you’ll recover what for a wonderful and
fascinating affair the COs really are.


Now with NWA  6021 we’re glad to introduce an aesthetically especially
pleasing representative of that class:

http://www.chladnis-heirs.com/special-nwa6021.html


Densest clouds of chondrules!
To some of you immediately will come the gimmicky title into mind once
attributed to the later Kainsaz-finds:  the “Space-van-Goghs”.
But other than with these, the stainings causing these wonderful patterns
are in NWA 6021 not so brown oxidized.

For you being able to enjoy the full beauty of this meteorite also on a
minor scale,
the slices are of course professionally polished.

The price for these daedal pieces of art by nature,
is somewhat under average, the slices are of good sizes and though for every
purse affordable.

And we are convinced, that your specimen will bring you satisfaction and
hours of joy on long winter’s evenings.

All the best,
Stefan  Martin

Chladni's Heirs
Munich - Berlin
Fine Meteorites for Science  Collectors

http://www.chladnis-heirs.com




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[meteorite-list] AD: Special: Truly Perplexing New Rumurutiite NWA 6022 prov. ( budget slices of fresh BRA NWA 6349)

2011-02-02 Thread Chladnis Heirs
Dear meteorite community,

today we demonstrate once again, why our Specials are called special.

We have here a new R-chondrite
- which alone, also in our spoiled times, is something very remarkable.  -
But..
Usually, as you know us,  we would explain the particular properties of the
type, chemically and textural details, perhaps we would make some historical
excursions, would tell about statistics, masses, ev. a little price 
availability discourse ...and so on.

But here?

I think we should simply let you alone for some minutes with the pictures.

http://www.chladnis-heirs.com/special-nwa6022.html


Well.
We issued really a lot of different Rumurutiites the recent years, but one
like that one, we haven't seen yet - have you?

A very unique appeal. That very distinct and constantly thick weathering
frame all around.
That grayish-brown matrix, with the orange freckles everywhere.
Unbrecciated.
Chondrules - it is classified as an R4.
And here and there these huge inclusions, sometimes alabaster sometimes
somewhat pink, as if they would be borrowed from a bencubbinite.
Very interesting material, isn't it?
One could suppose that this strange appeal may be phenomena of extensive
weathering, but it isn't - as with W2/3  NWA 6022 is slightly fresher than
the average.

As we - and most probably you neither - haven't seen such an R before and so
far, we guess, that it must be unpaired.

Alas. Spectacular it is.

So let's keep the Special even more special.
The R-chondrite-prices everywhere you know - 
we say simply and despite these unique appearance:   20$ per gram

(and both Chladni's Heirs have a bet running, how quickly this special will
have been sold out :-)


And an addendum we have.

You might remember the very fine, fresher and affordable brachinite, NWA
6349, form the last but one special.
There we were asked, whether we couldn't cut also some smaller slices.
So we prepared also some very good budget pieces - at the same price per
gram like the large ones.

Here you are:
http://www.chladnis-heirs.com/special-nwa6349-2.html


Best wishes!

Martin  Stefan

Chladni's Heirs
Munich - Berlin
Fine Meteorites for Science  Collectors

http://www.chladnis-heirs.com




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[meteorite-list] AD: Special: Gemmology of Vesta - Blossoms of Planetary Poetry

2011-02-13 Thread Chladnis Heirs
Dear Passionates,


today we make something different than usual - curious as we are, we want to
test whether facebook could be something for us and launched our special
offer there.

For the impatient ones - here already the link:
http://kuerzer.de/VestaGems

But don't worry, if you're not familiar with or if facebook is suspect to
you,
just give us a note, and we immediately will send you a private email 
with pictures  prices of all available specimens.


For that experiment we chose quite the most fabulous material which was
readily prepared at hand.

A few of you will remember our NWA 5478.
That incredible eucrite with such a diversity of appearances, from a perfect
Moon mimicry, to patterns you rather would expect on the catwalks of Paris
or Milano,
up to picture puzzles of fine art:

http://www.chladnis-heirs.com/euc-face.jpg


We were lucky to gather a longer while ago a few marbles of this material
more.
Or to say it like it should be correct:  
Some stones which we personally strongly believe to be paired to NWA 5478.

Of course they will be correctly classified and they will obtain an own
NWA-number.

In fact we rather would have waited until we got the number, before we'd
think about setting them on sale,
but when we showed that specimen:
http://www.chladnis-heirs.com/1_062gb.jpg

..the collectors urged us to offer them already in advance.

We always sincerely hoped to get one day a larger stone of that material,
without doubts such a specimen would be from the beginning on: legend.
Alas, three years waiting yielded nothing more than these few pebbles, less
than a small handful.
If you keep in mind, that on a find site or in a strewnfield always the
largest stones are picked up first and the smallest found last, we're not
confident that our dream ever will come true.
However.
As small as the marbles are, it is certainly one of the finest HEDs, the
deserts ever spat out.

23 specimens we have for sale.
All are true astonishing gems. All are polished half-stones.

The price per gram is higher than for average eucrites,
but because the weights of the gems are so small,
the overall-prices for the specimens are very comfortable.

They rank between 51$ and 180$ per piece,
two are larger and cost 500$ and 700$.


Only with the best specimen of the whole new series we will make an
exception,
and will have a kind of an private auction without hurry.
Highest bid will fetch it, increments are 10$,
Secret maximum bids remain secret and will automatically used only to that
extent necessary to hold the leading bid.
http://www.chladnis-heirs.com/1_062gb.jpg

And that, until nobody wants to bid more. With fair warnings.
Hence without battles in the last 10 seconds.

We're quite in the beginning at 90$ now.

Duration - a day will be enough, but also necessary, for the Japanese and
Australian collectors having a chance too.

So again,
Don't be shy to ask us for an email, if you don't like facebook.
Alone the pictures you HAVE to see, they are a delight.


Have all a fine and relaxing Sunday!

Stefan  Martin

Chladni's Heirs
Munich - Berlin
Fine Meteorites for Science  Collectors

http://www.chladnis-heirs.com






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[meteorite-list] AD: The Pearls of the Vestals - Budget pieces

2011-02-20 Thread Chladnis Heirs
Dear list,

Normally we hardly advertise a meteorite twice, but this time we want to
give you a short note,
because we hadn't set up a Special like usually - in general we wait for
the NWA-number first,
though when we had shown samples of this meteorite, the collectors didn't
want to wait.

And first and foremost, because this meteorite after our fancy, regarding
its beauty and the huge variety of its forms of appearances, the cut stones
offer,  belongs to the most outstanding eucrites of our times.

It's about the supposed NWA 5478-pairing from recently. After almost the
whole load was sold out within one day, Stefan expertly prepared the
remaining marbles we had left.  Small half-stones,
and the second course now, could be of special interest for the collector
with limited budget, as the pieces rank between 20 and 60$ - many of them
already gone too.
(And for those aiming for highlights for their collections: the main mass
stone, cut into halves is still available too).
Despite the weights being small, we believe the specimens to be very use-
and meaningful for any collector, as they show such an overabundance of
amazing details and uncommon features, 
and aesthetically seen, they a true jewels.

Well, and to whom that all sounds somewhat too elated,
let's say it more soberly:  If from 41 specimens, 32 are gone in 2 days -
then that eucrite and that offer must have something..  

So, just for feeling not responsible, for someone missing out on,
we just wanted to give that quick reminder.

If you're interested in, please send us an email, and we will send back the
details about the pieces still left.

(and if you ever wanted to know, why Vesta is a goddess? - You'll do so :-)


Thank you for your attention,
And have a fine Sunday.

Martin  Stefan

Chladni's Heirs
Munich - Berlin
Fine Meteorites for Science  Collectors

http://www.chladnis-heirs.com



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[meteorite-list] Your Strong Presence in the Solar System

2011-03-19 Thread Chladnis Heirs
Hello all,

and one thing you should not forget, so surprisingly it may sound for the
one or the other:

You all here on the list are actively taking part in and grandly supporting
the exploration of our Solar System, either in hunting samples of the
celestial bodies of our Solar System or enabling with your purchases of your
collection specimens the work of the prominent and of the anonymous hunters.

You're building up the backbone of earthbound planetology - and that more
than ever.

Your enthusiasm for the rocks of space and your hand-tight money spent grant
that all these samples and materials are and steadily become available for
science. Those samples, which mankind with its technical and financial means
cannot retrieve else and which allow a more profound, much broader and
detailed research on the history and compositions of the bodies of the Solar
System than remote sensoring with space probes and in situ work with landers
and rovers allow.

Let's all hope, that this awareness wins recognition also in those
countries, which are about or already have abandoned that most low-cost, but
in the same place extremely efficient form of planetary research and
exploration of the Solar system in taking away the legal preconditions
necessary that those materials can be found at all.

 
Let us take the opportunity to portend the next set of brand-new abstracts
with new data and results about our recent Martian meteorites;
Stones, which never could have been found without the help of the
collectors, the tireless dedication of the anonymous hunters in Sahara and
the support of the scientists.
To all of you we and science owe deepest respect.



Introducing abstract for NWA 6162:  

S. M.Kuehner, A. J. Irving, C. D. K. Herd, M. Gellissen, T. J. Lapen and D.
Rumble, III:

PRISTINE OLIVINE-PHYRIC SHERGOTTITE NORTHWEST AFRICA 6162: A PRIMITIVE MAGMA
WITH ACCUMULATED CRYSTALS DERIVED FROM DEPLETED MARTIAN MANTLE.

http://www.lpi.usra.edu/meetings/lpsc2011/pdf/1610.pdf



Dating and formation of the depleted permafic diabase NWA 5990: 

C.-Y. Shih, L. E. Nyquist, Y. Reese, and A. J. Irving:
Rb-Sr AND Sm-Nd AGES, AND PETROGENESIS OF DEPLETED SHERGOTTITE NORTHWEST
AFRICA 5990.

http://www.lpi.usra.edu/meetings/lpsc2011/pdf/1846.pdf


New data for cosmic and terrestrial ages for eight Martian meteorites,
among them NWA 4925 and NWA 5789:

K. Nishiizumi, K. Nagao, M. W. Caffee, A. J. T. Jull, and A. J. Irving:
COSMIC-RAY EXPOSURE CHRONOLOGIES OF DEPLETED OLIVINE-PHYRIC SHERGOTTITES.

http://www.lpi.usra.edu/meetings/lpsc2011/pdf/2371.pdf



Let the voyage go on!
Have all a fine weekend.

Martin  Stefan

Chladni's Heirs
Munich - Berlin
Fine Meteorites for Science  Collectors 

http://www.chladnis-heirs.com



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Re: [meteorite-list] Help with Kunya-Urgench

2010-05-06 Thread Chladnis Heirs
Hi Henry and Gary,

in my opinion this specimen is definitely no Kunya-Urgench.

In principle Kunya-Urgench, if fresh, is of a light-grey to witish
appearance. 

But Kunya seemed to have to be exposed to humidity on the place of fall,
so that it has more or less very often hefty stainings from rust.

Kunya was a large mass - the second largest stone meteorites in existence.
Scattered around the impact pit were collected hundreds of small and
smallest fragments and a few larger ones.
Some of the hunters, who collected them, are here also on the list.

The small fragmets, usually in the weight range form 1-10 grams, are almost
all very oxidized, but nevertheless some show here and there still some
fresh corners.

The larger ones (like necessary for having such a cut like Henry has)are
often somewhat better preserved.
The clean ones are withish grey mottled with tiny brown and ochre rust
spots, the somewhat more oxidized ones, have larger areas of rust.

But all have still parts of the original fresh matrix preserved.

Here some examples of various degrees of oxidation of Kunya.
http://www.thetricottetcollection.com/met_kunyaurgench.html

http://www.meteoritelabels.com/images/Kunya.jpg

http://www.meteorite-martin.de/images/meteor/kunyaurgench.jpg


Henry's specimen display a fully oxidized matrix, hence it is an old and
weathered chondrite, which certainly doesn't belong to the fall of
Kunya-Urgench.

I'd recommend to return it to the seller.

Best!
Martin


-Ursprüngliche Nachricht-
Von: meteorite-list-boun...@meteoritecentral.com
[mailto:meteorite-list-boun...@meteoritecentral.com] Im Auftrag von Gary
Fujihara
Gesendet: Donnerstag, 6. Mai 2010 04:07
An: hxmendoza
Cc: meteorite-list@meteoritecentral.com
Betreff: Re: [meteorite-list] Help with Kunya-Urgench

Henry Mendoza's specimen, possibly Kunya-Urgench:

http://bigkahuna-meteorites.com/Images/KU.jpg

On May 5, 2010, at 3:59 PM, hxmendoza wrote:

 Thanks for the responses folks. I've tried replying to some of you  
 emails directly. I hope you received them as I don't know how it works  
 when the emails are sent thru this list.
 
 I work graveyards eight on and six off. Tonite is the first day of my  
 eight day stretch so it's off to work I go. I will try to send pics of  
 my mystery endpiece over the next couple days or so to whomever asks  
 for them, as time permits. I sent them to Gary Fujihara as he said he  
 may post them thru his website for me. Thanks once again Gary. Oh and  
 did I tell you folks that  Gary's a swell guy?! LOL!!
 
 Ann thank you. And yes I don't believe the dealer in question to be  
 deceitful just very disorganized. I really believe that.
 
 Martin, my endpiece matrix does not look like that. On the Meteorite  
 Bulletin listing for the Kunya, the only puc that matches mine is the  
 one posted by a person called Brice D. Hornback, or something like  
 that. It's a little slice in an acrylic box.
 Gotta go. If work permits I'll keep reading. Nite to you all.
 
 Regards,
 Henry Mendoza
 Aurora, CO
 
 Sent from my iPod
 
 
 
 
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Gary Fujihara
Big Kahuna Meteorites (IMCA#1693)
105 Puhili Place, Hilo, Hawai'i 96720
http://bigkahuna-meteorites.com/
http://shop.ebay.com/fujmon/m.html  
(808) 640-9161

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[meteorite-list] AD: Short Note - Last 6 small pieces of the sensational NWA 6162 prov. Martian

2010-07-20 Thread Chladnis Heirs
Dear list members,

reading Ron's last posting below, it seems, that in some years we'll get
some competition by NASA and ESA.

Was already there,
Said the hedgehog 
to the hare...

Now seriously, we're about to distribute the very last six samples of the
best shergottite.
When they'll be gone, then NWA 6162 prov. unfortunately will be already
history.

To try to do justice to that material in a hyperventilating staccato of
superlatives would fail,
just click instead on these pictures given in this link again to get a vague
impression.
http://www.rocksfromspace.org/June_12_2010.html

It is stunning and it is breathtaking.
Ask those, who already have their specimen home or in the lab.

The only alternatives of comparable freshness among the shergottites to NWA
6162 are Zagami and Shergotty.
But NWA 6162 is somewhat more eye-appealing.

I hope we have now supplied all Martian-complete-collectors.

These are the last 3 grams of the 89g stone.

We currently have 5 partslices left - all with a long fusion-crusted edge:

0.290g

0.398g

0.415g

0.437g

0.450g

As well as a partial endcut with especially much of the fantastic crust

0.916g


Email for (moderate) prices and pictures.


And don't forget to take a look to the Western evening sky and the planetary
theatre we have these days there going on; also to see, where your specimen
really comes from!

Best greetings,

Martin  Stefan


Chladni's Heirs
Munich - Berlin
Fine Meteorites for Science  Collectors

http://www.chladnis-heirs.com




 



-Ursprüngliche Nachricht-
Von: meteorite-list-boun...@meteoritecentral.com
[mailto:meteorite-list-boun...@meteoritecentral.com] Im Auftrag von Ron
Baalke
Gesendet: Dienstag, 20. Juli 2010 18:07
An: Meteorite Mailing List
Betreff: [meteorite-list] Mars Sample Return Mission Could Begin in 2018


http://www.spaceflightnow.com/news/n1007/20sample/


Mars sample return mission could begin in 2018
BY STEPHEN CLARK 
SPACEFLIGHT NOW
July 20, 2010

Space officials in the United States and Europe are planning an
ambitious dual-rover mission that could start collecting Martian soil
samples in 2018 to be picked up by a subsequent mission and returned to
Earth in the 2020s.

The costly mission would blast off on an Atlas 5 rocket in 2018 and land
two rovers on Mars with a single sky crane descent system that will be
tested for the first time at the Red Planet in August 2012.

It would be the first time two rovers will be delivered to the same
landing site on Mars.

The European Space Agency's ExoMars rover and a $2 billion NASA Mars
Astrobiology Explorer-Cacher mission are the leading candidates for the
tandem project.

ExoMars carries a drill to burrow into the Mars subsurface and retrieve
samples from as deep as six feet underground. Some of that soil could be
placed inside a high-tech storage device on NASA's rover for eventual
return to Earth, according to Doug McCuistion, head of the agency's Mars
exploration program.

There may be a possibility to actually cache subsurface samples that
the ExoMars drill collects, which had not been in our plans before,
McCuistion said in an interview last week.

Marcello Coradini, ESA's coordinator for solar system missions,
confirmed the studies of placing underground samples into a NASA cache
for later retrieval.

We're hoping that what we do with our rover is actually collect the
samples that we will then go back in the 2020s to retrieve in the Mars
sample return campaign, McCuistion said.

A simple sample cache was originally planned for NASA's Mars Science
Laboratory launching next year, but officials removed the payload due to
scientific and technical concerns, according to McCuistion.

Spacecraft traveling from Earth to Mars can only launch about every 26
months, limiting sample return options. Scientists agree the best
strategy is to spread the effort across three missions to spread the
high cost of the endeavor among several years.

By breaking it up into those three pieces, you can sort of thread the
costs and spread some of the risks over multiple missions and make the
overall program both more robust and more affordable, said Steve
Squyres, a Cornell University researcher leading an independent review
of potential NASA science missions.

Called the decadal survey, the review will rank the scientific value of
28 proposed missions for the next 10 years.

The ultimate timing of a sample return campaign will boil down to the
budget of both NASA and ESA, McCuistion said.

David Southwood, ESA's director of science and robotic exploration, said
kicking off a sample return campaign by 2020 would mean going above the
200 million (euros) a year we're assuming as a steady-state (budget) in
the late part of this decade.

Squyres said the decadal survey will attempt to settle on an estimated
total cost for three sample return missions. Recent cost projections
have pegged the effort's total price at more than $5 billion.

(The sample return missions) could be spaced as close as close 

Re: [meteorite-list] Rocks from Space Picture of the Day - August 24, 2010

2010-08-24 Thread Chladnis Heirs
Hi Richard,

Chladnite is a synonym for enstatite and was a synonym for the aubrites
among the meteorites.

That mineral name was introduced by Charles U. Shepard (1804-1886) in 1846
when he firstly observed enstatite in the 1843 fallen Bishopville aubrite,
to honor Ernst Florens Friedrich Chladni as the founder of modern
meteoritics.


Best!
Martin  Stefan

Chladni's Heirs
Munich - Berlin
Fine Meteorites for Science  Collectors

http://www.chladnis-heirs.com
 

-Ursprüngliche Nachricht-
Von: meteorite-list-boun...@meteoritecentral.com
[mailto:meteorite-list-boun...@meteoritecentral.com] Im Auftrag von Richard
Kowalski
Gesendet: Dienstag, 24. August 2010 06:45
An: meteorite list
Betreff: Re: [meteorite-list] Rocks from Space Picture of the Day - August
24, 2010

Chladnite?

I see this fall is now classified as a Diogenite but could anyone discuss
the term Chladnite a bit more?

Nice addition to the fall collection Mike!

--
Richard Kowalski
Full Moon Photography
IMCA #1081


--- On Mon, 8/23/10, Michael Johnson mich...@rocksfromspace.org wrote:

 From: Michael Johnson mich...@rocksfromspace.org
 Subject: [meteorite-list] Rocks from Space Picture of the Day - August 24,
2010
 To: meteorite-list@meteoritecentral.com
 Date: Monday, August 23, 2010, 9:38 PM
 http://www.rocksfromspace.org/August_24_2010.html
 
 
 
 ---
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Re: [meteorite-list] More on Chladnite (Was: Rocks from Space Picture of the Day - August 24, 2010) - Part 2

2010-08-26 Thread Chladnis Heirs
And because it would be unfair, to have lost that great name this way,
We have since 1994 the mineral:  Chladniite

http://webmineral.com/data/Chladniite.shtml

Best!


-Ursprüngliche Nachricht-
Von: meteorite-list-boun...@meteoritecentral.com
[mailto:meteorite-list-boun...@meteoritecentral.com] Im Auftrag von
bernd.pa...@paulinet.de
Gesendet: Dienstag, 24. August 2010 18:57
An: Meteorite-list@meteoritecentral.com
Betreff: [meteorite-list] More on Chladnite (Was: Rocks from Space Picture
of the Day - August 24, 2010) - Part 2

BURKE J.G. (1986) Cosmic Debris, Meteorites in History, Chapter 4, p. 121:

Chladnite:

Again, it was an observation by Charles U. Shepard that paved the way toward
the
identification of the pyroxenes. In 1846 he described a mineral which, he
wrote,
is a ter-silicate of magnesia...[and] forms more than two-thirds of the
Bishopville
stone. He named the mineral chladnite in honor of Chladni, the scientific
founder
of this department of knowledge. Two years later Shepard reported his
analytical
results: 70 percent silicic acid,  28 percent magnesia, and 1 percent soda,
so that the
ratio of oxygen in the magnesia to that in the silica was 1 to 3. In 1851
Sartorius von
Waltershausen analyzed a fragment of the Bishopville meteorite and arrived
at about
the same results, but also found 1.5 percent alumina. Though making errors
in his
calculations, Sartorius did produce the correct formula - MgO,SiO2; however,
he
postulated that chladnite was a kind of wollastonite, in which magnesia
substituted
for lime. The issue was confused further in 1861, when Rammelsberg found by
analysis almost 3 percent alumina, 35 percent magnesia, and only 57.5
percent silicic
acid. Doubting the existence of a definite mineral, Rammelsberg did not
attempt to
devise a chemical formula.

Meanwhile, Shepard in 1854 described the Tucson iron meteorite and
speculated
that certain inclusions were chladnite. J. Lawrence Smith immediately
corrected
him, pointing out that the inclusions were actually olivine, and added a
note that
he suspected chladnite is likely to prove a pyroxene. At about the same
time, in
1855, Gustav A. Kenngott, professor of mineralogy at Zurich, published a
memoir
giving details of the minerals of what he termed the augite group of the
pyroxenes.
One member of the group was enstatite, which, Kenngott wrote, was a
bisilicate of
magnesia, was augitic in crystallization, and had the formula 3MgO,2SiO3.
In 1861, when Kenngott saw Rammelsberg's analysis of chladnite, he insisted
that
the mineral was identical with enstatite. Smith then made two analyses of
the
Bishopville meteorite and reported in 1864 that chladnite consisted of 60
percent
silica and nearly 40 percent magnesia. He agreed with Kenngott that the
mineral
was the magnesian pyroxene, enstatite, and accepted Kenngott's formula, in
which
the oxygen content of the magnesia to that of the silica was 1 to 2. Both
Rammelsberg
and Maskelyne acted to clarify the formula of enstatite, and through his
work on the
Breitenbach, Bustee, and Manegaon meteorites, Maskelyne recognized the
existence
of solid-solution series that included enstatite and bronzite. By the 1870s
mineralogists
began to report regularly these constituents in meteorites.

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[meteorite-list] AD: Special: A New, unusual and Unbrecciated Aubrite! NWA 6350 prov

2010-10-13 Thread Chladnis Heirs
Dear collectors and meteoricists,


after a long time, we are back with one of our Specials,
which became necessary, as this time we want to introduce a stone,
where it's difficult to avoid the so worn-out term: Sensational.


NWA 6350 provisional- A new aubrite.


If you follow us, in checking the Meteoritical Bulletin database,
you'll understand, why this find has such a special meaning for us.

The database is still somewhat biased, as the numerous El Haggouina-pairings
there aren't changed from AUB to EL yet.
(And with them we personally follow Bunch, Wittke, Irving et al. that El
Haggouina is an EL).

So the first true aubrite in the list there, should be NWA 4799.
You remember, it was introduced here on the list, the very uncommon highly
brecciated one.
To what extent NWA 4832/4871 are belonging to NWA 4799, that we don't know
yet; David Weir lists 4871 as a pairing of NWA 4799

Find them here, also a wonderful resource of information, on the meteorite
pages of NAU:
http://www4.nau.edu/meteorite/Meteorite/Aubrite.html


For NWA 5419 zero information is available, therefore not yet clear in which
context it belongs.


Well, and the second real aubrite was NWA 5217.
NWA 6350 is paired to it.

Therefore, from 2 decades of desert hunt in Sahara and 1 decade in Oman,
we have so far most probably only two different aubrites at all.
And aubrites are the most difficult discipline, it seems much more easier to
find a lunaite or even a nakhlite.


Hence, we choose in the title several attributes:  

Unbrecciated we wrote, to show, that it is not paired with NWA 4799.

Fresh we could have added,
not only because NWA 6350 is relatively well preserved, but to signal, that
it isn't just another El Hagg.

But why we said New?
NWA 5217 was a small stone of 40grams. It is listed in the Bulletin to be at
an Anonymous.
Never we saw it offered - with NWA 6350 for the first time this exciting
material will be available for the collector.


Unusual: 

NWA 6350/5217 as well as NWA 4799 are important finds.
They both are distinct from the other aubrites.

Let us simply quote from that short abstract:
http://www.lpi.usra.edu/meetings/metsoc2008/pdf/5309.pdf

The high temperature igneous cumulate characteristics
of NWA 4799 and 5217 are unique among aubrites.
Moreover, the complex mineralogy of NWA 5217 is remarkable
and distinctive. Because these aubrites appear to be igneous cumulates
and not derived from shock melts, they likely formed in
a fairly large parent body rather than a small asteroid (such as
main belt E asteroids and the NEO E asteroid 3103 Eger [2]).


And now in medias res.

NWA 6350 was unfortunately also of a very small tkw.  50grams the stone only
had.

The number of available specimens is so limited, that by far we wouldn't be
able to satisfy the needs of even only our truest collectors and customers.
Therefore we decided to set all pieces here on the list,
for everyone allowing the chance to get one equally.

We hope you don't mind, that we made an exception and had let David Weir to
pick a specimen in advance,
because his fantastic Meteorite Studies are such an enormous service to the
meteorite world,
that we think, that he deserves all support to keep his studies complete.
And - science first - one of the partial endcuts is temporary on hold for an
institute.

Although, as a cumulate one, its relative freshness and its tiny tkw,
we kept the prices with   60-100$/g 
still partially in the Pena Blanca Spring range.
That Norton County can be had cheaper, is explained, also to the historics
collector, well by this hilarious photo:
http://kuerzer.de/Aubpaz


Usually, whenever we announce a novelty of such a caliber,
quite a rush of emails comes over us.
It would be extremely helpful, if you would send us a ranking of the
specimens you desire,
to grant a fast and chronologically course.

Now - long enough we kept you on the tenterhooks.

Here they are:

http://www.chladnis-heirs.com/special-nwa6350.html



Let the games begin!

Stefan Ralew  Martin Altmann

Chladni's Heirs
Munich - Berlin
Fine Meteorites for Science  Collectors
http://www.chladnis-heirs.com





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Re: [meteorite-list] AD: Unbrecciated Aubrite! NWA 6350 prov Shallowater......

2010-10-16 Thread Chladnis Heirs
Hi Greg,

many thanks for the congrats!

Of course, 34 years Antarctic campaigns and only 2 different aubrites found
there; 20 years Sahara and 10 years Oman, also only 2 different aubrites...

But not only due this absurd rareness, that little stone is in our internal
VIP-meteorite-ranking settled quite near the top,
it's moreover the characteristics of the material itself!

We confess, that our Ad was a little bit inapt, as probably only the experts
recognized immediately, what we have there.

In fact it would have been easier and sufficient, just to write two
catchphrases:


  UNBRECCIATEDSHALLOWATER



You know, ALL aubrites were so far heftily brecciated, destroyed, shocked,
annealed, partially molten, partially morphed and metamorphed, brecciated,
brecciated and brecciated - with all the implications about their precursor
material, - El Haggouina's initially misclassification was no accident, melt
an E-chondrite and you get out something very similar to an aubrite - and
their possible parent bodies, small, large, differentiated, chondritic,
catastrophic collisions, regolith formation,... in space one is looking,
Steins or the Hungaria-Family  ect. pp.

ALL but one.  Shallowater!

The one and only originally preserved aubrite - the unbrecciated one.

And Shallowater was s alone.
So alone, that in former times, it got even a suffix -an added behind the
AUB:

Now Shallowater got a little sister and a little brother:   NWA 5217/6350.

And it's amazing. We read, that the little enstatites in Shallowater hadn't
grown randomly in all directions, but they show a preferred orientation,
which means they grew under gravitational influence - which in turn means,
that the parent body have had to be fairly large. 100km.
It's always astonishing, what you can read out from such a little stone.

See, Shallowater looks in several ways similar to NWA 6350.

TCU-specimen, photo Geoff Notkin:
http://tin.er.usgs.gov/meteor/get_original_photo.php?recno=5637847

Close-up - Hey Madame Anne has just two Shallowaters for sale!
(It's fairlyvery difficult to get any.)
http://www.impactika.com/catpix/AA043.jpg

Small slice, we had once:
http://www.chladnis-heirs.com/shallowater-0.455g.jpg



...if you'd ask us, we would say, that NWA 6350 is maybe a slight idea
fresher than Shallowater.
(and it seems to be mineralogically also somewhat more interesting, but the
research isn't finished yet).

Well, and there we see it, even the most inveterate historics collector has
to admit,
in what for meteoritically happy  fantastic years we're living right now!

And again and again we can't only appeal and pray for reason among the
responsible persons,
that they keep the deserts open!! For such stones, see Antarctica, see NWA,
see Dho you need terrific large find numbers,
until once such a find will be among them. And really most researchers don't
want to play only with a handful of weathered new L6s or H5s
a year.  MetSoc, scientists, collectors, curators - we all need your help,
that we won't destroy for ourselves all that, what we so laboriously,
but also so fantastically have built up these years.


It's only a pity, that NWA 5217 wasn't available and that NWA 6350 was such
a small stone too.
So to collectively answer all requests, it's sold out.
Though - cause it's a little bit unfair, that we explained the stone now a
little better:

There is still HOPE!

We still wait for the final o.k. by a researcher, for whom we had reserved
the 12.5g partial endcut:

http://www.chladnis-heirs.com/nwa6350-12.506g-end.JPG

http://www.chladnis-heirs.com/nwa6350-12.506g-end-2.JPG


We can't promise anything right now, because politeness requires to wait
still some days more,
but maybe maybe it will be free again and available.
So it's possible to secure an option on it, for that case.

At 60$/g - a tenth of the Shallowater price.
Desert made it possible.

All the best!
Martin  Stefan



-Ursprüngliche Nachricht-
Von: meteorite-list-boun...@meteoritecentral.com
[mailto:meteorite-list-boun...@meteoritecentral.com] Im Auftrag von
gmh...@htn.net
Gesendet: Donnerstag, 14. Oktober 2010 05:29
An: n...@chladnis-heirs.com; meteorite-list@meteoritecentral.com
Betreff: Re: [meteorite-list] AD: Special: A New, unusual and Unbrecciated
Aubrite! NWA 6350 prov

Hi Martin and List,

Congratulations to Martin and Stefan for your latest aubrite discovery and
becoming members of the NWA Aubrite Club! :-)

I am glad my NWA 4799 aubrite is with great company. For anyone interested
in a couple of 'images' of NWA 4799, here are some links I posted to the 
Met List in Feb. 2008:


NWA 4799 - The first TRUE Aubrite from Northwest Africa (as Martin stated
earlier):

Image of 26.7 gram polished half of largest stone:
http://www.lunarrock.com/nwa4799/nwa4799a.jpg

Image of large whitish enstatite grains at 26x magnification:
http://www.lunarrock.com/nwa4799/nwa4799c.jpg

Image of large enstatite grain and veins of goethite from 

[meteorite-list] AD: Special: New subtype - the First L-Metachondrite - NWA 6348 prov.

2010-10-16 Thread Chladnis Heirs
Dear meteorite enthusiasts,


Today we release already the next stunning Special.

The differences and relations between PACs, 7ers and metachondrites were
already once in detail discussed here on the list,
- for those not remembering so well, we – like always – recommend David
Weir’s Meteorite Studies:
http://www.meteoritestudies.com/

Therefore this Special and this new meteorite doesn’t require a such verbose
introduction like usually.

So far there were LL-, H-, CM- and CR-metachondrites,
funny enough L-metachondrites were still missing.


With NWA 6348 prov. we announce:  Mission accomplished.


NWA 6348 
was one stone, found this year, with a weight of 136g.
Averagely shocked with S3, nevertheless displaying various shock zones and
veins,
and with W2 somewhat less weathered than the average.

Here you have all specimens.

Prices:  50$/g for the small polished slices from 3g to 10g.  
 40$/g for specimens 10g.
 (The main mass is currently on hold).

http://www.chladnis-heirs.com/special-nwa6348.html


Have a fine weekend!

Stefan Ralew  Martin Altmann


Chladni's Heirs
Munich - Berlin
Fine Meteorites for Science  Collectors

http://www.chladnis-heirs.com 



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[meteorite-list] AD: Special: Absolutely Ama zing! The Trompe-l'œil-Eucrite NWA 6347prov . Fully recrystallized melted.

2010-10-21 Thread Chladnis Heirs
Good Morning Collectors!


For this Special it is absolutely necessary to show the pictures first!


http://www.chladnis-heirs.com/special-nwa6347.html



Hands up! To whom of you we could have sold it as Lunar?



Awesome, isn't it?
But what do we have here? 

An eucrite, 
which was completely melted, recrystallized afterwards and was in the end
brecciated into a fine jigsaw puzzle.

Extremely fine grained, no visible metal, wonderful shock veins.
Very fresh with a perfectly contrasting black fusion crust.


A stunner, an eyecatcher - no matter how full your showcase is already.
A stone, which makes us love our profession.

Quick the data:

NWA 6347 provisional
Sahara
Find 2010
Tkw 148g
Recrystallized and melted eucrite breccia

Prices 40-45$/g.  First come, first serve.


Promise us, to bring your slice not in the even far proximity of an NWA
482-label ;-)

All the Best!

Stefan  Martin 

Chladni's Heirs
Munich - Berlin
Fine Meteorites for Science  Collectors 

http://www.chladnis-heirs.com




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Re: [meteorite-list] metachondrite

2010-10-24 Thread Chladnis Heirs
Hi Steve,

no..  a metachondrite is a chondrite without chondrules  :-)

The meta comes from metamorph.
A metamorphosis means, that a rock is changed in its structure or its
composition into a different rock, but remaining in a solid state, while
this happens. This change can be caused by different agents, like heat,
pressure, liquids or contact with other rocks.

Well, with the metachondrites (or 7ers or PACs, where they were/are sorted
in too)
their chemistry and their isotopes are similar with or the same as the
respective chondrite groups.
L-metachondrites with L; H-metachondrites with H, LL-...ect.

Though - they are free of chondrules. 

But: they show evidence of recrystallization and in some of these stones of
that kind, one finds remainders left and relicts, which once were
chondrules.
Therefore it's clear, they were once chondrites (of the respective groups H,
LL, CV, CR  now with NWA 6348 the first one, named to come from the L-group)
and they are directly derived from the chondrites.

So. With the chondrites, you have always those numbers behind the H, L, ect.
- the petrological grade.  3,4,5,6.

In the type-3 chondrites, you have the full garden of these funny balls
called chondrules, sharply defined sitting in the matrix.
If you heat now the affair, the crystal growing will take place, and from
the 4, to 5, to the 6ers the chondrules and the matrix are more and more
grown together, the chondrules get less sharper defined, they got often also
more sparsely.
And a second thing happens, the constituents of such a 3er, they are
chemically and physically different from each other. But like all in
universe, they want to be balanced, they desire an equilibrium. If you heat
now such a rock, the ions can roam in the rock. And the constituents start
to assimilate to each other or to get in a chemical balance.
So the type-3 chondrites are those, which were least heated and are the most
unchanged preserved once. Called unequilibrated, while from type 4 on they
are called equilibrated. 

Well. So the chondrites evolve and are more and more changed from type-3 to
type 6.
But with the new finds from the deserts, we got some rocks, which showed,
that type 6 is not the end!
That there are also chondrites, which were more heated or were that process
continued - so that in the end they had lost all their chondrules, and got
the most equilibrated ones and fully recrystallized.

Two main heat sources you have for such parent bodies. Heating due impacts,
where the kinetic energy of the impactor is relieved in deformation of the
target rock and heat. The other one is after the formation of such a
celestial body, the radioactive decay of its instable and heavy elements.
The larger such a body is, the more of that stuff it has, the hotter it can
get - up to the complete melting of the body. And the larger such an body is
the longer it can keep the heat - Earth e.g. is large enough, that it was
quite still warm down there, where the Chilean miners were sitting.

Impacts, you know what happens, if the smack is hefty, then the rock beneath
simply melts - making these IMB, impact melt breccias meteorites,
usually quite black, homogenous and with textureless glasses.. 
The metachondrites are different from them.
If you take that idea with that heating by decay, then you can suppose, that
they once sat more deeper, closer to the core of their parent body than the
3ers, 4ers,... where it got hotter and where it was longer hot.

Now, cause 6 was obviously not the end, Dodd in the 1970ies thought it is
necessary to have also a 7.

Problem: Most of these crazy stones have no chondrules left.
Therefore some say: A chondrite is called a chondrite because it has
chondrules!
A stone, that has no chondrules has to be called: achondrite!!

Therfore a 7er-chondrite would be per definition not allowed.
And because the stuff is directly derived from chondrites, which are the
most primitive matter we have,
we put these stones into the group, we already have, where the ACAPs, LODs,
WINs are already sitting in
and call them primitive achondrites.

And that is somewhat unhappy. 
Achondrites we have all that stuff from differentiated, non-chondritic
parent bodies,
like the Vesta matters eucrites, diogenites, howardites, but also the
aubrites, ureilites, brachinites, angrites, Martians, Lunars...

But from these stones, we know exactly from their composition that they were
chondrites.
And primitive doesn't fit so well neither - because they aren't that
primitive but among the chondrites the most metamorph, most evolved, most
equilibrated ones of all.
And they are not an unchanged primary meteorite, they are a product of them.
The opposite of primitive.

The term Metachondrite is there more exact, it says: Look I was a
chondrite - I am a metamorph chondrite.
So in the name the genesis of the rock is already visible.
And it allows to be more specific,
as one hasn't to lump all these rocks, from ACAPs, WINs and all these
diverse ex-chondrites 

Re: [meteorite-list] metachondrite

2010-10-24 Thread Chladnis Heirs
 chondrule outlines 
sometimes persist.

The new term metachondrite has not been defined in the formal 
literature, but it seems to overlap with what I would call the high 
end of type 6 and primitive achondrites.  I think Ted Bunch reads this 
list, so he can chime in if this is not correct.  Personally, I see no 
benefit to this term, as I am comfortable calling those with chondritic 
compositions type 6 chondrites, and I am uncomfortable calling those 
which have differentiated chondrites, even with the prefix meta-.

Jeff

On 2010-10-24 10:16 AM, Chladnis Heirs wrote:
 Hi Steve,

 no..  a metachondrite is a chondrite without chondrules  :-)

 The meta comes from metamorph.
 A metamorphosis means, that a rock is changed in its structure or its
 composition into a different rock, but remaining in a solid state, while
 this happens. This change can be caused by different agents, like heat,
 pressure, liquids or contact with other rocks.

 Well, with the metachondrites (or 7ers or PACs, where they were/are sorted
 in too)
 their chemistry and their isotopes are similar with or the same as the
 respective chondrite groups.
 L-metachondrites with L; H-metachondrites with H, LL-...ect.

 Though - they are free of chondrules.

 But: they show evidence of recrystallization and in some of these stones
of
 that kind, one finds remainders left and relicts, which once were
 chondrules.
 Therefore it's clear, they were once chondrites (of the respective groups
H,
 LL, CV, CR  now with NWA 6348 the first one, named to come from the
L-group)
 and they are directly derived from the chondrites.

 So. With the chondrites, you have always those numbers behind the H, L,
ect.
 - the petrological grade.  3,4,5,6.

 In the type-3 chondrites, you have the full garden of these funny balls
 called chondrules, sharply defined sitting in the matrix.
 If you heat now the affair, the crystal growing will take place, and from
 the 4, to 5, to the 6ers the chondrules and the matrix are more and more
 grown together, the chondrules get less sharper defined, they got often
also
 more sparsely.
 And a second thing happens, the constituents of such a 3er, they are
 chemically and physically different from each other. But like all in
 universe, they want to be balanced, they desire an equilibrium. If you
heat
 now such a rock, the ions can roam in the rock. And the constituents start
 to assimilate to each other or to get in a chemical balance.
 So the type-3 chondrites are those, which were least heated and are the
most
 unchanged preserved once. Called unequilibrated, while from type 4 on they
 are called equilibrated.

 Well. So the chondrites evolve and are more and more changed from type-3
to
 type 6.
 But with the new finds from the deserts, we got some rocks, which showed,
 that type 6 is not the end!
 That there are also chondrites, which were more heated or were that
process
 continued - so that in the end they had lost all their chondrules, and got
 the most equilibrated ones and fully recrystallized.

 Two main heat sources you have for such parent bodies. Heating due
impacts,
 where the kinetic energy of the impactor is relieved in deformation of the
 target rock and heat. The other one is after the formation of such a
 celestial body, the radioactive decay of its instable and heavy elements.
 The larger such a body is, the more of that stuff it has, the hotter it
can
 get - up to the complete melting of the body. And the larger such an body
is
 the longer it can keep the heat - Earth e.g. is large enough, that it was
 quite still warm down there, where the Chilean miners were sitting.

 Impacts, you know what happens, if the smack is hefty, then the rock
beneath
 simply melts - making these IMB, impact melt breccias meteorites,
 usually quite black, homogenous and with textureless glasses..
 The metachondrites are different from them.
 If you take that idea with that heating by decay, then you can suppose,
that
 they once sat more deeper, closer to the core of their parent body than
the
 3ers, 4ers,... where it got hotter and where it was longer hot.

 Now, cause 6 was obviously not the end, Dodd in the 1970ies thought it is
 necessary to have also a 7.

 Problem: Most of these crazy stones have no chondrules left.
 Therefore some say: A chondrite is called a chondrite because it has
 chondrules!
 A stone, that has no chondrules has to be called: achondrite!!

 Therfore a 7er-chondrite would be per definition not allowed.
 And because the stuff is directly derived from chondrites, which are the
 most primitive matter we have,
 we put these stones into the group, we already have, where the ACAPs,
LODs,
 WINs are already sitting in
 and call them primitive achondrites.

 And that is somewhat unhappy.
 Achondrites we have all that stuff from differentiated, non-chondritic
 parent bodies,
 like the Vesta matters eucrites, diogenites, howardites, but also the
 aubrites, ureilites, brachinites, angrites, Martians, Lunars...

 But from

[meteorite-list] Video of Lunar and Martian Meteorites

2011-05-03 Thread Chladnis Heirs
Hello there,

as it seems, that videos presenting meteorites from all sides are
appreciated by you, let us show a little one we made a while ago from some
of
our planetaries.
We animated a little intro to set the stones in a context.

Well, here it is, the production from the Chladni Studios.  ;-)

http://www.chladnis-heirs.com/Filme/pl-meteorites.mp4

(has 77MB)

Hope, you'll like it.

Martin  Stefan

Chladni's Heirs
Munich - Berlin
Fine Meteorites for Science  Collectors

http://www.chladnis-heirs.com





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[meteorite-list] AD: Special: New uncommon Martian meteorite - NWA 6710 prov.

2011-05-04 Thread Chladnis Heirs
Good Day meteorite and planetary lovers,


Proudly we announce, that our next Martian has arrived, is sliced and
grinded already and waits now for flying into your collection!    

NWA 6710 (provisional)

will be its name and according the newer more systematic nomenclature it is
a

Intermediate Permafic Olivine-Phyric Shergottite.

Already a first glance reveals, that NWA 6710 doesn’t meet the usual viewing
habits for shergottites and that it must be in several aspects a fairly
uncommon material.

We see a matrix of very fresh appearance, which is so incredibly
fine-grained that macroscopically it almost looks uniformly.
Very sparsely we find a few patches of dark maskelynite, though the clou of
this Martian is:
Over and over it is peppered with fine olivines of an intensive pastel
green!

An amazing stone.

The planetary connoisseur is immediately aware:  there is only one such
Martian – it has to be a pairing of NWA 2990.
This grouplet consist of four members;  NWA 2990, NWA 5960, NWA 6234 and now
NWA 6710.

NWA 2990 is long ago gone.  NWA 5960 had a tragic fate, the main mass was
stolen in mail (a fate, which makes us all angry as it happened by such a
stupidity. Such a stone is absolutely unsalable for any thief and it is the
rarest matter on the globe, almost irreplaceable. Please alert us or the
owner immediately for the case, that such material will be offered to you).
And NWA 6234 seems already to be sold out too.

The characteristics of the entire stones were, that they are covered with a
very green skin.
Only NWA 2990 had one side with a good black fusion crust, while NWA 5960
and NWA 6234 were naked.
Not so our new NWA 6710, it has some dark fusion crust left, but worn and
not so fine preserved as with NWA 2990.
Internally all stones are very fresh.

NWA 6710 prov. has a tkw of 74 grams.

Astonishingly few is published yet about the NWA 2990-group, we think, that
will change now with the recent finds.
So that we can refer you at the moment only to the introductory paper for
NWA 2990 from two years ago, 
where you can find the essential details about this uncommon Mars rock:

T. E. Bunch, A. J. Irving, J. H. Wittke, D.Rumble, III, R. L. Korotev, M.
Gellissen and H. Palme:
PETROLOGY AND COMPOSITION OF NORTHWEST AFRICA 2990: A NEW TYPE OF
FINEGRAINED, ENRICHED, OLIVINE-PHYRIC SHERGOTTITE.
http://www.lpi.usra.edu/meetings/lpsc2009/pdf/2274.pdf


In medias res,
here you find our complete stock of available slices
- from the complete cross sections

http://www.chladnis-heirs.com/specials/special-nwa6710.html

down to smallest partial slices, small but more than meaningful enough to
serve for more than a sole place holder of the number.

http://www.chladnis-heirs.com/specials/special-nwa6710-2.html

And the best is, although it is a fresh and fairly uncommon shergottite, it
costs only half as much as our recent three Martians went for.

You'll love it!

Best regards,

Stefan  Martin

Martin Altmann  Stefan Ralew
Chladni's Heirs
Munich - Berlin
Fine Meteorites for Science  Collectors 

http://www.chladnis-heirs.com




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Re: [meteorite-list] AD: Special: New uncommon Martian meteorite - NWA6710 prov.

2011-05-04 Thread Chladnis Heirs
Hello Greg,

yes it's very bad.
Not only NWA 5960 went missing, had 124 grams, though in the same parcel a 
lunar NWA 2995-pairing of 118 grams went lost.

Find details here:
http://www.sahara-nayzak.com/stolen/planetary.html

Best,
Martin



-Ursprüngliche Nachricht-
Von: meteorite-list-boun...@meteoritecentral.com 
[mailto:meteorite-list-boun...@meteoritecentral.com] Im Auftrag von Greg Hupe
Gesendet: Mittwoch, 4. Mai 2011 23:30
An: Chladnis Heirs; meteorite-list@meteoritecentral.com
Betreff: Re: [meteorite-list] AD: Special: New uncommon Martian meteorite - 
NWA6710 prov.

Hello Martin,

Congrats on the NWA 6710 Martian! I am saddened to hear about the stolen NWA 
5960 pairing. I only just heard about this today and here through your 
announcement. What was the weight of 5960? I heard who the stone was shipped 
to and who the Moroccan dealer is. If this is a clear-cut case of theft by 
the recipient, then that person's name should be made known to all dealers, 
collectors and police if possible. I do not know any details, you know more 
than I do and I am sure you are helping the Moroccan dealer who was ripped 
off either by the shipping company or the recipient. This kind of behavior 
should not be tolerated. I hope the thief, whoever it is, finds a conscience 
and sends the stone back to the rightful owner! In the possibility that it 
got lost in shipping by the carrier, lets hope the wayward package, with 
stone, finds its way to the recipient or back to the Moroccan owner!

Best Regards,
Greg


Greg Hupe
The Hupe Collection
gmh...@centurylink.net
www.LunarRock.com
IMCA 3163


-Original Message- 
From: Chladnis Heirs
Sent: Wednesday, May 04, 2011 4:54 PM
To: meteorite-list@meteoritecentral.com
Subject: [meteorite-list] AD: Special: New uncommon Martian meteorite - 
NWA6710 prov.

Good Day meteorite and planetary lovers,


Proudly we announce, that our next Martian has arrived, is sliced and
grinded already and waits now for flying into your collection!

NWA 6710 (provisional)

will be its name and according the newer more systematic nomenclature it is
a

Intermediate Permafic Olivine-Phyric Shergottite.

Already a first glance reveals, that NWA 6710 doesn’t meet the usual viewing
habits for shergottites and that it must be in several aspects a fairly
uncommon material.

We see a matrix of very fresh appearance, which is so incredibly
fine-grained that macroscopically it almost looks uniformly.
Very sparsely we find a few patches of dark maskelynite, though the clou of
this Martian is:
Over and over it is peppered with fine olivines of an intensive pastel
green!

An amazing stone.

The planetary connoisseur is immediately aware:  there is only one such
Martian – it has to be a pairing of NWA 2990.
This grouplet consist of four members;  NWA 2990, NWA 5960, NWA 6234 and now
NWA 6710.

NWA 2990 is long ago gone.  NWA 5960 had a tragic fate, the main mass was
stolen in mail (a fate, which makes us all angry as it happened by such a
stupidity. Such a stone is absolutely unsalable for any thief and it is the
rarest matter on the globe, almost irreplaceable. Please alert us or the
owner immediately for the case, that such material will be offered to you).
And NWA 6234 seems already to be sold out too.

The characteristics of the entire stones were, that they are covered with a
very green skin.
Only NWA 2990 had one side with a good black fusion crust, while NWA 5960
and NWA 6234 were naked.
Not so our new NWA 6710, it has some dark fusion crust left, but worn and
not so fine preserved as with NWA 2990.
Internally all stones are very fresh.

NWA 6710 prov. has a tkw of 74 grams.

Astonishingly few is published yet about the NWA 2990-group, we think, that
will change now with the recent finds.
So that we can refer you at the moment only to the introductory paper for
NWA 2990 from two years ago,
where you can find the essential details about this uncommon Mars rock:

T. E. Bunch, A. J. Irving, J. H. Wittke, D.Rumble, III, R. L. Korotev, M.
Gellissen and H. Palme:
PETROLOGY AND COMPOSITION OF NORTHWEST AFRICA 2990: A NEW TYPE OF
FINEGRAINED, ENRICHED, OLIVINE-PHYRIC SHERGOTTITE.
http://www.lpi.usra.edu/meetings/lpsc2009/pdf/2274.pdf


In medias res,
here you find our complete stock of available slices
- from the complete cross sections

http://www.chladnis-heirs.com/specials/special-nwa6710.html

down to smallest partial slices, small but more than meaningful enough to
serve for more than a sole place holder of the number.

http://www.chladnis-heirs.com/specials/special-nwa6710-2.html

And the best is, although it is a fresh and fairly uncommon shergottite, it
costs only half as much as our recent three Martians went for.

You'll love it!

Best regards,

Stefan  Martin

Martin Altmann  Stefan Ralew
Chladni's Heirs
Munich - Berlin
Fine Meteorites for Science  Collectors

http://www.chladnis-heirs.com




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[meteorite-list] AD: Special: NWA 6826 - the Best Karoonda-Chondrite Chladni's Heirs ever had

2011-06-08 Thread Chladnis Heirs
Dear meteorite lovers and experts,


one of the grand specialties of Chladni's Heirs are the CK-Chondrites. 
Still this year, we will receive the number for our 20th CK,
all among each other unpaired - as many as nobody else had in that time
span.
Nevertheless the CK-chondrites remain rarer
than any CV, CO or any eucrite, diogenite and howardite.

Today, we have the honor and the joy to introduce to you,
that CK, which we consider the best CK of all we ever had:  NWA 6826.

Here already for the most hasty ones, the specimens!

http://www.chladnis-heirs.com/specials/special-nwa6826.html

 
Much we explained about the CK-group in our former Specials, their genetic
relation to the CV and CO-group,
their differences to these types and about the characteristics, which make
the CK-group so interesting and fascinating.
With NWA 6826 today, we will abstain from lengthy explanations and
iterations, (in case Weir's Studies will help you)
because the beauty of this very material
touches the heart of every collector.

Time it is - that we learned from many of our CKs,
and now this very NWA 6824 is the most incontrovertible argument for that -
to rewrite the old books, 
which disqualify the CKs as dull, chondrules- ad CAI-poor and featureless,
due to their sulphides and iron-oxides and shock-blackening.
(Probably they had only Kobe, Karoonda and old HaH 280/281 at hand).

NWA 6826 speaks a different language!

It demonstrates par excellence how vivid, busy and spectacular CKs can be,
displaying a huge variety of different details.

Absolutely NECESSARY for you to get, what we're talking about, is TO ENLARGE
THE THUMBNAIL PHOTOS by clicking,
to fully enjoy that extravaganza and not missing out by skimming quickly the
page.

NWA 6824 is weakly shocked with S2.
And it is very fresh and unweathered with a weathering grade of W1.
We had also even slightly fresher ones, W0/1 among our palette of CKs,
though they were not so dazzling like this jewel now.
Note also the great snakeskin of fusion crust on the backside of the
endcuts:
http://www.chladnis-heirs.com/specials/nwa6826-688.5g-end3.JPG


Well, you might be worried about the costs for such an overwhelming
material,
and finally our Moroccan friends and colleagues raised the issue here on the
list 
of the dramatically changed situation, which is going to happen since a
longer while in the NWA-scene.

But - we are proud to tell you, that we decided to make today an offer,
which regarding the quality,
should beat out the price levels, which you are used to commonly see for the
CK-group;

and priced all specimens - from the centerpiece of your carbonaceous-section
to the meaningful reference partslice,
all grinded and polished,
at one price, a reference to the Golden Times of NWA

of 25$/g.

With a tkw of 1.3kg we hope, that nobody has to miss out and we can launch
this Special earlier than usually.
Nevertheless, as always, it would be very helpful, if you would send us a
wish-list with the ranking of your desired specimens,
to avoid delays and traffic jam.

Once again, here they are now:
http://www.chladnis-heirs.com/specials/special-nwa6826.html 


Enjoy!
Martin  Stefan

Chladni's Heirs
Munich - Berlin
Fine Meteorites for Science  Collectors
http://www.chladnis-heirs.com



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[meteorite-list] AD: Special: Multicolor Ragland-like Chondrules-Galore - NWA 6864 L3.4

2011-06-23 Thread Chladnis Heirs
Dear collector-friends,

back from the Ensisheim fair, we're thinking, what we could offer as a
consolation for those, who had to stay home and are now longingly watching
the pictures of the show.
So we were pondering, and picked for our little Special a brand-new
unequilibrated L-chondrite:  NWA 6864.

Here you are, after a longer absence of 3ers among our specials - a really
pretty one, isn't it?

http://www.chladnis-heirs.com/specials/special-nwa6864.html

Look how densely the chondrules are sitting together in this meteorite.
All sizes, from sparse giants to tiniest dwarves, freely mixed in a happy
clutter.
With W2 somewhat fresher than the average.
But the main eye-catchers are - exactly: The Colors!
The full spectrum is given by the colors of the individual chondrules.

This L3.4 strongly resembles historic Ragland,
we even think, that it is a slight idea more beautiful 
(biased as our taste is).

Affordable it is, slices for every purse available.

Just the right stone at the right moment.

A very fine unequlibrated chondrite, of a special aesthetics,
containing the germs for our planets -
not only for the chondrules-lovers.

Just Enjoy!

Yours,
Stefan  Martin

Chladni's Heirs
Munich - Berlin
Fine Meteorites for Science  Collectors

http://www.chladnis-heirs.com


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Re: [meteorite-list] Buyers BEWARE!!!!

2011-06-28 Thread Chladnis Heirs
Short disclaimer:

As we see our lunaite NWA 4881 and our shergottite NWA 4925 involved,
only the quick remark, that we don't know, who this person is

and that these mounts have nothing to do with our original display cases,
which you are used to know for years from various offerors and shops around
the world.

Examples:
http://www.chladnis-heirs.com/moonrock2.jpg

http://www.chladnis-heirs.com/boxes/Mars-XS-1.jpg


(Anyway, I can't see any cleverness of that seller to re-pack the samples
into other boxes,
as the original boxes yield the same or higher results on ebay...).


Best!

Martin


Martin Altmann  Stefan Ralew

Chladni's Heirs
Munich - Berlin
Fine Meteorites for Science  Collectors 

http://www.chladnis-heirs.com




-Ursprüngliche Nachricht-
Von: meteorite-list-boun...@meteoritecentral.com
[mailto:meteorite-list-boun...@meteoritecentral.com] Im Auftrag von Dan
Furlan
Gesendet: Dienstag, 28. Juni 2011 17:24
An: met-list
Betreff: [meteorite-list] Buyers BEWARE

Hello all, unfortunately I have found another person on ebay who is
selling underweight lunar and martian material.  His ebay ID is
spaceterrain4sale and his first name is Ariel.  He is advertising his
mounts at 24mg each at the time i purchased.. i purchased a whole
bunch from him for around 8.00 each thinking he was an honest seller
and i liked the display cases they came in.  When i got the items they
looked very small... I decided to break open one of the mounts and
weigh it on my diamond scale.  IT ONLY WEIGHS 7 MG and this was the
biggest piece.. if you are bidding on any of his items make sure you
understand he is misleading people in the weight he is stating.  his
ebay ID is spaceterrain4sale just to let everybody know.  I am talking
to him now about getting a refund for all the mounts i bought another
meteorite dealer ripping people off on ebay.. what a waste.. if he
doesn't agree to refund me my money i will open a claim against him
with paypal... i noticed on his new listings he is not stating the
weight anymore but I am talking about the items i purchased and the
listings at the time of when i purchased the items.. please beware of
this guy.

Daniel Furlan
dealer and collector
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[meteorite-list] AD: Special: Truly baffling sensational Howardite - NWA 6709 - absolutely stunning and very fresh.

2011-07-20 Thread Chladnis Heirs
Dear meteorite community,

with this Special we have to introduce to you an enormous oddity. 
It is about a HED-meteorite of a kind, which we hadn't ever seen before in
our careers before.

It came in two stones, one of them was covered with a lush fusion crust,
wonderfully structured by thick and oriented flowlines.
And in some parts, that very crust displayed a gloss and a shine, iridescent
in all colours of the rainbow;
an effect, reminding almost to bismuth! 

Please take a look to the photos, where we tried to captured the effect:
http://www.chladnis-heirs.com/new-meteorites/nwa6709.html


The interior was no less a riddle for us.
The distribution and sizes of the various fragments and clasts were unlike
we had seen in any polymict HED before.
A variety of clasts is of a kind, like we never had recovered in any Vesta
meteorite. Please take a closer look to the slices and you will share our
surprise.

And a very few of these clasts develope due to their microscopically
lamellae-texture a fire like an opal, if turned around in the light.
The response to a magnet is very inhomogeneous within the slices, 
although no differences are visible to the eye
and all in all the interior has a somewhat dull yellowish tint - although
the material is very fresh - and that tint and the circumstances made us
initially think, it might be diogenitic.

It is under classification at Dr. Anthony Irving and the values say, that it
is a shocked howardite.

We crafted now a set of polished sliced of all sizes, to share this
exceptional material with you.
Please acknowledge that we have kept the price, despite of the for us so
unique properties of the material, well affordable,
for everybody staying able to add a specimen of this truly exceptional stone
to his collection.
And an addition it is, also for the most experienced veteran collector.

Earlier today we had published the Special in the German forum, therefore
not so many specimens are left.

For the largest slice we can offer a discount as it is the only one, which
isn't coplanar.

And finally, the specimen named piece #2, which we chose to illustrate
best that rainbow-bismuth-gloss of the fusion crust on the first linked
page, is available too. It weighs 119.2g and we're accepting offers.

Here you are now:
http://www.chladnis-heirs.com/specials/special-nwa6709.html


Best Regards,
Stefan  Martin

Chladni's Heirs
Munich - Berlin
Fine Meteorites for Science  Collectors

http://www.chladnis-heirs.com



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[meteorite-list] Statement

2011-08-05 Thread Chladnis Heirs
Hello list members,

Here is our statement regarding the allegations Mr.Jain published here in
that place:

http://moonrocks.de/statement.html


Kind regards,

Martin Altmann  Stefan Ralew


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[meteorite-list] Test - ignore

2009-12-05 Thread Chladnis Heirs
Tests are boring.

Meteorite collection in Switzerland...
http://www.youtube.com/watch?v=tHQn7VNLUJI


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[meteorite-list] Was Test - ignore - the meteorite collection in the Mysty Park, Interlaken

2009-12-06 Thread Chladnis Heirs
Hello,

we were asked, what for a meteorite display it could be in that
youtube-clip, we filled our test-posting with:

http://www.youtube.com/watch?v=tHQn7VNLUJI

These are the remainders of the once most important (and perhaps still most
important) meteorite collection of Switzerland:

The former collection of the Bally-Prior museum in Schoenenwerd, Canton
Solothurn, 
(where Rolf Buehler was also curator - author of the still best meteorite
book in German language).
Bally-Prior was a fabricant of shoes.
In the end the meteorite collection comprised 500 historic meteorites from
more than 70 countries.

The museum housed also one of the most important mineral collections of
Switzerland.
Was financed by an private foundation,
but the museum went more or less bankrupt.

To restore and to maintain the museum and the collections in the end a
relatively modest amount was missing, approx 450.000$.
A sum the Suisse state obviously wasn't willing to pay.

So unbelievable but true: the mineral  meteorite collections were dissolved
and hawked 5-6 years ago!

Museums and universities had a preemption to buy before the private
collectors.
All museums and universities failed in taking over the meteorite collection,
even the ETH Zurich, whereto Bally-Prior had donated endless mineral
specimens and whole collections.

So afterwards a private person bought the meteorite collection.

Maybe one can say, that with that failure to secure the Bally-Prior
meteorite collection for the public and for research, Suisse meteorite
history hit rock bottom.
Only one similar grave case comes into our minds, the mistake not to have
held Zeitschel's collection, once largest private collection in the World,
in Germany - but that was in the 1980ies.
 
The private buyer gave a part (most?) of the collection on loan to that
place, where the video was taken.
Well, maybe not an ideal place, but at least they are on display.
It's a kind of a Disneyland once created by Europe's most famous ufologist,
Erich von Daeniken.  - the Mysty Park in Interlaken, Canton Bern.

Side remark - we had these discussions about laws, meteorites as natural or
cultural heritage (and a museum collection is for sure a cultural heritage
in the terms of the UNESCO-Convention of 1970) etc. - 
Well, if one regards this case, doubts can rise, whether meteorites in
Switzerland really are objects of cultural meaning, scientific importance
and public interest and if the respective laws about such objects found can
be applied on meteorites.

Mistakes are made to learn from them.

Have a fine Sunday,
Martin

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[meteorite-list] AD: Unique and Uncommon new Martian - NWA 5990

2009-12-10 Thread Chladnis Heirs
Dear collectors,

today it is highest time to introduce our new – not only in our eyes – quite
sensational planetary recovery.
NWA 5990. A new Martian, remarkably distinct from the so far known finds.

Before cutting it was a relatively small stone of only 59 grams, coated with
an unweathered black fusion crust with some indications of flight marks,
which seemed to have spalled of on one corner by impacting the ground. The
stone felt somewhat heavier than one would expect for a planetary one.

Here you have a picture of the intact mass:

http://www.chladnis-heirs.com/uncut-mainm-klein.jpg


The first cut then revealed the outstanding nature of that small stone.
The overall fresh appearance of the exterior was trumped by the pristinely
looking cross section and you may comprehend our sudden elatedness, if you
take a look at this picture of the unpolished cut surface:

http://www.chladnis-heirs.com/6.995g-end-kl.jpg


As you can see, that stone looks simply different from all other Martians we
know. 
Well, with the numerous partially blackened olivines, one could tend to
think into the direction of a lherzolithe, but it turned out, that the stone
contains by far too much plagioclase to be lherzolithic. The grain size
however fits to a diabase.


That material is currently under analyses with a high priority at Dr.Irving,
Dr.Herd et al. - and perhaps as early as in January an abstract will be
already available. 
Therefore we beg for your understanding, that we can't forecast the exciting
results, but have to leave the first publication to the researchers, avidly
working on that surprising material.
Maybe the one or other being already the proud owner of a slice will share
his/her observations here in this thread with us instead.

And here starts our dilemma - you may wonder, why we go public with this new
Martian already without being able to name and explain the particularities
and specifics of this new material - especially so shortly before a paper is
scheduled; also it is planned to introduce the stone at the next Lunar 
Planetary Science Conference in Houston in beginning March..

Well the reason is simple - until then the material will have been
completely gone and you would have to miss out that important new Martian.

As the tkw was so low and this unique meteorite has such a scientific
brisance, we had of course to address firstly to research institutes, like
we had to do with NWA 5789 too. Afterwards we supplied the Martian
enthusiasts from our address book (and we cordially recommend and invite the
planetary specialists to contact us, if they want to be added there too).

So in the end and at present there are only two specimens left!


Half a fullslice with fusion crust.   2.338g 
Price is 1600$/g

http://www.chladnis-heirs.com/2_338g.jpg


And a crusted partial endcut. 1.908g 
at 1500$/g

http://www.chladnis-heirs.com/1_908g_endcut.jpg

http://www.chladnis-heirs.com/1_908g-end2.jpg



Else there would be only these two pieces, but they are on hold for a
museum, the negotiations aren't finished yet.
So most probably they won't be available.

A cap of the stone with a lot of crust and flight marks.
(Largest intact piece, hence depending on definitions the main mass):
http://www.chladnis-heirs.com/6.955g-end2-kl.jpg

http://www.chladnis-heirs.com/6.995g-end-kl.jpg

 
And a partslice.
http://www.chladnis-heirs.com/2_055g.jpg


If these specimens will have been gone, not a single grain of the stone will
remain available.


We hope you're as fascinated as we are from that new Christmas greeting from
the Red Planet and wish you a peaceful time.

Stefan Ralew  Martin Altmann

Chladni's Heirs
Munich - Berlin
Fine Meteorites for Science  Collectors
http://www.chladnis-heirs.com/





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[meteorite-list] Addendum: NWA 5990 already in the MetBul Database! Details there.

2009-12-10 Thread Chladnis Heirs
Good Afternoon again!

A collector found out, that a preliminary report of the new Martian is
already available in the database!
Must have been implemented right these very days.

So we can unveil a little more!
Find a description and the data here: 

http://kuerzer.de/NWA5990

Many thanks,
For having told that to us Pallasit!

Stefan  Martin



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Re: [meteorite-list] AD: Unique Martian NWA 5990 - Smaller Pieces desired?

2009-12-13 Thread Chladnis Heirs
Good Afternoon list,

we received several emails with list-members expressing their disappointment
or sadness that they'd not able to add this really exciting Martian material
to their collection, because the offered specimens are somewhat too mighty.

Aye, it's a dilemma. We had almost no small cuts, neither many crumbs broke
loose while cutting and on the other hand, with such important material of
such a low tkw, we feel always somewhat guilty, if we produce too much cut
loss. 

Indeed it is somewhat unfair..
Well, in a Christmassy mood, what do you think about the idea, to sacrifice
one slice, in cutting it down to more budget-friendly servings?
A kind of a pool - if enough collectors will raise their fingers, so that a
complete slice can be moved, we could slaughter it, perhaps with a 100/g
spread to compensate the cut loss and the pain. 
That said (and of course having in mind, that it's quite the most inadequate
time of the year for offering such a bomb - but most of you know our often
liberal payment policy),

just send a PM and we will see and try our best.

Winterly Greetings,

Stefan  Martin

Chladni's Heirs
Munich - Berlin
Fine Meteorites for Science  Collectors
http://www.chladnis-heirs.com/



-Ursprüngliche Nachricht-
Von: meteorite-list-boun...@meteoritecentral.com
[mailto:meteorite-list-boun...@meteoritecentral.com] Im Auftrag von Chladnis
Heirs
Gesendet: Donnerstag, 10. Dezember 2009 22:36
An: Meteorite-list@meteoritecentral.com
Betreff: [meteorite-list] AD: Unique and Uncommon new Martian - NWA 5990

Dear collectors,

today it is highest time to introduce our new – not only in our eyes – quite
sensational planetary recovery.
NWA 5990. A new Martian, remarkably distinct from the so far known finds.

Before cutting it was a relatively small stone of only 59 grams, coated with
an unweathered black fusion crust with some indications of flight marks,
which seemed to have spalled of on one corner by impacting the ground. The
stone felt somewhat heavier than one would expect for a planetary one.

Here you have a picture of the intact mass:

http://www.chladnis-heirs.com/uncut-mainm-klein.jpg


The first cut then revealed the outstanding nature of that small stone.
The overall fresh appearance of the exterior was trumped by the pristinely
looking cross section and you may comprehend our sudden elatedness, if you
take a look at this picture of the unpolished cut surface:

http://www.chladnis-heirs.com/6.995g-end-kl.jpg


As you can see, that stone looks simply different from all other Martians we
know. 
Well, with the numerous partially blackened olivines, one could tend to
think into the direction of a lherzolithe, but it turned out, that the stone
contains by far too much plagioclase to be lherzolithic. The grain size
however fits to a diabase.


That material is currently under analyses with a high priority at Dr.Irving,
Dr.Herd et al. - and perhaps as early as in January an abstract will be
already available. 
Therefore we beg for your understanding, that we can't forecast the exciting
results, but have to leave the first publication to the researchers, avidly
working on that surprising material.
Maybe the one or other being already the proud owner of a slice will share
his/her observations here in this thread with us instead.

And here starts our dilemma - you may wonder, why we go public with this new
Martian already without being able to name and explain the particularities
and specifics of this new material - especially so shortly before a paper is
scheduled; also it is planned to introduce the stone at the next Lunar 
Planetary Science Conference in Houston in beginning March..

Well the reason is simple - until then the material will have been
completely gone and you would have to miss out that important new Martian.

As the tkw was so low and this unique meteorite has such a scientific
brisance, we had of course to address firstly to research institutes, like
we had to do with NWA 5789 too. Afterwards we supplied the Martian
enthusiasts from our address book (and we cordially recommend and invite the
planetary specialists to contact us, if they want to be added there too).

So in the end and at present there are only two specimens left!


Half a fullslice with fusion crust.   2.338g 
Price is 1600$/g

http://www.chladnis-heirs.com/2_338g.jpg


And a crusted partial endcut. 1.908g 
at 1500$/g

http://www.chladnis-heirs.com/1_908g_endcut.jpg

http://www.chladnis-heirs.com/1_908g-end2.jpg





Else there would be only these two pieces, but they are on hold for a
museum, the negotiations aren't finished yet.
So most probably they won't be available.

A cap of the stone with a lot of crust and flight marks.
(Largest intact piece, hence depending on definitions the main mass):
http://www.chladnis-heirs.com/6.955g-end2-kl.jpg

http://www.chladnis-heirs.com/6.995g-end-kl.jpg


And a partslice.
http://www.chladnis-heirs.com/2_055g.jpg


If these specimens will have been gone

Re: [meteorite-list] Ordinary chondrites - rarest to the most common classes

2009-12-16 Thread Chladnis Heirs
Indeed,

it's for the first time, that I read that R-chondrites are included in the
OC-group. If so, why exactly them and not the K-chondrites, the Carbonaceous
from grade 3-6, the ungrouped and the enstatite chondrites too?
 
valuable type of OC from a 
scientific perspective is petrologic type 3.00-3.01

Where one has to say, that it's maybe too early to say that,
Because the classification with decimal places, (even with two!), is a
relatively new occurrence - most classifiers seems still to prefer to use a
simple 3 - so that in case, there are still a lot known type-3ers awaiting
to be revisited regarding the degree of their (un)equilibration.

But I agree - Ordinary is a somewhat misleading term,
- as the ordinary chondrites have told us most about the origin and
formation of the solar system, the planets and ourselves, more than any iron
or any lunar rock!

Keep that always in mind, if you are tempted, now in the end of the
desert-era and the decreed end of meteorite finding in so many countries,
with all their weird and fancy exotic types, to wrinkle your nose about the
ugly ordinary 25$-a-kilo-chunk from NWA-wonderland!
Rare as brilliants they are - and they were our beginnings!

Happy holidays to all!
Martin


-Ursprüngliche Nachricht-
Von: meteorite-list-boun...@meteoritecentral.com
[mailto:meteorite-list-boun...@meteoritecentral.com] Im Auftrag von Jeff
Grossman
Gesendet: Mittwoch, 16. Dezember 2009 11:33
An: Meteorite-list
Betreff: Re: [meteorite-list] Ordinary chondrites - rarest to the most
common classes

I agree with Doug... the rarest and most valuable type of OC from a 
scientific perspective is petrologic type 3.00-3.01, from any of the 
chemical groups.  Only one is known... Semarkona.  If we take a more 
expansive definition of ordinary chondrite than most of my rather 
conservative colleagues are normally willing to accept, I would say that 
the rarest group of OCs is the R chondrites (only ~100 are known and 
many of those are paired).  In addition, a number of unique ungrouped 
meteorites are OC-like.  But again, I don't know of any colleagues who 
agree with me that R chondrites are in the OC class. [I would say that 
the OC class has two clans, the H-L-LL clan and the R clan].

Jeff

Mexicodoug wrote:
 Hi Melanie and thanks for the enthusiasm you add to the list ...

 Here's a high to low sorting of the ordinary chondrites, for over 
 32,000 meteorites:

 22.0% L6 (most common)
 19.9% H5
 12.9% L5
 12.3% H4
 11.5% H6
 7.8% LL5
 4.2% LL6
 3.3% L4
 2.2% H3
 2.0% L3
 0.8% LL4
 0.8% LL3
 0.1% L7
 0.1% LL7
 0.03% H7 (least common)

 But this common and rare is a misleading label. That is a harder 
 question if you look too closely at the deails and consider 
 inhomogeneous and brecciated ordinary chondrites. That can all become 
 somewhat unique if you ask the right person. Then there are the motley 
 crew of ungrouped ordinary chondrites where it is hard to generalize. 
 Some may be a weak classification while others might truly be weird 
 (rare).

 Just a few notes: the H7, L7, LL7 types are not widely used in the 
 literature and border on impact melts, so I'd take them with a grain 
 of salt unless someone goes postal on me in which case they are right 
 in whatever they say. The way I listed these, the meteorites are 
 counted by the lowest number and won't show up in the higher thermal 
 (metamorphosed) levels. In other words, for example, an LL3.8-6 is 
 counted with the LL3's.

 If you have a special meteorite, it can sometimes be a rarer type if 
 you start to split hairs, like H3.8 instead of just grouping it within 
 the H3's, but there is some degree of arbitrariness to this. The 
 tendency is that more virgin Solar system stuff (closer and closer 
 3.00) is more special and like a holy grail (rare in a sense) to 
 some who study that - since it is more representative of the original 
 material before water and heat were added and did their thing. From 
 hat we can try to get the proof we need to work out early formation 
 processes and theorize on the related dynamics happening. By this 
 logic, and considering it is a very studied meteorite, the precious 
 meteorite SEMARKONA (LL3.00 or is it 3.01 :-)), a witnessed fall from 
 India, is rather unique being the only one with that 3.00 
 classification, which makes it super intact since formation and 
 especially interesting to experts, and most notably Dr. Jeff Grossman 
 who reviewed and updated its classification upon careful study.

 By another measure, the common ordinary chondrite, L5, Canadian 
 witnessed fall, VILNA, is one of those very few special meteorites 
 that was imaged during atmospheric entry and a precise orbit was 
 determined. It was not too far from Buzzard Coulee, and what makes it 
 even more special is that it was classified from a (although witnesses 
 heard pieces whizzing around) 94 milligram fragment with fusion crust. 
 The only other specimen found was a 48 milligram piece! This 

[meteorite-list] AD: Special: Tribute to Vesta - Four different new and excellent Eucrites!

2011-10-20 Thread Chladnis Heirs
Dear Collectors,


our autumn season we will start with a truly mighty Special.
These weeks and months we can say, that we all are captivated by the
incredibly fascinating and sometimes almost shocking pictures the Dawn probe
transmits through the outer space on our screens from this New World called
Vesta.
And with each new sight and capture for us meteorite lovers the eagerness
grows more unendurable, when finally the first mineralogical data will
arrive - and whether then we meteorite collectors could say to the hare: we
are the hedgehogs; We were already there.

So as a tribute to Dawn and a salute to Vesta we will reveal four different
new eucrites all at once,
each of them of such a discrete excellence and also of a quality, that we
can imagine, that it won't be that easy to make a decision, which specimen
to pick, from the kaleidoscope, we try to demonstrate with the diversity of
the Eucrite group.

Let us begin:


NWA 6970

With a tiny tkw of 15.5g only the smallest. A moderately shocked polymict
one, which exhibits an extremely busy small scale tessellate.
A very dense and compact material, polishing excellently. Internally fresh,
with fine spots of colourful inclusions.
http://www.chladnis-heirs.com/specials/special-nwa6970.html



NWA 6971

Displays gorgeous cubistic shock patterns! Straight and extremely angular
shock lines, triangular shock veins and whole slightly shock darkened
polygons - and that all in a perfect contrast to an almost Dho 007 looking
eucritic matrix. Glossy black fusion crust preserved.
http://www.chladnis-heirs.com/specials/special-nwa6971.html



NWA 6972

Disguises as a lunaite. As you can see it plays a mimicry of a fine
fragmental anorthosic breccia. 
(And among these NWA 6972 chose the prettiest ones). A high diversity of
clasts and inclusions; Highly shocked and Stefan applied a wonderful
polishing. Note the black and granular fusion crust on the endpieces!
http://www.chladnis-heirs.com/specials/special-nwa6972.html



NWA 6974

Elitist extravagance.

The climax of our special.
A stone like we like it, cause it makes any words obsolete.
The Covergirl for any glossy magazine about meteorites or about Vesta.

A low shock allowed these different lithologies to merge together to that
masterpiece.
Overwhelming variety of inclusions. Some weird, some black like coal.
Holding our breath now, we only still mention, that it wears a fresh black
skin of fusion crust all around (and while we are writing, we recognize,
that the price we chose is maybe a little bit too shy).
http://www.chladnis-heirs.com/specials/special-nwa6974.html




Enjoy the Art of Vesta!
Yours,
Stefan  Martin

Chladni's Heirs
Munich - Berlin
Fine Meteorites for Science  Collectors

http://www.chladnis-heirs.com






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[meteorite-list] AD: Special: The new, fresh and very peculiar Martian meteorite NWA 6963

2011-11-09 Thread Chladnis Heirs

Dear collectors,


Today we have once again the especial pleasure to continue our serial of new
finds 
of unpaired and extraordinary Martian meteorites.

It's about the most recent Martian recovery of this year, which has found
its way already as NWA 6963 into the Meteoritical Bulletin.

Again it is an unusually fresh material. NWA 6963 owns a very good
glossy-black fusion crust and the interior presents itself to be absolutely
unaltered by terrestrial weathering.
What is remarkable about NWA 6963 is that it doesn't belong to the olivine-
and olivine-orthopyroxene-phyric main group, but that we have here a basalt,
which resembles, if anything, Shergotty.

Already the first long- and eagerly awaited cut revealed the fantastic
texture of this Mars rock. 
The crystallization pattern consist of a a dense and angular lattice of
broad spindles and bars, much more distinctly and clearer pronounced than
that one
of Zagami or Shergotty, of which some of you might feel reminded of.
And other than these, which are gray, does NWA 6963 attend upon us with an
accented greenish tint,
which turns that shergottite into an acutely aesthetical delight.  

Classified was NWA 6963 this time by Dr. Carl Agee at the university of New
Mexico.
NWA 6963 is highly shocked, so that the plagioclase is completely
transformed into maskelynite.
The bulk composition is 60% pyroxene, 35% maskelynite, 2% ulvöspinel.
Additionally it contains melt pockets with traces of merrillite, pyrrhotite
and chlorapatite.
Of course no abstracts are on hand yet, according to reports the composition
of the pyroxene shall be very similar to that of Shergotty, and hearsay
tells,
that the bulk chemistry could point also in the direction of NWA 480/1460.

Therefore a lot of research is still to do and with that NWA 6963 the
scientist certainly will be occupied for quite a while, like it was
with the previous, each for its own very special Martian meteorites, where
we had the possibility to introduce them here on the list,
and so we can look forward to thrilling results and publications still to
come!

Here you are now.
All specimens down to 1.6g do have minimum one fully fusion-crusted edge.
The smaller ones sometimes and here and there a few specks of crust.
Note also, that this time, seen the news value, the freshness and the
specialty of that amazing material among the other Martians and regarding
the overall price level of the Martians of the last 2 years,
we kept the offer tempting:


http://www.chladnis-heirs.com/specials/special-nwa6369.html



Enjoy and Success!

Stefan  Martin 

Chladni's Heirs
Munich - Berlin
Fine Meteorites for Science  Collectors 

http://www.chladnis-heirs.com







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[meteorite-list] AD: Addendum: Fusion crust share on the smaller slices of the pretty sensational new Martian

2011-11-10 Thread Chladnis Heirs
Dear collectors,

because some of you asked, only that short additional information,
also because it isn't so well visible in the photos:

That is the approx. fusion crust share of the still available smaller
specimens,
in % of the circumference:

0.508g 5%
0.603g 10-15%
0.653g 15-20%
0.731g 30%
0.978g 45%
1.018g 40%

Find them here:
http://www.chladnis-heirs.com/specials/special-nwa6369-2.html


All the Best!
Martin  Stefan

Chladni's Heirs
Munich - Berlin
Fine Meteorites for Science  Collectors 

http://www.chladnis-heirs.com




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[meteorite-list] AD: Special: NWA 6659 prov. - Superior Lodranite

2011-11-16 Thread Chladnis Heirs

Dear meteorite friends,


in our weekly Special we're able this time to present you a wonderful
dainty:  NWA 6659 - a Lodranite!

Lodranites are counted among the absolutely rarest classes a meteorite
collector can have in his cabinet and a meteoricist in his lab.
Currently the Meteorite Bulletin Database accounts for only 32 lodranitic
numbers with a combined weight of 9.39kg (15 of them with 1.14kg yielded the
Antarctic campaigns of the last 35 years).  And 9 numbers not otherwise
specified as belonging to the acapulcoite-lodranite family with 0.33kg 
(7 Antarctics) - making the lodranites to a much rarer type than any lunar
meteorite.

Let us say as long-time established meteorite offerers, that it was the
NWA-complex of the recent decade, which brought the lodranites at all in the
range of the collector and a certain variety of finds into the research
institutes. A check of our global price compilation of the season ten years
ago only (660 different meteorites, 92 offerers - currently available in the
German meteorite forum), gives, that the only chance to get a lodranite was
then to acquire micromounts of Lodran, priced at an average of 38,400$ a
gram and that among the related acapulcoites, the collector had only the
choice between Acapulco (average 1408$/g) and Monument Draw (1016$/g).

Lodranites and acapulcoites share common ground and are generic relatives
from the same parent body, which seems to have had consisted of a CM or
CI-like precursor material. The main differences between these types is the
lack of plagioclase in the lodranites and the larger grain-sizes than the
acapulcoites display, hence indicating that lodranites underwent during
their melt phase higher temperatures and a different cooling period,
stemming from deeper layers than the acapulcoites.
However, as enigmatic that group perhaps still might be - it are just the
very recent years with these new desert finds, which lead science to develop
a better understanding of the composition and the complex thermal history of
the acapulcoite-lodranite parent body.
A perfect overview of the brand-new models and hypotheses you will find on
David Weir's meteorite studies pages.

The perhaps a little provocative title of this Special we chose, because
most lodranitic specimens in our collections are recruited from the large
pairing group, which was revised from ACAP to LOD and where we once all
tried to put the numbers together here on the list (NWA 2565/2714/2866
seqq.) 
And we regard NWA 6659 as definitely more comely.
It is better preserved than the old group, which had weathering grades of W3
and W3-4.
Not only the crystals of NWA 6659 are still relatively fresh-looking - it
has even here and there some metal grains and of course:  
Yes - the so highly desired Triple Junctions superabound.

All slices were grinded and polished successively with 6 different grits;
and you find them here:

http://www.chladnis-heirs.com/specials/special-nwa6659.html


Regarding the statistics from above, keeping in mind, that the Great Desert
Area is coming to an end and emphasizing that we price NWA 6659 at the
lowest edge of the lodranite spectrum, we think, that these specimens are
not only of highest interest for the advanced collector, but would
wholeheartedly commend them as an excellent choice also for the beginning
meteorite enthusiast, as one-and-only specimen for having an perfect
representative, once and for all, of that fascinating and so exceedingly
rare class.


Best regards,
Stefan  Martin

Chladni's Heirs
Munich - Berlin
Fine Meteorites for Science  Collectors 

http://www.chladnis-heirs.com





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[meteorite-list] AD: ALL slices do have METAL Flakes - of the Superior Lodranite NWA 6659

2011-11-16 Thread Chladnis Heirs
Hello again,

And sorry for the little explanation,
but for not all jumping on the 5.013g and the 4.397g-slices, respectively
being disappointed, that those are gone:

ALL slices do have the same amount of metal flakes and blebs!

It's only not so well visible, as we photographed only two with an angle of
the light, that the metal flakes are reflecting. 
All slices are the same wonderful!

http://www.chladnis-heirs.com/specials/special-nwa6659.html



And when we are just at addendums...

The unpaired new fresh Martian with that fantastic texture, where we perhaps
made the mistake to introduce it with too soberly chosen attributes last
week.   NWA 6963.
There we would invite those, who'd still need a smaller sample than those
slices currently left,
to inform us, which weight they prefer - for us to pre-plan, what and how we
still have to cut or to divide into smaller sections.

http://www.chladnis-heirs.com/specials/special-nwa6369-2.html

and 
http://www.chladnis-heirs.com/specials/special-nwa6369.html


Many thanks in advance!
Martin  Stefan

Chladni's Heirs
Munich - Berlin
Fine Meteorites for Science  Collectors 

http://www.chladnis-heirs.com







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[meteorite-list] AD: Special: Extremely aesthetical new H-Metachondrite NWA 7024 - and an Eucritic Surprise NWA 6969

2011-11-27 Thread Chladnis Heirs
Dear meteorite friends,

Stefan has prepared for this weekend Special again two enchanting gems.

NWA 7024
is a new H-metachondrite.  About metachondrites, in connection with type-7,
PACs and even melts, we spoke detailed and it was discussed on the list,
that this concept offers a higher taxonomic clarity, when we introduced the
first L-metachondrite one year ago.
Therefore you find it in the list-archives and we haven't to recur.
(And in case, David Weir will be as helpful as always:
http://www.meteoritestudies.com/ )

NWA 7024 is now a rock, that underwent a metamorphosis to such a degree,
that none of the chondrules of the precursor material prevailed and that a
complete recrystallization took place.
Well, and this time, especially if we compare it to the very few known
H-metachondrites, let us demonstrate additionally a completely
non-scientific attitude:  It is a beautiful meteorite!  
Internally very fresh, the photos hardly can do justice to the aesthetics of
the specimens. Just note only the shape and the distribution of the
iron-flakes - doesn't it resemble Itqiy, does it?
And Stefan has applied an especially fine finish to the surfaces; so that
all in all, we really don't have to accentuate the rareness of the material
or the importance for the systematics of your collection. It is simply again
a case for the high-end collector, two whom not size matters but the
unwontedness and the classiness of a meteorite - a case for his casket of
remarkable space jewels.

http://www.chladnis-heirs.com/specials/special-nwa7024.html



As we chose a moderate price and because the number of specimens is so
limited by the small tkw, that unavoidably some collectors will miss out,
let us add a second fantastic meteorite:

NWA 6969,
a wonderful little eucrite!

Here already the specimens:
http://www.chladnis-heirs.com/specials/special-nwa6969.html


That marble came as a complete, fully  freshly crusted stone.
As you can see on the backsides of the endcuts best, that fusion crust was
so atypical, that for the experienced specialist this little marble was
definitely too tempting to let it pass by!
Cut it revealed to be a monomict eucrite with a gorgeous brecciation and
shock vein pattern.
The basalt is looking not that common too - so imagine, what for tricks you
can play e.g. with the 0.584g or the 0.494g in showing it to the meteorite
connoisseur, when he visits you, in asking him for his expert opinion.


Have a fine Sunday,
Stefan  Martin


Chladni's Heirs
Munich - Berlin
Fine Meteorites for Science  Collectors

http://www.chladnis-heirs.com



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[meteorite-list] AD: Special: NWA 6966 prov. - a Classy and Elegant new Eucrite

2011-12-07 Thread Chladnis Heirs

Dear Meteorite Friends

Fittingly to the season we'll introduce today to you a very fine new
eucrite:   NWA 6966 prov.

Some of you might remember the number,
as the stone before cutting was displayed due to its aesthetics already in
Paul's MPOD before:
http://www.tucsonmeteorites.com/mpodPic.asp?DD=10/28/2011WYD=


NWA 6966 came as strongly flight oriented stone of 1105 grams, unfortunately
with a not fully complete fusion crust, but with some areas missing - else
it would have been a remarkable and true museum's specimen.
Nevertheless it was of a fine fresh appearance and the fusion crust
exhibited radial flow lines.

So the slicing was well worth, as the outcome resulted in, in our opinion,
very desirable specimens of attractive dimensions.

NWA 6966 presents itself as a weakly shocked polymict eucrite.
Most striking to the eye are the basaltic, typically freckled large
eucrite-nests, emerging from the especially fine grained matrix.
Other than the wilder polymict ones, the inventory of the clasts is more
limited and the colors and tints more monochrome,

.bestowing upon that material an especially elegant and wintery noblesse.


Here you find now the fine-grinded, fusion crusted and moderately priced
slices:

http://www.chladnis-heirs.com/specials/special-nwa6966.html


Greetings out of the first snow,
Martin  Stefan

Chladni's Heirs
Munich - Berlin
Fine Meteorites for Science  Collectors

http://www.chladnis-heirs.com




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[meteorite-list] A Masterpiece of the new Martian fall Tissint

2012-01-17 Thread Chladnis Heirs
Dear list-members,

let us contribute to the discussion about that new Martian fall, which
certainly belongs to one of the most exciting events in all our
collector-lives, in sharing some pictures of a stone, which is the most
amazing example of this new fall, we have seen so far.

The specimen is a completely fusion crusted individual with a weight of 147
grams.
The pristine and extremely clean crust displays a fantastic deep-black
gloss.
Furthermore it shows indications of a slight orientation, if you note the
lipping running over the edge to the left.

http://www.chladnis-heirs.com/new-meteorites/tissint.html


Simply enjoy!

Stefan  Martin

Chladni's Heirs
Munich - Berlin
Fine Meteorites for Science  Collectors

http://www.chladnis-heirs.com



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[meteorite-list] Phenomenology of Tissint Individuals

2012-01-19 Thread Chladnis Heirs
Dear Listers,
 
As if the complete Tissint individuals wouldn't be all wonders - there are
some especial surprises among them..
What do you think about that one?
 
http://www.chladnis-heirs.com/new-meteorites/tissintkl.jpg

 
Best!
Stefan  Martin

Chladni's Heirs
Munich - Berlin
Fine Meteorites for Science  Collectors

http://www.chladnis-heirs.com




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[meteorite-list] Special: AD: New Mars-Fall Tissint - Polished Fullslices!

2012-01-26 Thread Chladnis Heirs
Dear community,


Now we all were occupied with admiring the fragments and the rare
individuals that new epoch-making fall yielded; we studied the exterior,
were amazed about the variety of different fusion crusts, took a glance on
the interior by means of broken sides or crust-free fragments.
Now it is highest time to subject Tissint to the other viewing habits we are
used to
- and here we are proud to present now the first masterly prepared slices:

And what for slices!

http://www.chladnis-heirs.com/specials/tissint.html


In principle here could end our Special - in leaving you alone in your awe.


Well worth it was, that we pushed away our twinge of conscience to slice up
one of the scarce perfect individuals, any collector would rip his arm off
for.  Look, how we were rewarded.

See those fantastically pastel green olivine crystals, which strongly remind
us of those in NWA 5789.
Take a closer look, you'll find even a few single ones, which seems almost
to change from opaque to translucent.
They are sitting in a very accentuated matrix-grid, which is in some ways
similar to Shergotty or Zagami, though finer and on a smaller scale. And
finally those dramatic and huge melt pockets and maskelynite blotches.

With all historical respect for the four other observed Martian falls,
Tissint is macroscopically the most spectacular and the most aesthetical
among the observed falls. For sure.

Masterly polished by Stefan's craftsmanship, completely surrounded by fusion
crust, with at best only here and there naturally a small chip missing, are
these those adorable specimens, which also in later decades you'll take in
your hands, with a silent and almost triumphal blitheness, to have been once
so wise, to have saved these specimen just in the days of the birth of this
so famous meteorite.

And if you were one of the few lucky ones, who were able to gather one of
the few complete individuals, such a fullslice is almost a must to add.

(And those who weren't - watch the endcut, a perfect alternative
 or contact us for still a superb complete individual).

Enjoy!

Stefan  Martin

Chladni's Heirs
Munich - Berlin
Fine Meteorites for Science  Collectors

http://www.chladnis-heirs.com


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[meteorite-list] AD: Special: An unique and truly exotic anomalous Mesosiderite - NWA 7025

2012-03-15 Thread Chladnis Heirs
Dear List community,

as it wouldn't be already a really rare event, that a new unpaired
mesosiderite can be introduced, 
we have today a by all means astounding stone, worthy for one of our
Specials:

NWA 7025.

Well... if you take a look on the cut surfaces, we think, you'll tend to
guess or to reckon, to have here an evolved achondrite. Those chrystals, no
metal visible. Nevertheless not looking too weathered - Maybe a
brachinite...


To shorten it, we leave the word to the expert. Here is the gobsmacking
report of the classification:

The specimen contains two distinct domains in contact along curvilinear
boundaries. One lithology consists predominantly of orthopyroxene with
subordinate anorthite, ~25 vol.% troilite+metal (kamacite and taenite as
small cuspate grains), accessory chromite and merrillite, and appears to be
a variety of mesosiderite. Other portions of the specimen have similar
mineralogy, except that most of the troilite and metal has been replaced by
small cuspate voids (with the same general shape as the troilite and metal
grains in the other lithology), and there is a narrow transitional zone
between these domains (see image below). The overall mineralogy and the
orthopyroxene compositions (Fs26.3-26.5Wo2.9-3.1, FeO/MnO = 26-28) are
typical for mesosiderites, and oxygen isotopic compositions determined on
acid-washed subsamples by laser fluorination at Okayama University (d17O
1.961, 1.847, 2.082; d18O 4.149, 3.992, 4.387; D17O -0.223, -0.255, -0.228
per mil) also are consistent. This specimen appears to be a mesosiderite,
which has undergone terrestrial weathering by infiltration of fluids that
selectively leached much of the primary troilite and metal in some parts of
this meteorite.


It is an anomalous, an altered mesodiderite!

Our baffling and surprising NWA 7025.


A stone for the expert.
A stone for the collector aiming for the really all new.


And now we invite you to order your specimen, as always prepared to the
standard, you're used to from Chladnis Heir's, and as long as that surprise
lasts:

http://www.chladnis-heirs.com/specials/special-nwa7025.html


Success!

Stefan  Martin

Chladni's Heirs
Munich - Berlin
Fine Meteorites for Science  Collectors

http://www.chladnis-heirs.com


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Re: [meteorite-list] What is Chladni's book on 18 meteorite fallstitle??????

2012-04-12 Thread Chladnis Heirs
Hi Jan,

here are some more meteoritic publications by Chladni additional to those, 
listed in your link:

1796 - Auszug aus einem Aufsatze über ein am 24.Juli 1790 in Gascogne 
beobachtetes feuriges Meteor, von   Baudin, Professor der Physik in Pau.
Nebst einigen allgemeinen Bemerkungen über Feuerkugeln und Sternschnuppen., 
Voigt Magazin, Vol 11, p. 112 seqq.


1797 - Fortsetzungen der Bemerkungen über Feuerkugeln und niedergefallene 
Massen,
Voigt Magazin, Vol 1, p. 17 seqq.


1812 - Ueber die Ellbogener gediegenen Eisenmassen, 
   Gilbert, Annalen der Physik, Vol 42, p. 203 seqq

 - Ueber Gediegeneisen und besonders ueber eine noch nicht bekannte, im 
Mailändischen gefundene   Gediegeneisenmasse,
Schweigger, Journal für Chemie und Physik, Vol 4, p. 116 seqq.

 - Chronologisches Verzeichnis der herabgefallenen Stein- und Eisenmassen,
   Schweigger, Journal für Chemie und Physik, supplement p. 1 seqq.


1814 - Ueber vergebliche Bemühungen, verschiedene ältere Meteorsteine 
aufzufinden, nebst einigen Bemerkungen,
  Gilbert, Annalen der Physik, Vol 47, p. 96 seqq.


1815 - Bemerkungen über gediegen Eisenmassen,
   Gilbert, Annalen der Physik, Vol 50, p. 257 seqq.


1816 - Bemerkungen zu einem Aufsatze von Dr.Blumhof zu Biedenkopf,
   Gilbert, Annalen der Physik, Vol 53, p. 310 seqq.

 - Erste Fortsetzung der bisher bekannt gewordenen Stein- und Eisenmassen, 
nebst neuen Beiträgen zur Geschichte der Meteore und einigen diesen Gegenstand 
betreffenden Bemerkungen,
   Gilbert, Annalen der Physik, Vol 53, p. 369 seqq.

 - Zweite Fortsetzung des Verzeichnisses der vom Himmel gefallenen Massen,
   Gilbert, Annalen der Physik, Vol 54, p. 329 seqq.

 - Einige Berichtigungen und Zusätze,
   Gilbert, Annalen der Physik, Vol 54, p. 393 seqq

 - Fortsetzung des im 4. Bde. Enthaltenen chronologischen Verzeichnisses 
der herabgefallenen Stein- und Eisenmassen, nebst einigen Bemerkungen über 
deren Ursprung,
   Schweigger, Journal für Chemie und Physik, Vol 17, p. 113 seqq.


1817 - Ueber die sprungweise gehende Bewegung mancher Feuerkugeln, nebst 
einigen Folgerungen,
   Gilbert, Annalen der Physik, Vol 55, p. 91 seqq

 -  Dritte Fortsetzung des Verzeichnisses und der Geschichte der vom 
Himmel gefallenen Massen
   Gilbert, Annalen der Physik, Vol 56, p. 375 seqq

 - Beitrag zu dem Aufsatze über die sprungweise gehende Feuerkugeln,
   Gilbert, Annalen der Physik, Vol 56, p. 387 seqq

 - Ueber Unabhängigkeit der Meteorsteinfälle und der Feuerkugeln von 
Jahres- und Tageszeiten,
von den Himmelsgegenden, von der geographischen Lage von Wetter und von 
bestimmten Perioden,
   Gilbert, Annalen der Physik, Vol 57, p. 121 seqq

 - Ueber Dinge, die sich im Weltraum befinden und von den bekannten 
Weltkörpern verschieden sind,
   Lindenau, Bohnenberger, Zeitschrift für Astronomie, Vol 4, p. 303 seqq  
p. 480 seqq.


1818 - Ueber Sternschnuppen von dem Dr. Benzenberg,
   Gilbert, Annalen der Physik, Vol 58, p. 289 seqq

 - Bemerkungen über einige kosmologische Gegenstände,
   Lindenau, Bohnenberger, Zeitschrift für Astronomie, Vol 5, p. 376 seqq

 - Verschiedene physikalische Bemerkungen: Mondvulkane, Feuerkugeln,
   Gilbert, Annalen der Physik, Vol 59, p. 3 seqq

 - Sur le Mouvement par bonds de plusieurs globes de feu, et conséquences 
tirées de ce phénomène.
   Annales de chimie et de physique, Vol 9, p. 389 seqq


1819 - Vierte Fortsetzung des Verzeichnis der vom Himmel gefallenen Massen,
   Gilbert, Annalen der Physik, Vol 60, p. 238 seqq

 - Einige Ideen über das Innere der Erde,
   Gilbert, Annalen der Physik, Vol 62, p. 72 seqq

 - Fünfte Fortsetzung des Verzeichnis der vom Himmel gefallenen Massen,
   Gilbert, Annalen der Physik, Vol 63, p. 17 seqq

 - Ueber Feuermeteore und die mit denselben herabgefallenen Massen. Nebst 
zehn Steindrucktafeln von C. v.   Schreibers,
   Heubner, Vienna

 - Ueber die Feuermeteore,
   Schweigger, Journal für Chemie und Physik, Vol 26, p. 156 seqq.

 - Ueber die Widmannstädtschen Figuren,
   Schweigger, Journal für Chemie und Physik, Vol 26, p. 196 seqq.


1822 - Neues Verzeichnis der bis jetzt bekannt gewordenen Niederfälle 
meteorischer Stein- und Eisenmassen,
und anderer Substanzen,
Gilbert, Annalen der Physik, Vol 36, p. 87 seqq
 
- Einige Bemerkungen über Tod durch einen Meteorstein,
   Abendzeitung 1822, N° 300

1824 - Neue Beiträge zur Kenntnis der Feuermeteore und der herabgefallenen 
Massen,
   Poggendorff, Annalen, Vol 2, p. 151 seqq. (Vierte Lieferung)
 
 -  E. F. F. Chladni’s Beschreibung seiner Sammlung vom Himmel 
herabgefallener
   Massen. Nebst einigen allgemeinen Bemerkungen, 
   Archiv für die gesammte Naturlehre, Nürnberg, Vol 4, p. 200 seqq.


1825 - Nachrichten von einem Meteorsteinfalle am 15. Januar 1824 im 
Bolognesischen 
   

Re: [meteorite-list] What is Chladni's book on 18 meteorite falls title?????? (Stuetz)

2012-04-12 Thread Chladnis Heirs
Hi Shawn,

the paper by Andreas Xaver Stuetz, you're looking for,
was published in Born's  Trebra's Bergbaukunde, second volume, 1790.

You have it here online:
http://kuerzer.de/shawnstuetz

Page 398 - 409.

In fact he reports there from the fall of Eichstädt, mentions the
Pallas-Iron
and gives at length a report about the fall of Hraschina - with eyewitness
observations,
in translating the report about the fall by Wolfgang Kukulyewich, vicar of
Agram.
Here and there he gives some ironic remarks.

Stuetz is classifying these reports as fairy tales,
closing the article with a lengthy explanation, that these stonesirons were
formed by lightning.

Best!
Martin  Stefan 



-Ursprüngliche Nachricht-
Von: meteorite-list-boun...@meteoritecentral.com
[mailto:meteorite-list-boun...@meteoritecentral.com] Im Auftrag von Shawn
Alan
Gesendet: Donnerstag, 12. April 2012 10:25
An: Meteorite Central
Betreff: [meteorite-list] What is Chladni's book on 18 meteorite falls
title??

Hello Listers

I am wondering if any of you history meteorite buffs by chance know the name
of Chladni's book he wrote on 18 meteorites falls and if there might be an
English pdf version floating around on the Internet or somewhere else? Also,
I was trying to look for a copy of the paper titled On Some Stones
Allegedly Fallen from the Heaven published in 1790 by Abbe Andreas Xavier
Stutz which Chladni extensively quoted from when he was writing his book.

Shawn Alan
IMCA 1633
ebay Store
http://www.ebay.com/sch/ph0t0phl0w/m.html?
http://www.meteoritefalls.com/  
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[meteorite-list] OT: on a personal note

2012-08-09 Thread Chladnis Heirs
Dear list members,

to avoid possible irritations, I've to give out:

Due to a longsome disease I'm forced to take a downtime from meteorites.
How long it will take, I can't foresee, but I'm confident, to be there for
you, in the way you're used to, after recovery.

In the meantime I'd like to ask you to address with your meteoritical
concerns to Chladni's Heir Stefan:

ste...@meteoriten.com
or
n...@chladnis-heirs.com

Thank you for your understanding
and best regards,
Martin



Stefan  Martin

Chladni's Heirs
Munich - Berlin
Fine Meteorites for Science  Collectors

http://www.chladnis-heirs.com


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Re: [meteorite-list] Christian Anger

2010-01-13 Thread Chladnis Heirs
It is a tragedy,
which leaves us without words.

Martin and Stefan



-Ursprüngliche Nachricht-
Von: meteorite-list-boun...@meteoritecentral.com
[mailto:meteorite-list-boun...@meteoritecentral.com] Im Auftrag von
impact...@aol.com
Gesendet: Mittwoch, 13. Januar 2010 23:57
An: meteorite-list@meteoritecentral.com
Cc: h63str...@aol.com
Betreff: [meteorite-list] Christian Anger



Hello everybody,
 
I just received this email (below) from Hanno, with very sad news.
For all of you who did not know Christian Anger, he was an expert meteorite 
collector and a very friendly guy. In his real life he was an Engineer, and 
lived near Vienna, Austria. He leaves behind an (ex)wife and two little 
girls.
And I still remember when we were waltzing together in Ensisheim, in much 
happier times.
 
Anne M. Black
_http://www.impactika.com/_ (http://www.impactika.com/) 
_impact...@aol.com_ (mailto:impact...@aol.com) 
Vice-President, I.M.C.A. Inc.
_http://www.imca.cc/_ (http://www.imca.cc/) 

Hello Anne,

today I received an email from Harald Stehlik, that our good friend 
Christian Anger had on 14.dec 2009 a very heavy car accident and he died.

I am very shocked and sad, because Christian was not only a collector but a 
friend.
Everybody know how much fun we had when we were togheter.
We had also other private contact and were real friends.

At first he told me that he cannot come to the Munich show, because he had 
so many private problems in his mind.
Then he called me thursday evening when I was in Munich that he decided to 
come. So he was with us friday evening at the Fliegerbräu and stayed in 
Munich till sunday afternoon. He helped me to bring some of my material back

into the car sunday afternoon.
This was the last time I saw him.

True friendship never ends..

Hanno Strufe

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Re: [meteorite-list] Pairing discussion/questions

2010-01-19 Thread Chladnis Heirs
Hello Jeff,

This statement, appearing in some of the recent emails, is wrong.

Really? I was speaking about different meteorites.

M.Lindstrom  R.Score
came to the the result,

that the average number of Antarctic meteorites per pairing group is 5.

M.Lindstrom, R.Score:
Populations, Paring and Rare Meteorites in the U.S. Antarctic Meteorite
Collection

http://www-curator.jsc.nasa.gov/antmet/ppr.cfm


And where in the world did this 
figure of billions of dollars being spent by the US to collect its 
20,000 meteorites come from?

Not the U.S. - USA, Japan, China, Europe together.

Antarctic is an expensive place to work and to live.
You need special equipment, you have to transport everything there, you have
to maintain the infrastructure, and like with any other program, you have
the running costs for the personnel (salaries, social insurances, working
place costs).

The figures are scattered over the web.
There you can read, only to give some examples, that one standard ANSMET
team causes 800,000$ primary costs without secondary costs for 6 weeks on
the ice - and that the whole Antarctic summer semester over would be hunted.

Somewhere you will find, that the supply and the transport of fuels 
to maintain the McMurdo Station costed 70 millions $ in one year.

And so on.

Personnel costs too, remember EUROMET, who had basic costs for personnel
without any expedition yet of 20 millions $ per year (they went also to
Antarctica).

Labs, tertiary costs - 

it will be all difficult to amount.
(Would be interesting, if someone would do this once).

Well and then think, that not only the U.S. are hunting there, but for a
similar long time NIPR, then the few EUROMET trips, as well as China.

Well and that for 33 years...

will easily sum up to a total of far more than a billion.


Personnel, equipment, insurances, pension plan, fuels, transportation,
administration,
These costs the public hasn't to pay, if they are buying NWAs.

The Bulletins you know.
Seen the tkws and the numbers from almost all rarest, rare and semi-rare
types - it was meanwhile more found in NWA than in Antarctica.

An unclassified averagely weathered kg NWA-OC delivered to your doorstep
costs you around 30$.
What does it cost to recover 1kg of an averagely weathered OC in Antarctica?

How long does it take and what did it cost to find 19 different lunaites in
Antarctica for USA, Japan, Europe and China together? 33 years.
How long takes the same task in the private desert sector? 5 years.

What does cost 1 1/4 kg of an classified R-Chondrite from NWA?  12,000$?
In 33 years of Antarctic expeditions in total R-chondrites were found:  
1 1/4kg.

A scientist is accepted to take part in an ANSMET-hunt.
He steps out of the door in sunny Arizona - will 12,000$ be enough to reach
his final destination?

Jeff, don't get me wrong please.

It is not my intention to play the cold desert hunts off against the hot
desert hunts.

The Antarctic meteorite programs are wonderful, great, absolutely necessary
and the expenses more than justified.

But in my opinion it would also extremely stupid, if science would abstain
from the NWA and Oman finds, and wouldn't work additionally on them.
Because they are meanwhile even more manifold than the Antarctic finds,
outweigh them by mass, 
and cost the public compared to the Antarctic finds virtually almost nothing
at all.

To set them aside would IMHO also not directly justifiable to the public,
because, sorry to say that, but sometimes it is forgotten, ANSMET, NIPR,
PRIC, ect. are paid with public tax-money.

I'd say,
Martin



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Von: meteorite-list-boun...@meteoritecentral.com
[mailto:meteorite-list-boun...@meteoritecentral.com] Im Auftrag von Jeff
Grossman
Gesendet: Dienstag, 19. Januar 2010 13:46
An: Meteorite-list
Betreff: Re: [meteorite-list] Pairing discussion/questions

 Make your homework. How many different meteorites do we have from 
 Antarctica after a third of a century hunting and spending billions of 
 USD? 7000.
This statement, appearing in some of the recent emails, is wrong.  There 
are over 16,000 classified meteorites from the ANSMET expeditions, plus 
a few thousand unclassified.  Counting the Japanese, Chinese,European,  
Korean, and minor collections, There ~27,000 classified Antarctic 
meteorites, and probably close to 20,000 not yet classified (mostly in 
the Japanese and Chinese collections).  And where in the world did this 
figure of billions of dollars being spent by the US to collect its 
20,000 meteorites come from?

Also, don't overlook the fact that Antarctic meteorite have proven to be 
vastly more valuable scientifically than NWA meteorites.  They probably 
occur as subjects of scientific publications at 10x the frequency as 
NWA meteorites (I posted statistics on this some years ago, but can't 
locate it at the moment).  This is because the main masses are well curated.

Jeff

-- 
Dr. Jeffrey N. Grossman   phone: (703) 648-6184
US 

Re: [meteorite-list] Dumb Questions About Meteors Meteorites

2010-01-26 Thread Chladnis Heirs
Hi Erik,

unfortunatly most of these balls are also anthropogenic pollution.
Especially industries like coal-burning power plants, foundries and metal
processing produces such spherical particles.

That's why one has either to go in the stratosphere to collect
micrometeorites or to use unpolluted sources like Antarctic wells or ice
or sediments - from the times where there wasn't human pollution,
to be able to isolate them.

Especially in the late 70ies and early 80ies it was quite a fashion among
the collectors to try to find micrometeorites by filtering rainwater.

Best!
Martin  Stefan


-Ursprüngliche Nachricht-
Von: meteorite-list-boun...@meteoritecentral.com
[mailto:meteorite-list-boun...@meteoritecentral.com] Im Auftrag von Erik
Fisler
Gesendet: Dienstag, 26. Januar 2010 08:34
An: meteorite-list
Betreff: Re: [meteorite-list] Dumb Questions About Meteors  Meteorites


Eric, try this:
 One way to collect micrometeorites is to set a large shallow tray of
water outside for a couple days. You should see some residue on the
bottom in time. Cover a magnet with Saran wrap, wax paper or some other
type of material. Pick up magnetic material in tray with your magnet
and set on paper to dry. Observe material with a good- strong
microscope. Some of what you see will be spherical balls- those are the
micrometeorites.

Steve from the nuggetshooter
forum(http://www.nuggetshooter.ipbhost.com/index.php?showforum=4) posted
that 2 years ago.  There were great links and photos but the sites are long
gone.  I quote, If you're not having any luck hunting macrometeorites, try
hunting micrometeorites. You'll never get skunked.

Can someone with a microscope try this and post pictures if they can?

[Erik]



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[meteorite-list] AD: Special - Fabulous New Diogenite - NWA 6024 prov.

2010-02-18 Thread Chladnis Heirs
Dear collectors,

Today we have the pleasure to present you an – in our eyes - simply
wonderful stone:

NWA 6024 - a new diogenite.

We all are aware of the Vesta-debris-breccias,
where the bow is drawn from the polymict eucrites with their often typically
light-grey matrix - over the howardites - to the polymict diogenites.
And at the diogenitic end we arrived with NWA 6024.
And to what an end we came!

NWA 6024 is by all means unusual, as it contains these large smashed
blackish pyroxene crystals,
giving it an extraordinary appearance.

This diogenite is looking so characteristically, that we are not aware of
any other similar NWA at present – so that we strongly presume that it is
probably unpaired and a really new one.

Never before it was so easy for us to advertise a diogenite.  
Just watch the pictures and you’ll know why!


Here the data:

NWA 6024 prov.
Morocco 2009
Tkw  65g
Diogenite
Shock stage: moderate, Weathering grade: low

Unfortunately it had a low weight.
Fullslices we priced at 45$ a gram,
40$ a gram for the endcut with patches of remaining fusion crust.

And here you are:

http://www.chladnis-heirs.com/special-nwa6024.html


Enjoy!

Stefan Ralew  Martin Altmann

Chladni's Heirs
Munich - Berlin
Fine Meteorites for Science  Collectors
http://www.chladnis-heirs.com




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[meteorite-list] Abstracts about NWA 5789 and NWA 5990

2010-02-25 Thread Chladnis Heirs
Good evening,

we forgot to point out, that the abstracts abouth both in their way unique
new Martians were made available online.
From the program of the upcoming LPSC:

Irving A. J. Kuehner S. M. Herd C. D. K. Gellissen M. Korotev R. L. Puchtel
I. Walker R. J. Lapen T. Rumble D. III:
Petrologic, Elemental and Multi-Isotopic Characterization of Permafic
Olivine-Phyric Shergottite Northwest Africa 5789: 
A Primitive Magma Derived from Depleted Martian Mantle

http://www.lpi.usra.edu/meetings/lpsc2010/pdf/1547.pdf

We report on an extensive petrological-chemical study of a very primitive
depleted shergottite, which is similar in many (but not all) respects to
Yamato 980459/98497.


and


Irving A. J. Kuehner S. M. Herd C. D. K. Gellissen M. Rumble D. III Lapen T.
J. Ralew S. Altmann M.:
Olivine-bearing Diabasic Shergottite Northwest Africa 5990: 
Petrology and Composition of a New Type of Depleted Martian Igneous Rock

http://www.lpi.usra.edu/meetings/lpsc2010/pdf/1833.pdf

Petrologic, elemental and Nd isotope characteristics of a depleted permafic
shergottite, which bridges the gap between most olivine-phyric shergottites
and QUE 94201.


Best Regards,

Stefan  Martin

Chladni's Heirs
Munich - Berlin
Fine Meteorites for Science  Collectors  
http://www.chladnis-heirs.com


 

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Re: [meteorite-list] The Perils of Type Collecting - A Guide

2010-03-04 Thread Chladnis Heirs
Hi Mike,

So, is there a C3?

The Bulletin Database has 12 (not pairing-adjusted) C3-ungrouped entries.

Most prominent should be Ningqiang, which was first a CV3, than a CK3 (some
intermediates between CVs and CKs, you have with Tanezrouft 057 and NWA
2900)
and which is now a C3-ungr.

Well and else... we have that stone,
http://www.chladnis-heirs.com/nwa5377-6.671g.jpg

which was preliminarily classified as a C3 (without ungr).
But it's provisional and has still to be accepted by the NomCom. 

http://kuerzer.de/5377


Best!
Martin  Stefan

Chladni's Heirs
Munich - Berlin
Fine Meteorites for Science  Collectors   
http://www.chladnis-heirs.com





-Ursprüngliche Nachricht-
Von: meteorite-list-boun...@meteoritecentral.com
[mailto:meteorite-list-boun...@meteoritecentral.com] Im Auftrag von Galactic
Stone  Ironworks
Gesendet: Freitag, 5. März 2010 00:13
An: zelimir.gabel...@uha.fr
Cc: meteorite-list@meteoritecentral.com
Betreff: Re: [meteorite-list] The Perils of Type Collecting - A Guide

Hi Zelimir and List!

Now that I look closely (on David Weir's site), I see that the CM3
class is tenative and is probably not official nomenclature yet.  The
following specimens are listed as tenative CM3 :

Acfer 094, WIS 91600, B-7904,and Paris.

About Tagish Lake and the C2 group (which I overlooked the C2, but
initially had Tagish in the wrong class as C-ung, which I now notice
is C2-ung).  So, is there a C3?

Best regards,

MikeG

Revised List -

---
Carbonaceous Chondrites :

CI (Ivuna)
CM1 (Mighei)
CM2 (subdivided into CM2.0 to CM2.6)
CM3
CO3 (Ornans) (subdivided into CO3.03 to CO3.7)
CV (Vigarano) (also CV2 and CV3)
CK (Karoonda) (CK4, CK5, CK6)
CR (Renazzo) (CR1, CR2, CR3)
CB (Bencubbin)
CH
CR ungrouped
C ungrouped
C2 ungrouped (Tagish Lake)
C4 ungrouped


Ordinary Chondrites :

Rumuruti R3 (subdivided into R3.5-6 to R3.9)
R4
R5
R6

LL (subdivided into LL3.0 to LL3.9)
LL4
LL5
LL5/6
LL6
LL6/7
LL7
LL impact melt

LL transitional (L/LL3 to L/LL6)
L (subdivided into L3.0 to L3.9)
L4
L5
L6
L6/7
L7
L impact melt

H/L transitional (H/L3 to H/L6 IMB, H/L3.6 to H/L3-4)
H (subdivided into H3.0 to H3.9)
H4
H5
H6
H7
H impact melt

ungrouped ordinary chondrites


Enstatite Chondrites :

EL (EL3 to EL7)
EL impact melt
EH/L
EH (EH3 to EH7)
EH impact melt
ungrouped enstatite chondrites

K (Kakangari)

Meta-chondrites (M-CV, M-CR, M-H, M-LL)


Primitive Chondrites :

Acapulcoite
Lodranite
Winonaites
ungrouped primitive chondrites


Achondrites :

Howardite (subdivided into fragmental breccia and regolith breccia)
Eucrite (monomict and polymict with each having subclasses)
Diogenite (monomict and polymict)
Olivine Diogenite
Dunite
Ureilite (monomict and polymict)


Martian achondrites :

Shergottite
Pyroxene-phyric basaltic shergottite
Olivine-phyric basaltic shergottite
Olivine-orthopyroxene-phyric basaltic shergottite
Pyroxene-peridotitic (Wehrlitic) shergottite
Lherzolitic shergottite
Diabasic shergottite

Nakhlite
Chassignite
Orthopyroxenite (ALH 84001)


Lunar Achondrites :

Feldspathic breccias
Regolith breccia
Fragmental breccia
Impact melt breccia
Granulitic breccia
Mafic-rich
Thorium-rich
KREEP-rich

Mingled Breccia
Mare Basalt


Other Achondrites :

Angrites (Plutonic and Basaltic)
Brachinite
Aubrite
ungrouped achondrites (Ibitira, Pasamonte, etc)


Stony-Irons :

Mesosiderites (1A,1B,2A,2B,2C,3A,3B,4A,4B)
ungrouped mesosiderites

Pallasites (Main Group, Eagle Station group, Pyroxene group)
Pallasite-am (anomalous, PMG-am, PMG-as)
ungrouped pallasites


Iron meteorites :

Note, iron meteorites are a can of worms. I will only focus on the
main chemical groups, and not the various grouplets and sub-types of
each main chemical group. Also note that many of these types include
silicated varities. Listing all of the known sub-types of irons would
require a LONG list resembling a flow-chart.

IAB
IC
IIAB
IIC
IID
IIE
IIF
IIG
IIIAB
IIIE
IIIF
IVA
IVB
ungrouped irons

-


On 3/4/10, zelimir.gabel...@uha.fr zelimir.gabel...@uha.fr wrote:

 Hi Mike,

 Can you tell me the name of the CM3 ?

 Btw: a very complete list of types ( subtypes) can also be found in
 both the Met. Bull. database or at the end of the Meteorites from A
 to Z booklet (ed 2008) by Jensen bros.

 Note: Murchison is CM2.5 (Rubin  al, Geochim, Cosmochim. Acta, 2008)

 Note 2: don't forget to add CK3 and C2 (Tagish) and a few other (see
 Carl's remarks)

 Note 3: I am not sure metachondrite is official, though I very much
 appreciate that new nomenclature suggested by D. Weir in his
 outstanding comprehensive site.

 Best wishes,

 Zelimir



 Galactic Stone  Ironworks meteoritem...@gmail.com a écrit :

 Thanks to Carl, Katsu, Greg, Martin, and everyone else who provided
 corrections and input on this list.  I have made corrections and the
 revised list is presented below :

 Carbonaceous Chondrites :

 CI (Ivuna)
 CM1 (Mighei)
 CM2 (subdivided into CM2.0 to CM2.6)
 CM3
 CO3 (Ornans) 

[meteorite-list] Quick-AD: Last SMALL Specimen of very special Martian NWA 5990 Last New Halfa

2010-03-14 Thread Chladnis Heirs
Good afternoon,

today we want to give only a short note on 2 specimens.

First is a sample of the most noteworthy new Martian NWA 5990.
Here again the abstract, outlining its special rank among the Martians:
http://www.lpi.usra.edu/meetings/lpsc2010/pdf/1833.pdf

There, because several collectors were somewhat worried not being able to
add this important Martian to their systematics, because originally only
full- and half-slices were available,
we sacrificed a half-slice to make smaller samples for them.
These are all distributed now, 
but we have a surplus sample left.

A quarter-gram (0.256g) partslice.

Unfortunately this specimen is already the last opportunity for the private
collector, still to add such a smaller sample of this Martian to his
collection.


Secondly:  We forgot to piggyback on Martin Horejsi's fine article about 
New Halfa in the November issue of the Meteorite Times.

http://www.meteorite-times.com/Back_Links/2009/november/Accretion_Desk.htm


There we would have still a partial endcut left, 33.60g, with some fusion
crust.

Stems from a fragment, somewhat larger than a fist, which we acquired years
ago from the eyewitness Mr.Khalil, who is also mentionned in the Bulletin
entry. (The Catalogue of Meteorites has a little mistake, the fall happened
close to village N°19 and not N°9).
Mr.Khalil and friends were going there from door to door, asking the locals,
whether they may had collected some pieces, but without success,
because then not many dared to leave the house, because all thought that
sound phenomena of the fall would origin from a rocket assault.
The fall area itself is destroyed by agriculture, so that it's highly
unlikely that still finds could be made there.

Would maybe also interesting not only for private collectors,
if one thinks, that from the top-twenty collections of the World none, but
Berlin (8 grams) has this observed fall.

Well, instead to incite a longsome bidding battle on ebay for these two last
specimens, we'd rather say,
just send us an email for pictures and details, if interested.


Have all a fine Sunday!

Stefan Ralew  Martin Altmann

Chladni's Heirs
Munich - Berlin
Fine Meteorites for Science  Collectors 

http://www.chladnis-heirs.com


 

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[meteorite-list] Quick-AD: a Piece of the Enigmatic Tamdakht-Ralewite a Slice of a new Stony Winonaite

2010-04-21 Thread Chladnis Heirs
Hello members,

just a small  speedy AD:

From our last travel we brought back once again a small lot of specimens of
that incredible Tamdakht-Couscous, which still awaits an explication for
its formation. See also the discussion on the list one year ago:
http://kuerzer.de/Ralewite1

http://kuerzer.de/Ralewite2
  

There we have a grinded half of a specimen to spare. 7.106g. 50$/g
http://www.chladnis-heirs.com/7_106g.jpg

http://www.chladnis-heirs.com/7_106g-2.jpg


Second offer today is a fullslice of a small new winonaite (NWA 6187 prov.)
There we wrote stony in the title, because it doesn't belong to the
iron-rich ones, where here on the list it was discussed, how they could be
differentiated from the silicated IAB-irons.
Well, that here would be a normal AWIN (if something like this exists.
They are so rare...)

A fullslice of 4.281g, one side polished, one side grinded. 100$/g
http://www.chladnis-heirs.com/nwa6187-4_281g.jpg

http://www.chladnis-heirs.com/nwa6187-4_281g-2.jpg



Thank you for your attention
and our (admittedly somewhat jealous) greetings
to the hunters and collectors in WI!
Go for the main mass!

Stefan Ralew  Martin Altmann

Chladni's Heirs
Munich - Berlin
Fine Meteorites for Science  Collectors

http://www.chladnis-heirs.com



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[meteorite-list] Quick-AD: a Piece of the Enigmatic Tamdakht-Ralewite a Slice of a new Stony Winonaite

2010-04-21 Thread Chladnis Heirs
Hello members,

just a small  speedy AD:

From our last travel we brought back once again a small lot of specimens of
that incredible Tamdakht-Couscous, which still awaits an explication for
its formation. See also the discussion on the list one year ago:
http://kuerzer.de/Ralewite1

http://kuerzer.de/Ralewite2
  

There we have a grinded half of a specimen to spare. 7.106g. 50$/g
http://www.chladnis-heirs.com/7_106g.jpg

http://www.chladnis-heirs.com/7_106g-2.jpg


Second offer today is a fullslice of a small new winonaite (NWA 6187 prov.)
There we wrote stony in the title, because it doesn't belong to the
iron-rich ones, where here on the list it was discussed, how they could be
differentiated from the silicated IAB-irons.
Well, that here would be a normal AWIN (if something like this exists.
They are so rare...)

A fullslice of 4.281g, one side polished, one side grinded. 100$/g
http://www.chladnis-heirs.com/nwa6187-4_281g.jpg

http://www.chladnis-heirs.com/nwa6187-4_281g-2.jpg



Thank you for your attention
and our (admittedly somewhat jealous) greetings
to the hunters and collectors in WI!
Go for the main mass!

Stefan Ralew  Martin Altmann

Chladni's Heirs
Munich - Berlin
Fine Meteorites for Science  Collectors

http://www.chladnis-heirs.com




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Re: [meteorite-list] VERY SAD NEWS

2010-04-22 Thread Chladnis Heirs
Dear Abdelfattah,

this is a really sad and the more shocking news,
as we met Mbarek just a few weeks ago and found him in his always jocund and
friendly mood.

We and we think we can speak also for all the countless collectors,
researchers and curators keeping knowingly or unknowingly specimens in their
collections from the stones, which had passed through his hands,
are grateful to his contribution and will honour his memory.

Today the meteorite family has lost a good man.


Saddened we express our condolences to Mbarek's family and his friends.

Stefan  Martin



-Ursprüngliche Nachricht-
Von: meteorite-list-boun...@meteoritecentral.com
[mailto:meteorite-list-boun...@meteoritecentral.com] Im Auftrag von
abdelfattah gharrad
Gesendet: Donnerstag, 22. April 2010 17:19
An: meteorite-list@meteoritecentral.com
Betreff: [meteorite-list] VERY SAD NEWS

Dear list members,
 
I want to inform you that Mbarek Ait El Caid was dead today I had this bad
news from a friend of Rissani.
 
Mbarek is a serious and honest confidant man who helped the science in field
of meteorites. the majority of meteorites that have the scientific,
collectors and dealers coming  from this person.

and I think many people know Mbarek or heard about him and specialy those
who have visited Morocco.
 
Mbarek is a person well experienced in meteorites. the world of meteorites
has really lost a wise man and the active tillering person.
 
I do not know what to say about this person. He has a good and exellent
performance. I worked with him for years.

 ( INA LI ALLAH WA INA ILAYHI RAJIOUNE) we are all to GOD and to GOD we
return.
 
Cheers,
Abdelfattah.


  
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