Re: [meteorite-list] Chladni's Heirs NORWAY field report

2006-07-25 Thread Meteoriteshow
Many thanks Martin, Andreas and Stefan for sharing the information with us.
I hope that you are not too much disapointed and that at least you had fun!
You made a very good report and I wish a long 'life' to your CHALDNI'S HEIRS
Kind regards,

Frederic

- Original Message -
From: Martin Altmann [EMAIL PROTECTED]
To: meteorite-list@meteoritecentral.com
Sent: Monday, July 24, 2006 11:44 PM
Subject: [meteorite-list] Chladni's Heirs NORWAY field report


 Collectors, enthusiasts, list!

 The searching delegation of Chladni's Heirs* just returned from a
 6-days-trip in Norway on the hunt for the new fall.
 We set up a little website with an illustrated report:
 http://www.meteoriten.com/norway.html





 *Chladni's Heirs
 was planned to be officially launched after a summer break,
 now with this actual event you will already got to know our brand's name.

 Chladni's Heirs is an amalgamation of your (hopefully soon) preferred
 meteorite dealers:
 Stefan Ralew
 Andreas Gren
 Martin Altmann
 founded for the purpose to bundle their strengths to serve the collectors
 even better than before, to assist them in all concerns more accurate and
 faster and to offer them the enlarged and full palette of meteorites: irons,
 rare and aesthetic common desert types, historic finds and falls at best
 quality and competitive prices.

 Although the official launch will be dated later,
 we already accept congratulations :-)

 Stefan Ralew
 Andi Gren
 Martin Altmann

 Chladni's Heirs will take part in the Tucson show 2007


 And now we sing:

 There's a mineral shop down our street,
 It's run by a German,
 And they sells good things to collect,
 But you should hear him speak,
 When you ask him anything,
 Never answers No,
 He just yesses you to death,
 And as he takes your dough he tells you:

 Refrain:
 Yes! We have no martians,
 We have no martians today.
 We've chondrites, and onions,
 rumurutis and eucrites
 And all kind of stones, and say,
 We have an old fashioned Gibeon
 Moroccan potato,
 But yes! We have no martians,
 We have no martians today!


 Things were going well with him,
 He wrote home to say,
 Send me Patrick and Peter and Jim,
 I need them right away,
 When he got them in the shop,
 There was fun, you bet,
 'Cause when you asked them anything,
 They answered in quartet: Oh,


 And now all together:
 Yes! We have no martians,
 We have no martians today.
 We've chondrites, and onions,
 rumurutis and eucrites
 And all kind of stones, and say,
 We have an old fashioned Gibeon
 Moroccan potato,
 But yes! We have no martians,
 We have no martians today!



 __
 Meteorite-list mailing list
 Meteorite-list@meteoritecentral.com
 http://six.pairlist.net/mailman/listinfo/meteorite-list



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Re: [meteorite-list] Black inclusions in NWA R-Chondrites?

2006-07-25 Thread Jeff Kuyken
Thanks to everyone who replied both on and off-list regarding the Rumuruti
chondrites and their black inclusions. I will update the my page over the
next week or two with the info.

Thanks again,

Jeff


- Original Message -
From: [EMAIL PROTECTED]
To: Meteorite-list@meteoritecentral.com
Sent: Tuesday, July 25, 2006 4:25 AM
Subject: [meteorite-list] Black inclusions in NWA R-Chondrites?


Hi Jeff and List,

I'm hoping someone may know of an abstract/personal/web info on the black
 (xenolithic?) inclusions found in some of the NWA R-Chondrites? Any info
 would be appreciated either on or off-list. Here is an example:

http://www.meteorites.com.au/features/nwa2921.html

Beautiful specimen with a very conspicuous, large, dark clast and another
equally large but light greyish-brown clast set in a medium-gray matrix
(this light-dark structure is typical of regolith breccias).

As for the black inclusion, I don't think it is xenolithic. It represents
unequilibrated material of low(er) petrologic type. Hence all those tiny
chondrules set in a dark matrix that resembles that of carbonaceous chon-
drites.

The light- to medium-colored matrix areas show only few chondrules and/or
chondrule relics and thus correspond to petrologic types 5 or 6. The dark,
chondrule-rich clasts are unequilibrated and correspond to type 3.x (about
3.8 some sources say).

But: the dark clasts are NOT carbonaceous but are due to the dispersion of
tiny grains of sulfides and Cr-spinels, which causes silicate darkening.

My beautiful NWA 3098 (R5) and my latest addition, NWA 2943 (R3-6), which
is still in San Diego with Cap'n Blood, also show these dark, unequilibrated
clasts.

But, whereas my NWA 3098 from Stefan clearly shows chondrule-poor, light
clasts and a few small but chondrule-rich dark clasts (see JPEGs in my
private mail to you), the NWA 2943 from Michael Blood has an overall
higher abundance of chondrules - the chondrules are more evenly distributed.
throughout the busy matrix.

Best wishes,

Bernd

Here are some useful references:

BLAND P. et al. (1992a) A unique type 4 chondrite from
the Sahara - Acfer 217 (abs. Meteoritics 27, 1992, 204-205).

BISCHOFF A. et al. (1994a) Acfer 217 - a new member of
the Rumuruti chondrite group (Meteoritics 29, 264-274).

DIXON E.T. et al. (2003) 39Ar-40Ar chronology
of R chondrites (MAPS 38-3, 2003, pp. 341-355).

JACKEL A. et al. (1996) DaG 013 - A new Saharan Rumuruti-
chondrite (R3-6) with highly unequilibrated (Type 3) fragments
(abs. Lun.Plan. Sci. 27, 595-596).

BISCHOFF A. (2000) Mineralogical characterization of
primitive, type-3 lithologies in Rumuruti chondrites
(MAPS 35-4, 200, pp. 699-706).

BISCHOFF A. et al. (2001) Mineralogy, Chemistry, and noble
gases of the unpaired Rumuruti chondrites NWA 753 and NWA 755
(MAPS 36-9, 2001, A021).

LINGEMANN C.M. et al. (2000) Rumuruti chondrites: Origin and
evolution of primitive components (MAPS 35-5, 2000, A098).


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Re: [meteorite-list] Chladni's Heirs NORWAY field report

2006-07-25 Thread Marco Langbroek


Enjoyed reading the field report, and hals und beinbruch to the Chladni Heirs...

- Marco  :-)

-
Dr Marco Langbroek
Dutch Meteor Society (DMS)

e-mail: [EMAIL PROTECTED]
private website http://home.wanadoo.nl/marco.langbroek
DMS website http://www.dmsweb.org
-
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Re: [meteorite-list] Chladni's Heirs NORWAY field report

2006-07-25 Thread MARK BOSTICK

Hello list and Chladni's Heirs,

Thanks for your report Martin.  Nice to see you hunters showing respect to 
the landowners.  A big shame on you to the previous hunters that were not.


Clear Skies,
Mark Bostick
www.meteoritearticles.com


- Original Message -
From: Martin Altmann [EMAIL PROTECTED]
To: meteorite-list@meteoritecentral.com
Sent: Monday, July 24, 2006 11:44 PM
Subject: [meteorite-list] Chladni's Heirs NORWAY field report


 Collectors, enthusiasts, list!

 The searching delegation of Chladni's Heirs* just returned from a
 6-days-trip in Norway on the hunt for the new fall.
 We set up a little website with an illustrated report:
 http://www.meteoriten.com/norway.html





 *Chladni's Heirs
 was planned to be officially launched after a summer break,
 now with this actual event you will already got to know our brand's name.

 Chladni's Heirs is an amalgamation of your (hopefully soon) preferred
 meteorite dealers:
 Stefan Ralew
 Andreas Gren
 Martin Altmann
 founded for the purpose to bundle their strengths to serve the collectors
 even better than before, to assist them in all concerns more accurate and
 faster and to offer them the enlarged and full palette of meteorites: 
irons,

 rare and aesthetic common desert types, historic finds and falls at best
 quality and competitive prices.

 Although the official launch will be dated later,
 we already accept congratulations :-)

 Stefan Ralew
 Andi Gren
 Martin Altmann

 Chladni's Heirs will take part in the Tucson show 2007


 And now we sing:

 There's a mineral shop down our street,
 It's run by a German,
 And they sells good things to collect,
 But you should hear him speak,
 When you ask him anything,
 Never answers No,
 He just yesses you to death,
 And as he takes your dough he tells you:

 Refrain:
 Yes! We have no martians,
 We have no martians today.
 We've chondrites, and onions,
 rumurutis and eucrites
 And all kind of stones, and say,
 We have an old fashioned Gibeon
 Moroccan potato,
 But yes! We have no martians,
 We have no martians today!


 Things were going well with him,
 He wrote home to say,
 Send me Patrick and Peter and Jim,
 I need them right away,
 When he got them in the shop,
 There was fun, you bet,
 'Cause when you asked them anything,
 They answered in quartet: Oh,


 And now all together:
 Yes! We have no martians,
 We have no martians today.
 We've chondrites, and onions,
 rumurutis and eucrites
 And all kind of stones, and say,
 We have an old fashioned Gibeon
 Moroccan potato,
 But yes! We have no martians,
 We have no martians today!



 __
 Meteorite-list mailing list
 Meteorite-list@meteoritecentral.com
 http://six.pairlist.net/mailman/listinfo/meteorite-list



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Meteorite-list@meteoritecentral.com
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[meteorite-list] Check out the price per gram on this lunar meteorite!

2006-07-25 Thread Darren Garrison
http://cgi.ebay.co.uk/ws/eBayISAPI.dll?ViewItemitem=280009005570
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[meteorite-list] Check out the price per gram on this lunar meteorite!

2006-07-25 Thread bernd . pauli
These huge white areas are undoubtedly anorthositic
and the angular glassy clasts set in this groundmass
point to an volcanologically active area on the Moon
with busy touristic activity!


Bernd :-))

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[meteorite-list] Going Out With A Bang (SMART-1)

2006-07-25 Thread Ron Baalke

http://www.spaceflightnow.com/news/n0607/24smart1/

Going out with a bang
Lunar orbiter to impact
BY STEPHEN CLARK
SPACEFLIGHT NOW
July 24, 2006

A pioneering space probe has set a course for a dramatic end to its
three-year mission in September, when it will collide with the Moon in a
spectacular send-off for scientists to learn new information about the
lunar surface.

The innovative SMART-1 technology demonstrator is about to wrap up a
highly successful mission testing a range of new spacecraft concepts and
systems for potential use in the future. The Swedish-built craft also
conducted a broad science program using an array of instruments.

The end will come with a fiery crash into the Moon's nearside at about
0541 GMT (1:41 a.m. EDT) on September 3, according to the best data now
available. This time is only certain within seven hours.

The exact timing of the impact will slightly change as the probe's orbit
evolves in several upcoming trim maneuvers designed to fine-tune the
craft's approach. Five such burns are planned for July 27, July 28,
August 25, and on the final two days before SMART-1 hits the surface.

Scientists' best guess on the impact site puts it in the Moon's
mid-southern latitudes in a region known as the Lake of Excellence. The
location is believed to be of mostly volcanic origin and areas of
highlands and hills are also nearby. The area is also known as Lacus
Excellentiae in Latin.

At the time of impact, the Lake of Excellence will be shrouded in
darkness - only slightly illuminated by light from the Earth in a
phenomenon called earthshine. The boundary between bright sunshine and
nighttime on the Moon will be located not far away, possibly allowing
material blown above the surface to reach altitudes high enough to be
lit by sunlight.

Ground controllers in Germany had to command a two-week series of
thruster firings to raise the low point of SMART-1's trek around the
Moon to push back the inevitable crash from about August 17 to the
current date of September 3. The plan also brought the forecasted impact
site into the direct view of scientists on the ground. If left
undisturbed, the 630-pound probe would have smacked into the far side of
the Moon facing away from Earth.

The set of orbit-raising maneuvers began June 19 and ended on July 2 -
about five days ahead of schedule.

Astronomers at observatories across the globe plan to try to see the
plume of debris ejected high above the lunar surface as SMART-1 drives
into the Moon. Organized groups at the European Southern Observatory in
Chile, Kitt Peak in Arizona, telescopes in Hawaii, and other locations
will attempt to spot the impact and its aftermath

The most favorable position for observing an on-time impact will be in
North and South America and Hawaii. There, the quarter Moon will be high
in the sky for prime viewing.

Larger telescopes could detect a flash at the moment of impact due to
vaporized hydrazine fuel. A few minutes later, dust and rocks thrown
high above the Moon might be seen. If the debris reaches an altitude of
over 12 miles, it could be lit by sunlight. If so, amateur astronomers
with smaller backyard telescopes could see the dust cloud backdropped by
the darker lunar surface.

We are calling upon astronomical observatories and amateurs worldwide
to participate in a coordinated observation effort with SMART-1,
including the final orbits until impact, said European Space Agency
SMART-1 project scientist Bernard Foing.

Instruments to be operating during SMART-1's final hours include an
infrared spectrometer, an X-ray spectrometer, and a tiny camera to take
pictures of the Moon as the spacecraft passes near the surface.

The material propelled into sunlight will be closely analyzed to
determine details such as its mineral composition and physical
properties. Some of the debris could be excavated from underground
during SMART-1's crash, so scientists are especially interested in
learning about the sub-surface of the Moon.

During SMART-1's final orbits, the spacecraft should be speeding just a
few miles above the lunar surface. Accurate predictions of the expected
impact time and location are hard to produce because of unknown
variations in topography along the probe's trajectory over the Moon.
Officials say an unexpected mountain or cliff could cause the craft to
crash earlier than anticipated.

By early September, SMART-1 will complete one orbit of the Moon about
every five hours. With each orbit's closest approach to the surface, the
probe will slowly descend further.

Two low passes before the most likely impact time are also being closely
watched in case SMART-1 hits the Moon early. If the spacecraft strikes
the Moon at 0037 GMT, observers in South America and the Canary Islands
will garner the best view of the event. One orbit earlier - at 1933 GMT
on September 2 - astronomers based in Europe and Africa will have the
best chance to view the crash.

At first contact, engineers believe SMART-1 will gently 

[meteorite-list] SMART-1 Image: Lomonosov - A Large Crater Filled By Lava

2006-07-25 Thread Ron Baalke

http://www.esa.int/esaSC/SEM1R6BUQPE_index_0.html

Lomonosov - a large crater filled by lava
SMART-1
European Space Agency 
25 July 2006

This image, taken by the advanced Moon Imaging Experiment (AMIE) on
board ESA's SMART-1 spacecraft, shows crater Lomonosov on the Moon's far
side.
 
AMIE obtained the image on 30 January 2006 from a distance of about 2100
kilometres from the surface, with a ground resolution of 190 metres per
pixel. The imaged area is centred at a latitude of 27.8º North and a
longitude of 98.6º East.

Crater Lomonosov is a nice example for a large crater (92 kilometres in
diameter) which was filled by lava after the impact, thus exhibiting a
flat floor. The terraced walls indicate 'slumping', that is sliding of
the rocks downwards due to gravity after the end of the impact. The
small craters inside Lomonosov are the result of impacts into this lava
floor which happened after the formation of Lomonosov.

Looking closely to the left half of the crater, one can see changes in
the brightness of the crater floor, resembling horizontal paint strokes.
These can be seen frequently in this area of the Moon and are ejecta
deposits of the young crater Giordano Bruno which is at about 300
kilometres distance.

The crater is named in honor of Mikhail Vassilievitch Lomonossov, a
Russian physicist (1711 - 1765). He was professor of physics at Saint
Petersburg university and devoted his live to the study of the
properties of matter and electricity.

 
For more information
 
Jean-Luc Josset, SPACE-X Space Exploration Institute
Email: jean-luc.josset @ space-x.ch

Bernard H. Foing, ESA SMART-1 Project Scientist
Email: bernard.foing @ esa.int

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[meteorite-list] Chladni's Heirs

2006-07-25 Thread Stefan Brandes

Congrat´s from Austria !

Chladni´s Heirs short : SAM

for S tefan, A ndi, M artin

to bundle their strengths to serve the collectors
that´s a motto!

All the best for the german task force ;)

Stefan







Collectors, enthusiasts, list!

The searching delegation of Chladni's Heirs* just returned from a
6-days-trip in Norway on the hunt for the new fall.
We set up a little website with an illustrated report:
http://www.meteoriten.com/norway.html





*Chladni's Heirs
was planned to be officially launched after a summer break,
now with this actual event you will already got to know our brand's name.

Chladni's Heirs is an amalgamation of your (hopefully soon) preferred
meteorite dealers:
Stefan Ralew
Andreas Gren
Martin Altmann
founded for the purpose to bundle their strengths to serve the collectors
even better than before, to assist them in all concerns more accurate and
faster and to offer them the enlarged and full palette of meteorites: 
irons,

rare and aesthetic common desert types, historic finds and falls at best
quality and competitive prices.

Although the official launch will be dated later,
we already accept congratulations :-)

Stefan Ralew
Andi Gren
Martin Altmann

Chladni's Heirs will take part in the Tucson show 2007


And now we sing:

There's a mineral shop down our street,
It's run by a German,
And they sells good things to collect,
But you should hear him speak,
When you ask him anything,
Never answers No,
He just yesses you to death,
And as he takes your dough he tells you:

Refrain:
Yes! We have no martians,
We have no martians today.
We've chondrites, and onions,
rumurutis and eucrites
And all kind of stones, and say,
We have an old fashioned Gibeon
Moroccan potato,
But yes! We have no martians,
We have no martians today!


Things were going well with him,
He wrote home to say,
Send me Patrick and Peter and Jim,
I need them right away,
When he got them in the shop,
There was fun, you bet,
'Cause when you asked them anything,
They answered in quartet: Oh,


And now all together:
Yes! We have no martians,
We have no martians today.
We've chondrites, and onions,
rumurutis and eucrites
And all kind of stones, and say,
We have an old fashioned Gibeon
Moroccan potato,
But yes! We have no martians,
We have no martians today!



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Meteorite-list@meteoritecentral.com
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Re: [meteorite-list] Chladni's Heirs

2006-07-25 Thread bernd . pauli
Chladni's Heirs short: SAM

I was just wondering if Uncle SAM is amused about such activities ;-)

Bernd

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[meteorite-list] Lomonosov Crater

2006-07-25 Thread bernd . pauli
Beautiful crater! It looks like a combination of craters
Copernicus, Tycho and Plato. A little bit of everything:

- the terraced walls and slumping of Tycho and Copernicus
- the smooth crater floor of Plato

.. scientifically a very interesting lunar feature!


Cheers,

Bernd

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[meteorite-list] Ad - 90 Great Auctions!

2006-07-25 Thread Adam Hupe
Dear List Members,

I have several excellent auctions ending this afternoon, most started at
just 99 cents.  I also loaded 12 more 1 kilo and 4 more 2 kilo lots of
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To see all of the too numerous to list outstanding auctions, click on this
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in comparison with other hammer stones. This example was started at just 99
cents with no reserve and is nowhere near what one would expect to pay for a
hammer stone:
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A 1.5 gram piece of the Anomalous Tooth Stone started at just 99 cents:
http://cgi.ebay.com/ws/eBayISAPI.dll?ViewItemitem=130008670626

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NWA 2918 CO3.0, the least metamorphosed CO in private hands!  I just talked
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...and several unclassified entire large stones at the same low price

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http://cgi.ebay.com/ws/eBayISAPI.dll?ViewItemitem=170009204646
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Thank you for looking and if you are bidding, good luck.


Best Regards,


Adam Hupe
The Hupe Collection
Team LunarRock
IMCA 2185
[EMAIL PROTECTED]




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Re: [meteorite-list] Chladni's Heirs NORWAY field report

2006-07-25 Thread tracy latimer
Indeed, thank you very much for sharing; for the benefit of those of us who 
can't go forth and search more than a short drive from our homes.


It seems that this fall will be carbonaceous.  Aside from Allende, Tagish, 
and the CR2 that has been scooped in multiple pieces from Saharan sands, 
don't they seem to mostly fall in clumps of only a few stones?  Given this 
(and the nature of the fall location) I'm not surprised more was not found.  
Did anyone offer to ransack the street sweeper's collection bin? :)


Tracy Latimer


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Re: [meteorite-list] SMART-1 Image: Lomonosov - A Large Crater Filled By Lava

2006-07-25 Thread E.P. Grondine
Hi - 

While the Moon lacks an atmosphere, which is required
for an airblast, isn't it more likely that what we're
seeing here is impact glass rather than lava?  

I can't see how lava would pool at such a shallow
depth, given that the Moon's core hsa been cooled for
some billions of years now.

I suppose we'll just have to wait for the Chinese
rover's results in 2018. 

good hunting,
Ed



--- Ron Baalke [EMAIL PROTECTED] wrote:

 
 http://www.esa.int/esaSC/SEM1R6BUQPE_index_0.html
 
 Lomonosov - a large crater filled by lava
 SMART-1
 European Space Agency 
 25 July 2006
 
 This image, taken by the advanced Moon Imaging
 Experiment (AMIE) on
 board ESA's SMART-1 spacecraft, shows crater
 Lomonosov on the Moon's far
 side.
  
 AMIE obtained the image on 30 January 2006 from a
 distance of about 2100
 kilometres from the surface, with a ground
 resolution of 190 metres per
 pixel. The imaged area is centred at a latitude of
 27.8º North and a
 longitude of 98.6º East.
 
 Crater Lomonosov is a nice example for a large
 crater (92 kilometres in
 diameter) which was filled by lava after the impact,
 thus exhibiting a
 flat floor. The terraced walls indicate 'slumping',
 that is sliding of
 the rocks downwards due to gravity after the end of
 the impact. The
 small craters inside Lomonosov are the result of
 impacts into this lava
 floor which happened after the formation of
 Lomonosov.
 
 Looking closely to the left half of the crater, one
 can see changes in
 the brightness of the crater floor, resembling
 horizontal paint strokes.
 These can be seen frequently in this area of the
 Moon and are ejecta
 deposits of the young crater Giordano Bruno which is
 at about 300
 kilometres distance.
 
 The crater is named in honor of Mikhail
 Vassilievitch Lomonossov, a
 Russian physicist (1711 - 1765). He was professor of
 physics at Saint
 Petersburg university and devoted his live to the
 study of the
 properties of matter and electricity.
 
  
 For more information
  
 Jean-Luc Josset, SPACE-X Space Exploration Institute
 Email: jean-luc.josset @ space-x.ch
 
 Bernard H. Foing, ESA SMART-1 Project Scientist
 Email: bernard.foing @ esa.int
 
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[meteorite-list] Chladni's Heirs NORWAY field report + clumps of only a few stones

2006-07-25 Thread bernd . pauli
Tracy wrote:


...don't they seem to mostly fall in clumps of only a few stones?

Al Rais (CR2): A total weight of 160g fell near the city of Medina
Alais (CI): 2 stones, of about 4 and 2 kg respectively, fell
Banten (CM2): Four individuals, totalling 629g, were recovered
Bells (CM2): 6 fragments picked up
Boriskino (CM2): 2 stones recovered, 1165.6g together, 3 others destroyed
Crescent (CM2): Two stones were found, 72.7 g + 5.7 g
Erakot (CM2): One stone of 113g was recovered
Felix(CO3.3): a stone of about 7 lb was found
Haripura (CM2): a stone fell and broke into 2 pieces
Ivuna (CI): Two or three stones fell at Ivuna
Kaba (CV3): a stone of about 3 kg was found
Kaidun (CR): a single mass of 841.6g recovered from small impact pit
Kobe (CK4): one stone was recovered ... the total mass is 136 g
Mighei (CM2): a stone of over 8 kg was seen to fall
Mokoia (CV3): several stones seen to fall, 2 of about 5lb each recovered
Nawapali (CM2): 3 stones appear to have fallen but only 3 small fragments
of about 30g, 20g and 10g preserved
Ningqiang (CK3): a single stone, in 4 fragments of total weight 4.6 kg
Nogoya (CM2): a stone of about 4 kg fell
Orgueil (CI): about 20 stones
Ornans (CO3.4): a stone of about 6 kg fell and broke into two pieces
Pollen (CM2): a stone of 253.6g fell on the Pollen farm
Revelstoke (CI): search yielded 2 small fragments, together about 1 g
Sayama (CM2): a 430 gr stone was found
Tonk (CI): shower of small stones; a total weight of 7.7 g collected
Vigarano (CV3.3): 11.5 kg and 4.5 kg


Cheers,

Bernd

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Re: Re: [meteorite-list] Chladni's Heirs

2006-07-25 Thread Alexander Seidel
Bernd wrote:

 Chladni's Heirs short: SAM
 I was just wondering if Uncle SAM is amused about such activities ;-) 
 Bernd


Then again: qualified competition imo is good and healthy competition!

And rest assured they are even more than simply qualified when it gets down to 
knowledge about meteorites and customer support. If you have ever
dealt with any one of the guys individually, just as I did, you know what it 
means when they are bundling their efforts right now...

So, uncle SAM, don´t worry, be happy! :-)

Alex
Berlin/Germany


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[meteorite-list] Bessey specks for young people

2006-07-25 Thread E.P. Grondine
Hi all - 

I don't know why I'm bringing this up now (with some
300 messages yet to go through from the last several
weeks), but the thought is striking me that Bessey
Specks make good gifts for young people.

Given that, how do you think they should be packaged?
What prices?

Since I've been away from the list for the last
several years, I don't know what Moon and Mars
materials were recovered during that time, or how they
were prepared.

(my report on fire starting and thanks to Piper
Hollier  for the Canyon Diablo will be along shortly)

good hunting, 
Ed




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[meteorite-list] Lahoma Meteorite

2006-07-25 Thread bernd . pauli
Michael Cottingham wrote:

1. one very pretty meteorite
2. superb slices
3. L5 beauty
4. jade-green matrix
5. loads of metal
6. dark inclusions
7. very sweet meteorite

I concur and because I do I couldn't help buying three of these
pretty, jade-green, metal-rich (one of my specimens has a very
impressive oval FeNi/troilite inclusion), shock-veined beauties
featuring conspicuous dark inclusions. It was kept in a farmer's
front yard for 35 years. I am looking forward to meeting them
in person!


Cheers,

Bernd

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[meteorite-list] Tales of strange meteorites wanted

2006-07-25 Thread chris aubeck

Hi list,

If anyone comes across any claims or anecdotes about meteorites with
strange properties, bearing mysterious marks or containing strange
artifacts, do let me know so I can add them to my archive of
meteorite-related lore.

Many thanks to those who have helped me in the past with this ongoing project.

Kind regards,

Chris
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[meteorite-list] Rocks From Space Picture of the Day - July 26, 2006

2006-07-25 Thread SPACEROCKSINC
http://www.spacerocksinc.com/July_26.html  

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[meteorite-list] Iron Meteorites as the Not-So-Distant Cousins of Earth

2006-07-25 Thread Ron Baalke

http://www.psrd.hawaii.edu/July06/asteroidGatecrashers.html

Iron Meteorites as the Not-So-Distant Cousins of Earth
Planetary Science Research Discoveries
July 21, 2006

--- Numerical simulations suggest that some iron meteorites are
fragments of the long lost precursor material that formed the Earth and
other terrestrial planets.

Written by William F. Bottke (Southwest Research Institute, Boulder, CO) 
and Linda M. V. Martel (Hawai'i Institute of Geophysics and Planetology)

Iron meteorites are fragments from the cores of small differentiated
asteroids (20-200 kilometers in diameter) that formed very early in Solar 
System history. They are commonly assumed to have originated in the same 
region as most stony meteorite parent bodies, namely the main asteroid belt 
located between Mars and Jupiter. A new paper in the journal Nature by William 
Bottke, David Nesvorný, and Robert Grimm (Southwest Research Institute, 
Boulder, Colorado) along with Alessandro Morbidelli and David O'Brien
(Observatoire de la Cote d'Azure, Nice, France), however, finds that the
iron meteorites may have come from a different and possibly much more
intriguing place. According to their numerical simulations that tracked
the dynamical evolution of Moon- to Mars-sized planetary embryos
interacting with tens of thousands of test bodies during the first 10
million years of Solar System evolution, many iron meteorite parent
bodies formed and fragmented in the same region where Mercury, Venus,
Earth and Mars are found today. The fast accretion times of
planetesimals in this zone allowed heat produced by the decay of
short-lived radioactive isotopes like
26Al to melt and differentiate many of these objects into core, mantle,
and crust. At the same time, gravitational interactions with planetary
embryos increased their mutual impact velocities, enough that these
planetesimals broke apart when they struck one another. The net result
was the production of millions of fragments continually jostled about by
planetary embryos. Over millions of years, a small fraction of this
differentiated debris was scattered into the innermost region of the
main belt, where it then stayed for billions of years until chance
collisional and dynamical events sent it on a crash course to Earth.
Bottke and colleagues' prediction of these asteroid main belt
gatecrashers could mean that some of the iron meteorites we hold in our
hands today are pieces of the same precursor fabric that formed the
Earth and other terrestrial planets.

Reference:

* Bottke, W. F., D. Nesvorný, R. E. Grimm, A. Morbidelli, and D. P.
  O'Brien (2006) Iron Meteorites as Remnants of Planetesimals Formed
  in the Terrestrial Planet Region. Nature, v. 439, p. 821-824. [pdf
  link http://www.boulder.swri.edu/~bottke/Reprints/Reprints.html
  opens in a new window]



The Story Told by Iron Meteorites and Main Belt Asteroids

Numerical simulations have demonstrated that most of the stony and iron
meteorites found today in worldwide collections came from asteroids in
the main belt. For this reason, it is often taken as a given that their
parent bodies formed there as well. This assumption, while reasonable
for many meteorite types, does not do a very satisfying job of
explaining the origin of the iron meteorites.

Most irons are pieces of the cores of distinct, small (20 to 200
kilometer-diameter) differentiated asteroids. We know this from
chemical, petrographic (mineralogical and textural), and cooling rate
studies of iron meteorites performed in laboratories. Very few irons are
thought to be impact melts or fragments from a few, larger (500
kilometer-diameter) differentiated bodies.

[showing differentiation http://www.mnh.si.edu/earth/text/5_1_4_0.html]

This series of graphics from the Smithsonian depicts the process of
differentiation. Pictured left to right: Dust and grains clump together
until a small body forms. The growing body heats up inside and begins to
melt. Dense molten metal pools and sinks towards the center core of the
body. Less dense silicate liquid, or magma, rises towards the surface,
leaving dense residues of solid minerals in the mantle. The result is a
differentiated body with a core, mantle, and crust. [Click image to view
the source page.]

The fact that we have iron core fragments attests to the powerful
collisions that repeatedly shattered their parent bodies during the
early history of our Solar System. In our meteorite collections today,
irons represent over two-thirds of the unique parent bodies sampled
among all meteorites. This large percentage would suggest that
differentiated parent bodies and their fragments are common in the main
asteroid belt. The problem is there is little observational evidence to
support this idea, and it's not for lack of looking.

Despite intense searches with telescopes equipped with cameras and
spectrographs, the only clearly intact 

[meteorite-list] Chladni's Heirs NORWAY field report + clumps of only a few stones

2006-07-25 Thread Steve Schoner
Humm...
How about Kainsaz... Over 200 kg of CO 3's ?
And seeing that this fall in Norway is 5 km between the largest and smallest stone with one other reportedly heard but not recovered in Moss indicates a strewnfield. I doubt that 200 kg fell, however I would not be surprised if many more will turn up between the ones so far recovered.
Once the Norwegians get back from their Summer vacations and look through their gardens, who knows what they might find.
Steve Schoner IMCA# 4470

Tracy wrote: "...don't they seem to mostly fall in clumps of only a few stones?" Al Rais (CR2): A total weight of 160g fell near the city of Medina Alais (CI): 2 stones, of about 4 and 2 kg respectively, fell Banten (CM2): Four individuals, totalling 629g, were recovered Bells (CM2): 6 fragments picked up Boriskino (CM2): 2 stones recovered, 1165.6g together, 3 others destroyed Crescent (CM2): Two stones were found, 72.7 g + 5.7 g Erakot (CM2): One stone of 113g was recovered Felix(CO3.3): a stone of about 7 lb was found Haripura (CM2): a stone fell and broke into 2 pieces Ivuna (CI): Two or three stones fell at Ivuna Kaba (CV3): a stone of about 3 kg was found Kaidun (CR): a single mass of 841.6g recovered from small impact pit Kobe (CK4): one stone was recovered ... the total mass is 136 g Mighei (CM2): a stone of over 8 kg was seen to fall Mokoia (CV3): several stones seen to fall, 2 of about 5lb each recovered Nawapali (CM2): 3 stones appear to have fallen but only 3 small fragments of about 30g, 20g and 10g preserved Ningqiang (CK3): a single stone, in 4 fragments of total weight 4.6 kg Nogoya (CM2): a stone of about 4 kg fell Orgueil (CI): about 20 stones Ornans (CO3.4): a stone of about 6 kg fell and broke into two pieces Pollen (CM2): a stone of 253.6g fell on the Pollen farm Revelstoke (CI): search yielded 2 small fragments, together about 1 g Sayama (CM2): a 430 gr stone was found Tonk (CI): shower of small stones; a total weight of 7.7 g collected Vigarano (CV3.3): 11.5 kg and 4.5 kg Cheers, Bernd 
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Re: AW: [meteorite-list] Chladni's Heirs NORWAY field report

2006-07-25 Thread joseph_town
I hope the lyrics of this song prove to be inapplicable. It's a good choice 
nonetheless.

Bill

 -- Original message --
From: Martin Altmann [EMAIL PROTECTED]
 Hi Moni,
 
 if they won't behave, like that European team from a country starting with
 P trampling through the gardens ploughing up the flowerbeds under the eyes
 of the dumbfounded house owners, I wish all success to the American party.
 
 Hmm, the song will work with the melody of
 CohnSilver: Yes, we have no bananas today, 1923
 
 But later I guess, we will compose a new one :-)
 
 Buckl...oops, no, better now:
 
 Kindest Regards
 Chladni's Heirs
 
 Stefan Ralew
 Andi Gren
 Martin Altmann
 
 
 -Ursprüngliche Nachricht-
 Von: [EMAIL PROTECTED]
 [mailto:[EMAIL PROTECTED] Im Auftrag von moni
 Waiblinger-Seabridge
 Gesendet: Dienstag, 25. Juli 2006 00:29
 An: [EMAIL PROTECTED]; meteorite-list@meteoritecentral.com
 Betreff: RE: [meteorite-list] Chladni's Heirs NORWAY field report
 
 Hi list members,
 
 Stefan Ralew
 Andi Gren
 Martin Altmann and Morten Bilet,
 
 Thank you for this report!!!
 
 Its so wonderful to find out more of this fall without having to spend all 
 this money to get there, unless of course one finds a piece!
 Well, let's see how our American friends will do!   ;-)
 
 
 With best regards,
 Moni
 
 PS. Martin, what is the melody for this song?
 
 
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[meteorite-list] Happy Birthday to....

2006-07-25 Thread M come Meteorite Meteorites
Barbotan, Beaver-Harrison, Parambu ( and I have in
collection )Darryl Pitt and to me...

Matteo

ps= I need Gifu and Gross-Divina

M come Meteorite - Matteo Chinellato
Via Triestina 126/A - 30030 - TESSERA, VENEZIA, ITALY
Email: [EMAIL PROTECTED]
Sale Site: http://www.mcomemeteorite.it 
Collection Site: http://www.mcomemeteorite.info
MSN Messanger: spacerocks at hotmail.com
EBAY.COM:http://members.ebay.com/aboutme/mcomemeteorite/

Chiacchiera con i tuoi amici in tempo reale! 
 http://it.yahoo.com/mail_it/foot/*http://it.messenger.yahoo.com 
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[meteorite-list] NORWAY meteorite hunt

2006-07-25 Thread meteoritehunter
Hi everyone.
 Well,  it is 12:24 am here in Moss Norway, and I just came up from some heavy 
drinking with a heck of a batch of meteorite hunters. We have Robert Ward, 
Robert Haag,  and myself representing the USA. Moritz Karl, Alexander Gehler, 
Rainer Bartowtzewich (sp?) and Thomas Kurtz from Germany here tonight. WE saw 
many others today and yesterday though, even Poland was well represented. None 
from France, or Austria, or the UK though.
  Now, on to the meteorite! It IS A CO, Carbonaceous. NO DOUBT unless 
it gets some wierd exception in classification. So I was right, as were many 
others who guessed CO2 or CO3. It is a meteorite that will take your breath 
away! It also had  the misfortune of falling in one of the worst imaginable 
places for searching! This area is of course, absolutely beautiful, fjords, 
trees, endless berrys to eat like strawberrys, blueberrys, and raspberrys, lots 
of tall, blonde women, and it is not 400,000 degrees like Tucson right now.
What is wrong is that it is high growing season, so every flat surface is being 
farmed with full grown wheat, barley, peas, cabbage, etc. Every other surface 
is extremely heavy forest with deep layers of moss that you sink in, lakes, 
swamps, or fjords full of cruise ships. Their is absolutely no place to easily 
search other than a few parks and shopping centers and industrial sites.
From the siye of the fireball, it is certain  that there are many pieces, but 
highly unlikely that much will be found other than by locals in their yards, 
and most locals are on vacation and not here.
So to end so that I can get some sleep for the first time in 3 days, there is 
little news to report so far other than Norway got lucky with a fabulous new 
CC. Now it is time to feed the mosquitoes while I sleep for the few hours of 
darkness there is in this part of the world at this time of the year.
Michael Farmer
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Re: [meteorite-list] Chladni's Heirs NORWAY field report + clumps of only a few stones

2006-07-25 Thread Jason Utas
Hello Bernd, Tracy, All,
Anyone can make a statement look good if they exclude all contrary evidence. 
Aside from Allende(2+t), Tagish Lake (10kg), and NWA 801(unknown kg)? 

Murchison 100+kg
DaG CO3's with amain mass of 95kg alone
Kainsaz 200+kg
Karoonda ~50kg
Even Bencubbin and Gujba were at least a hundred kilos each.

Anyoneknow of others? I admit didn't put too much time into the research for this...just quick tkw referencing. 

Tracy's original statement of ...don't they seem to mostly fall in clumps of only a few stones? applies to all meteorite types, not just carbonaceous chondrites. Have a look at the catalogue of meteorites; the first page alone is enough for me, but if you continue reading, you'll see what I mean. 


If there's any discrepancy in these ratios at all, my best guess is that it would be due to their greater tendency to fragment while in the atmosphere due to their increased relative friability to other meteorites. Either that or the fact thatmany tend to turn into mud within a few days orweeks of falling. 



Yeah, there aren't too many large falls, but then again, how many largefalls are there in general? Not many.

Regards,
Jason
On 25 Jul 2006 18:27:56 UT, 
[EMAIL PROTECTED] 
[EMAIL PROTECTED]  wrote: 
Tracy wrote:...don't they seem to mostly fall in clumps of only a few stones?
Al Rais (CR2): A total weight of 160g fell near the city of MedinaAlais (CI): 2 stones, of about 4 and 2 kg respectively, fellBanten (CM2): Four individuals, totalling 629g, were recoveredBells (CM2): 6 fragments picked up 
Boriskino (CM2): 2 stones recovered, 1165.6g together, 3 others destroyedCrescent (CM2): Two stones were found, 72.7 g + 5.7 gErakot (CM2): One stone of 113g was recoveredFelix(CO3.3): a stone of about 7 lb was found 
Haripura (CM2): a stone fell and broke into 2 piecesIvuna (CI): Two or three stones fell at IvunaKaba (CV3): a stone of about 3 kg was foundKaidun (CR): a single mass of 841.6g recovered from small impact pit 
Kobe (CK4): one stone was recovered ... the total mass is 136 gMighei (CM2): a stone of over 8 kg was seen to fallMokoia (CV3): several stones seen to fall, 2 of about 5lb each recoveredNawapali (CM2): 3 stones appear to have fallen but only 3 small fragments 
 of about 30g, 20g and 10g preservedNingqiang (CK3): a single stone, in 4 fragments of total weight 4.6 kgNogoya (CM2): a stone of about 4 kg fellOrgueil (CI): about 20 stonesOrnans (CO3.4
 ): a stone of about 6 kg fell and broke into two piecesPollen (CM2): a stone of 253.6g fell on the Pollen farmRevelstoke (CI): search yielded 2 small fragments, together about 1 gSayama (CM2): a 430 gr stone was found 
Tonk (CI): shower of small stones; a total weight of 7.7 g collectedVigarano (CV3.3): 11.5 kg and 4.5 kgCheers,Bernd__Meteorite-list mailing list 

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Re: [meteorite-list] NORWAY meteorite hunt

2006-07-25 Thread Darren Garrison
On Tue, 25 Jul 2006 22:38:30 +, you wrote:

Hi everyone.
 Well,  it is 12:24 am here in Moss Norway, and I just came up from some heavy 
 drinking with a 
heck of a batch of meteorite hunters. We have Robert Ward, Robert Haag,  and 
myself 
representing the USA. Moritz Karl, Alexander Gehler, Rainer Bartowtzewich 
(sp?) and Thomas
 Kurtz from Germany here tonight. WE saw many others today and yesterday 
 though, 

Maybe you should go look for the one from a couple-three weeks ago while you are
there.
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Re: [meteorite-list] NORWAY meteorite hunt

2006-07-25 Thread Pat Brown
Hi All, 

Chances like this don't come along very often, so
please forgive my boasting.

I am a small fish in a sea of much larger fish... 
but I can lay claim to be the first to post to the
meteorite mail list that this Norway meteorite
was... carbonacious!

Back to your regularly scheduled mail list..

Best Regards to All, 
   Pat Brown

--- [EMAIL PROTECTED] wrote:

 Hi everyone.
  Well,  it is 12:24 am here in Moss Norway, and I
 just came up from some heavy drinking with a heck of
 a batch of meteorite hunters. We have Robert Ward,
 Robert Haag,  and myself representing the USA.
 Moritz Karl, Alexander Gehler, Rainer Bartowtzewich
 (sp?) and Thomas Kurtz from Germany here tonight. WE
 saw many others today and yesterday though, even
 Poland was well represented. None from France, or
 Austria, or the UK though.
   Now, on to the meteorite! It IS A CO,
 Carbonaceous. NO DOUBT unless it gets some wierd
 exception in classification. So I was right, as were
 many others who guessed CO2 or CO3. It is a
 meteorite that will take your breath away! It also
 had  the misfortune of falling in one of the worst
 imaginable places for searching! This area is of
 course, absolutely beautiful, fjords, trees, endless
 berrys to eat like strawberrys, blueberrys, and
 raspberrys, lots of tall, blonde women, and it is
 not 400,000 degrees like Tucson right now.
 What is wrong is that it is high growing season, so
 every flat surface is being farmed with full grown
 wheat, barley, peas, cabbage, etc. Every other
 surface is extremely heavy forest with deep layers
 of moss that you sink in, lakes, swamps, or fjords
 full of cruise ships. Their is absolutely no place
 to easily search other than a few parks and shopping
 centers and industrial sites.
 From the siye of the fireball, it is certain  that
 there are many pieces, but highly unlikely that much
 will be found other than by locals in their yards,
 and most locals are on vacation and not here.
 So to end so that I can get some sleep for the first
 time in 3 days, there is little news to report so
 far other than Norway got lucky with a fabulous new
 CC. Now it is time to feed the mosquitoes while I
 sleep for the few hours of darkness there is in this
 part of the world at this time of the year.
 Michael Farmer
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Re: [meteorite-list] Rocks From Space Picture of the Day - July 26, 2006

2006-07-25 Thread Pat Brown
This is a super nice, dare I saw sexy find!!

Pat

--- [EMAIL PROTECTED] wrote:

 http://www.spacerocksinc.com/July_26.html  
 
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