Re: [meteorite-list] Meteorite Pairing Discussions

2010-01-19 Thread Zelimir Gabelica

Hi John,

NWA 4024 is indeed a nice example of the 
discrepancy between Met. Bull. data and the 
amount of stuff circulating on the market.


This is perfectly illustrated if you compare the 
Met. Bull. write up regarding NWA 4024 an look at 
the photos included at the end of the same report.
There are some 15 pieces illustrated, coming from 
various sources. Although weights are not 
mentioned, a rough evaluation of the volume of 
the pieces (comparison with the scale cubes) 
leads to evaluate that the total weight of the 
illustrated pieces should largely overstep 100 g, probably more.
Not mentioning that the pieces pictured probably 
represent only a small fraction of what is really 
available as 'NWA 4024 in collections.


I have in collection a 4.43 g end section (got from Hanno Strufe).
But my own write up states that Mike Farmer 
reported at the time (2006) that the tkw was at least 745 grams.
He explicitly explained this discrepancy by the 
following argumentive comment: first piece sold, 
more pieces come out, which is, as we know, not really a surprise.


Nothing is mentioned officially about pairings 
and I don't know whether this meteorite is also 
being sold under another NWA N° but I guess the 
pics in the Met. Bull. suggest that all the 15 pieces were called NWA 4024.


The tkw of a meteorite is indeed rarely updated 
officially (by the Nom Com and thus reported in 
the Met. Bulls.) probably because nobody writes 
them to update the old tkw. I agree that the Nom 
Com should not be blamed for that.


As a typical example (among many others) the 
official tkw reported in Met. Bull. for Chiang 
Khan is still 367 grams, while everybody now agrees that it is of several kg.
When helping Mike Jensen to update the 2008 
edition of  Meteorites from A to Z, I reported 
him several such examples and, in some obvious 
cases, the actual tkw was updated (with, as 
reference: numerous sources including internet, 
personal communications and professional experience.
Needless to say that this updating is not 
official because not (yet ?) agreed by the Nom. Com.
For the cited example of Chiang Khan, we agreed 
to the put, as tkw, 7...@7.0+ kg, which is more 
realistic regarding the present market, although 
not official as I agree only the Met. Bull. (Nom. 
Com.) should act as official reference.


There is some pertinent work needed here and I am 
convinced many of us from the List and elsewhere 
can help in trying to provide more correct figures to the Nom. Com.


Zelimir


At 04:38 19/01/2010, John.L.Cabassi wrote:

G'Day List
This has been a very interesting read. Quite some time ago, I brought up
the question about NWA 4024, which apparently on the card that
accompanied it and the Met Bull stated a TKW of 38.1g.  But there's
definitely alot more out there ??? Is there pairing going on here?

http://tin.er.usgs.gov/meteor/metbull.php?sea=nwasfor=namesants=falls
=valids=stype=containslrec=50map=gebrowse=country=Allsrt=namecat
eg=Winonaitesmblist=Allrect=phot=snew=0pnt=Normaltablecode=34296


And now for another, I purchased this off of Tom some time back. NWA
231, the met bull lists is as being provisional, it has yet to be
classified. The main mass was 1054g. What I have is 1048g, 6 grams are
missing; I think due to polishing a window. But I confirmed with Michael
C.  and it was confirmed. The label on the rock states NWA 231 so
everything checks out. But it's yet to be classified. I have not found
the time to go ahead with this, but I was curious that NWA numbers were
handed out prior to being classified.

http://tin.er.usgs.gov/meteor/metbull.php?sea=nwa+231sfor=namesants=f
alls=valids=stype=containslrec=50map=gebrowse=country=Allsrt=name
categ=Allmblist=Allrect=phot=snew=0pnt=Normaltablecode=31470

Any thoughts?

Cheers
John
IMCA # 2125

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Prof. Zelimir Gabelica
Université de Haute Alsace
ENSCMu, Lab. GSEC,
3, Rue A. Werner,
F-68093 Mulhouse Cedex, France
Tel: +33 (0)3 89 33 68 94
Fax: +33 (0)3 89 33 68 15 


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Re: [meteorite-list] Meteorite Pairing Discussions

2010-01-19 Thread André Knöfel
Hello Zelimir

 This is perfectly illustrated if you compare the 
 Met. Bull. write up regarding NWA 4024 an look at 
 the photos included at the end of the same report.
 There are some 15 pieces illustrated, coming from 
 various sources. Although weights are not 
 mentioned, a rough evaluation of the volume of 
 the pieces (comparison with the scale cubes) 
 leads to evaluate that the total weight of the 
 illustrated pieces should largely overstep 100 g, probably more.

The total weight of the pieces from the EoM are 39.565g ...

Regards

André
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Re: [meteorite-list] Meteorite Pairing Discussions

2010-01-19 Thread Jason Utas
Hello John, Zelimir, All,
I've held samples of both; NWA 4024 is indistinguishable from NWA 2680.

http://www.arizonaskiesmeteorites.com/AZ_Skies_Links/NWA_2680/index.html

http://www.meteoriteguy.com/catalog/nwa4024.htm

It was likely misidentified the second time around because the sample
sent in for analysis was too small for an accurate study - or perhaps
the person who performed the analysis simply wasn't expecting an iron.
 Either way, it's funny -  an analysis based solely on the study of a
clast that comprises at most ~30-40% of the total volume of the
meteorite...I've never seen that done before.
It's a IAB with silicate inclusions - a pretty one, but an example
that's not crazily different from a few already-known irons.  Oh, and
it has winonaite-type silicate inclusions.  Just like Campo del Cielo
and many other IAB's...it's pretty typical in that respect.
We purchased a ~40g individual as a new iron in Tucson three or four
years ago; there were hundreds of small individuals of this iron
available at the time, totaling at least several kilograms (most
weighed only a few grams; Dean Bessey sold some of them on ebay later
that year, again, misidentified, and mixed with small mesosiderite
fragments).  In Tucson they were being sold as Zagora; we were
surprised to find a very fine pattern after we removed an end from
ours for analysis.
Based on what I have seen personally, I would estimate the TKW of the
find to be at least ten kilograms, but knowing NWA, there could be
(and likely is) much, much more.
Regards,
Jason

On Tue, Jan 19, 2010 at 2:58 AM, Zelimir Gabelica
zelimir.gabel...@uha.fr wrote:
 Hi John,

 NWA 4024 is indeed a nice example of the discrepancy between Met. Bull. data
 and the amount of stuff circulating on the market.

 This is perfectly illustrated if you compare the Met. Bull. write up
 regarding NWA 4024 an look at the photos included at the end of the same
 report.
 There are some 15 pieces illustrated, coming from various sources. Although
 weights are not mentioned, a rough evaluation of the volume of the pieces
 (comparison with the scale cubes) leads to evaluate that the total weight of
 the illustrated pieces should largely overstep 100 g, probably more.
 Not mentioning that the pieces pictured probably represent only a small
 fraction of what is really available as 'NWA 4024 in collections.

 I have in collection a 4.43 g end section (got from Hanno Strufe).
 But my own write up states that Mike Farmer reported at the time (2006) that
 the tkw was at least 745 grams.
 He explicitly explained this discrepancy by the following argumentive
 comment: first piece sold, more pieces come out, which is, as we know, not
 really a surprise.

 Nothing is mentioned officially about pairings and I don't know whether this
 meteorite is also being sold under another NWA N° but I guess the pics in
 the Met. Bull. suggest that all the 15 pieces were called NWA 4024.

 The tkw of a meteorite is indeed rarely updated officially (by the Nom Com
 and thus reported in the Met. Bulls.) probably because nobody writes them to
 update the old tkw. I agree that the Nom Com should not be blamed for that.

 As a typical example (among many others) the official tkw reported in Met.
 Bull. for Chiang Khan is still 367 grams, while everybody now agrees that it
 is of several kg.
 When helping Mike Jensen to update the 2008 edition of  Meteorites from A
 to Z, I reported him several such examples and, in some obvious cases, the
 actual tkw was updated (with, as reference: numerous sources including
 internet, personal communications and professional experience.
 Needless to say that this updating is not official because not (yet ?)
 agreed by the Nom. Com.
 For the cited example of Chiang Khan, we agreed to the put, as tkw, 7...@7.0+
 kg, which is more realistic regarding the present market, although not
 official as I agree only the Met. Bull. (Nom. Com.) should act as official
 reference.

 There is some pertinent work needed here and I am convinced many of us from
 the List and elsewhere can help in trying to provide more correct figures to
 the Nom. Com.

 Zelimir


 At 04:38 19/01/2010, John.L.Cabassi wrote:

 G'Day List
 This has been a very interesting read. Quite some time ago, I brought up
 the question about NWA 4024, which apparently on the card that
 accompanied it and the Met Bull stated a TKW of 38.1g.  But there's
 definitely alot more out there ??? Is there pairing going on here?

 http://tin.er.usgs.gov/meteor/metbull.php?sea=nwasfor=namesants=falls
 =valids=stype=containslrec=50map=gebrowse=country=Allsrt=namecat
 eg=Winonaitesmblist=Allrect=phot=snew=0pnt=Normaltablecode=34296


 And now for another, I purchased this off of Tom some time back. NWA
 231, the met bull lists is as being provisional, it has yet to be
 classified. The main mass was 1054g. What I have is 1048g, 6 grams are
 missing; I think due to polishing a window. But I confirmed with Michael
 C.  and it was confirmed. 

Re: [meteorite-list] Pairing discussion/questions

2010-01-19 Thread Jeff Grossman
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 Geological Survey  fax:   (703) 648-6383
954 National Center
Reston, VA 20192, USA


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[meteorite-list] Rocks from Space Picture of the Day - January 19, 2010

2010-01-19 Thread Michael Johnson
http://www.rocksfromspace.org/January_19_2010.html
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[meteorite-list] NWA 4024/2680

2010-01-19 Thread Zelimir Gabelica

Hi Jason,

Excellent link for NWA 4024 compared to 2680 (Birdsell).
From what I just can discern, I am convinced 
2680 is exactly the same material as 4024.
See, as comparison, the pics of both meteorites 
added at the end of their respective Met. Bull 
reports (although NWA 2680 is still provisional, there are pics attached).

In particular Mirko Graul provided pics of both.
Here they are, for comparison:

NWA 2680:

http://tin.er.usgs.gov/meteor/get_original_photo.php?recno=5645813

and NWA 4024:

http://tin.er.usgs.gov/meteor/get_original_photo.php?recno=5645817

Very similar slices, almost same pattern (look at details!)

My modest suggestion:

Owing to the fact that NWA 2680 is still 
provisional, why not suggesting to this specific 
classification working team (Zolensky  al ?) to 
conclude (after a thorough  re-examination) that 
both meteorites are the same and thus also 
consider to maintain only one NWA number, thus 
that NWA 2680 is identical to NWA 4024 (that 
should have priority because first classified)?


But here the question is perhaps even more 
complicated because NWA 4024 is said to be a 
winonaite, while it now appears obvious that only 
one (or a few) achondritic clast(s) were analyzed 
in it, not the (major ?) iron found all around (that is IAB ungr.).
It would then be wise to fully re-analyze both 
materials (ideally by the same team) and conclude.
If there rises evidence that both are the same, 
then I guess there should come an agreement for a common type and name ?


Sorry, I am not in the Nom Com nor I know how 
they would proceed in such a case, so perhaps my suggestion is very naive.
I therefore expect more comments from Nom Com 
experts and am ready to humbly accept their conclusions whatever they be.


This is here only one typical example of 
something that could still be done, because NWA 2680 is not yet official.

There are probably other such favorable examples.
Solving them, even if progressively, will push 
the pairing problem one step forward, though it 
is obvious, as Jeff pointed out, that this 
pairing problem is really very difficult (I'd say 
impossible) to solve completely.



Zelimir

At 12:56 19/01/2010, Jason Utas wrote:

Hello John, Zelimir, All,
I've held samples of both; NWA 4024 is indistinguishable from NWA 2680.

http://www.arizonaskiesmeteorites.com/AZ_Skies_Links/NWA_2680/index.html

http://www.meteoriteguy.com/catalog/nwa4024.htm

It was likely misidentified the second time around because the sample
sent in for analysis was too small for an accurate study - or perhaps
the person who performed the analysis simply wasn't expecting an iron.
 Either way, it's funny -  an analysis based solely on the study of a
clast that comprises at most ~30-40% of the total volume of the
meteorite...I've never seen that done before.
It's a IAB with silicate inclusions - a pretty one, but an example
that's not crazily different from a few already-known irons.  Oh, and
it has winonaite-type silicate inclusions.  Just like Campo del Cielo
and many other IAB's...it's pretty typical in that respect.
We purchased a ~40g individual as a new iron in Tucson three or four
years ago; there were hundreds of small individuals of this iron
available at the time, totaling at least several kilograms (most
weighed only a few grams; Dean Bessey sold some of them on ebay later
that year, again, misidentified, and mixed with small mesosiderite
fragments).  In Tucson they were being sold as Zagora; we were
surprised to find a very fine pattern after we removed an end from
ours for analysis.
Based on what I have seen personally, I would estimate the TKW of the
find to be at least ten kilograms, but knowing NWA, there could be
(and likely is) much, much more.
Regards,
Jason

On Tue, Jan 19, 2010 at 2:58 AM, Zelimir Gabelica
zelimir.gabel...@uha.fr wrote:
 Hi John,

 NWA 4024 is indeed a nice example of the 
discrepancy between Met. Bull. data

 and the amount of stuff circulating on the market.

 This is perfectly illustrated if you compare the Met. Bull. write up
 regarding NWA 4024 an look at the photos included at the end of the same
 report.
 There are some 15 pieces illustrated, coming from various sources. Although
 weights are not mentioned, a rough evaluation of the volume of the pieces
 (comparison with the scale cubes) leads to 
evaluate that the total weight of

 the illustrated pieces should largely overstep 100 g, probably more.
 Not mentioning that the pieces pictured probably represent only a small
 fraction of what is really available as 'NWA 4024 in collections.

 I have in collection a 4.43 g end section (got from Hanno Strufe).
 But my own write up states that Mike Farmer 
reported at the time (2006) that

 the tkw was at least 745 grams.
 He explicitly explained this discrepancy by the following argumentive
 comment: first piece sold, more pieces come 
out, which is, as we know, not

 really a surprise.

 Nothing is mentioned officially about 
pairings and I don't know 

Re: [meteorite-list] NWA 4024/2680

2010-01-19 Thread Marcin Cimala

Hi
You can add to this also my number NWA 5980. Its paired to 4024
TKW 298g

-[ MARCIN CIMALA ]-[ I.M.C.A.#3667 ]-
http://www.Meteoryty.pl marcin(at)meteoryty.pl
http://www.PolandMET.com   marcin(at)polandmet.com
http://www.Gao-Guenie.com  GSM: +48 (793) 567667
[ Member of Polish Meteoritical Society ]





Hi Jason,

Excellent link for NWA 4024 compared to 2680 (Birdsell).
From what I just can discern, I am convinced 2680 is exactly the same 
material as 4024.
See, as comparison, the pics of both meteorites added at the end of their 
respective Met. Bull reports (although NWA 2680 is still provisional, 
there are pics attached).

In particular Mirko Graul provided pics of both.
Here they are, for comparison:

NWA 2680:

http://tin.er.usgs.gov/meteor/get_original_photo.php?recno=5645813

and NWA 4024:

http://tin.er.usgs.gov/meteor/get_original_photo.php?recno=5645817

Very similar slices, almost same pattern (look at details!)

My modest suggestion:

Owing to the fact that NWA 2680 is still provisional, why not suggesting 
to this specific classification working team (Zolensky  al ?) to conclude 
(after a thorough  re-examination) that both meteorites are the same and 
thus also consider to maintain only one NWA number, thus that NWA 2680 is 
identical to NWA 4024 (that should have priority because first 
classified)?


But here the question is perhaps even more complicated because NWA 4024 is 
said to be a winonaite, while it now appears obvious that only one (or a 
few) achondritic clast(s) were analyzed in it, not the (major ?) iron 
found all around (that is IAB ungr.).
It would then be wise to fully re-analyze both materials (ideally by the 
same team) and conclude.
If there rises evidence that both are the same, then I guess there should 
come an agreement for a common type and name ?


Sorry, I am not in the Nom Com nor I know how they would proceed in such a 
case, so perhaps my suggestion is very naive.
I therefore expect more comments from Nom Com experts and am ready to 
humbly accept their conclusions whatever they be.


This is here only one typical example of something that could still be 
done, because NWA 2680 is not yet official.

There are probably other such favorable examples.
Solving them, even if progressively, will push the pairing problem one 
step forward, though it is obvious, as Jeff pointed out, that this pairing 
problem is really very difficult (I'd say impossible) to solve completely.



Zelimir

At 12:56 19/01/2010, Jason Utas wrote:

Hello John, Zelimir, All,
I've held samples of both; NWA 4024 is indistinguishable from NWA 2680.

http://www.arizonaskiesmeteorites.com/AZ_Skies_Links/NWA_2680/index.html

http://www.meteoriteguy.com/catalog/nwa4024.htm

It was likely misidentified the second time around because the sample
sent in for analysis was too small for an accurate study - or perhaps
the person who performed the analysis simply wasn't expecting an iron.
 Either way, it's funny -  an analysis based solely on the study of a
clast that comprises at most ~30-40% of the total volume of the
meteorite...I've never seen that done before.
It's a IAB with silicate inclusions - a pretty one, but an example
that's not crazily different from a few already-known irons.  Oh, and
it has winonaite-type silicate inclusions.  Just like Campo del Cielo
and many other IAB's...it's pretty typical in that respect.
We purchased a ~40g individual as a new iron in Tucson three or four
years ago; there were hundreds of small individuals of this iron
available at the time, totaling at least several kilograms (most
weighed only a few grams; Dean Bessey sold some of them on ebay later
that year, again, misidentified, and mixed with small mesosiderite
fragments).  In Tucson they were being sold as Zagora; we were
surprised to find a very fine pattern after we removed an end from
ours for analysis.
Based on what I have seen personally, I would estimate the TKW of the
find to be at least ten kilograms, but knowing NWA, there could be
(and likely is) much, much more.
Regards,
Jason

On Tue, Jan 19, 2010 at 2:58 AM, Zelimir Gabelica
zelimir.gabel...@uha.fr wrote:
 Hi John,

 NWA 4024 is indeed a nice example of the
discrepancy between Met. Bull. data
 and the amount of stuff circulating on the market.

 This is perfectly illustrated if you compare the Met. Bull. write up
 regarding NWA 4024 an look at the photos included at the end of the 
 same

 report.
 There are some 15 pieces illustrated, coming from various sources. 
 Although
 weights are not mentioned, a rough evaluation of the volume of the 
 pieces

 (comparison with the scale cubes) leads to
evaluate that the total weight of
 the illustrated pieces should largely overstep 100 g, probably more.
 Not mentioning that the pieces pictured probably represent only a small
 fraction of what is really available as 'NWA 4024 in collections.

 I have in collection a 4.43 g end section (got from Hanno 

Re: [meteorite-list] NWA 4024/2680

2010-01-19 Thread Mirko Graul
Hi Marcin and List,

oh NWA 5980 is your number of this same material?
What was the result of classification?
Winonaite or silic. iron?
I agree absolutly with Jason and Zelimir.
Also for me the material is the same.
And NWA 2680 are prefered for me.

Many greetings to all,

Mirko (sorry for my bad english)


Mirko Graul Meteorite 
Quittenring.4 
16321 Bernau 
GERMANY 

Phone: 0049-1724105015 
E-Mail: m_gr...@yahoo.de 
WEB: www.meteorite-mirko.de 

Member of The Meteoritical Society 
(International Society for Meteoritics and Planetery Science) 

IMCA-Member: 2113 
(International Meteorite Collectors Association)


--- Marcin Cimala mar...@meteoryt.net schrieb am Di, 19.1.2010:

 Von: Marcin Cimala mar...@meteoryt.net
 Betreff: Re: [meteorite-list] NWA 4024/2680
 An: Meteorite-list meteorite-list@meteoritecentral.com
 Datum: Dienstag, 19. Januar 2010, 16:01
 Hi
 You can add to this also my number NWA 5980. Its paired to
 4024
 TKW 298g
 
 -[ MARCIN CIMALA ]-[ I.M.C.A.#3667 ]-
 http://www.Meteoryty.pl       
      marcin(at)meteoryty.pl
 http://www.PolandMET.com   
    marcin(at)polandmet.com
 http://www.Gao-Guenie.com      GSM: +48
 (793) 567667
 [ Member of Polish Meteoritical Society ]
 
 
 
 
  Hi Jason,
  
  Excellent link for NWA 4024 compared to 2680
 (Birdsell).
  From what I just can discern, I am convinced 2680 is
 exactly the same material as 4024.
  See, as comparison, the pics of both meteorites added
 at the end of their respective Met. Bull reports (although
 NWA 2680 is still provisional, there are pics attached).
  In particular Mirko Graul provided pics of both.
  Here they are, for comparison:
  
  NWA 2680:
  
  http://tin.er.usgs.gov/meteor/get_original_photo.php?recno=5645813
  
  and NWA 4024:
  
  http://tin.er.usgs.gov/meteor/get_original_photo.php?recno=5645817
  
  Very similar slices, almost same pattern (look at
 details!)
  
  My modest suggestion:
  
  Owing to the fact that NWA 2680 is still provisional,
 why not suggesting to this specific classification working
 team (Zolensky  al ?) to conclude (after a
 thorough  re-examination) that both meteorites are the
 same and thus also consider to maintain only one NWA number,
 thus that NWA 2680 is identical to NWA 4024 (that should
 have priority because first classified)?
  
  But here the question is perhaps even more complicated
 because NWA 4024 is said to be a winonaite, while it now
 appears obvious that only one (or a few) achondritic
 clast(s) were analyzed in it, not the (major ?) iron found
 all around (that is IAB ungr.).
  It would then be wise to fully re-analyze both
 materials (ideally by the same team) and conclude.
  If there rises evidence that both are the same, then I
 guess there should come an agreement for a common type and
 name ?
  
  Sorry, I am not in the Nom Com nor I know how they
 would proceed in such a case, so perhaps my suggestion is
 very naive.
  I therefore expect more comments from Nom Com experts
 and am ready to humbly accept their conclusions whatever
 they be.
  
  This is here only one typical example of something
 that could still be done, because NWA 2680 is not yet
 official.
  There are probably other such favorable examples.
  Solving them, even if progressively, will push the
 pairing problem one step forward, though it is obvious, as
 Jeff pointed out, that this pairing problem is really very
 difficult (I'd say impossible) to solve completely.
  
  
  Zelimir
  
  At 12:56 19/01/2010, Jason Utas wrote:
  Hello John, Zelimir, All,
  I've held samples of both; NWA 4024 is
 indistinguishable from NWA 2680.
  
  http://www.arizonaskiesmeteorites.com/AZ_Skies_Links/NWA_2680/index.html
  
  http://www.meteoriteguy.com/catalog/nwa4024.htm
  
  It was likely misidentified the second time around
 because the sample
  sent in for analysis was too small for an accurate
 study - or perhaps
  the person who performed the analysis simply
 wasn't expecting an iron.
   Either way, it's funny -  an analysis
 based solely on the study of a
  clast that comprises at most ~30-40% of the total
 volume of the
  meteorite...I've never seen that done before.
  It's a IAB with silicate inclusions - a pretty
 one, but an example
  that's not crazily different from a few
 already-known irons.  Oh, and
  it has winonaite-type silicate inclusions. 
 Just like Campo del Cielo
  and many other IAB's...it's pretty typical in that
 respect.
  We purchased a ~40g individual as a new iron in
 Tucson three or four
  years ago; there were hundreds of small
 individuals of this iron
  available at the time, totaling at least several
 kilograms (most
  weighed only a few grams; Dean Bessey sold some of
 them on ebay later
  that year, again, misidentified, and mixed with
 small mesosiderite
  fragments).  In Tucson they were being sold
 as Zagora; we were
  surprised to find a very fine pattern after we
 removed an end from
  ours for analysis.
  Based on what I have seen personally, I 

Re: [meteorite-list] Pairing discussion/questions

2010-01-19 Thread Ted Bunch
Jeff - your statement from below  Also, don't overlook the fact that
Antarctic meteorite have proven to be vastly more valuable scientifically
than NWA meteorites is misleading and somewhat biased. Meteorites of the
various classes are nearly equally represented in the Antarctic and Desert
collections. Some classes are better represented from the desert
collections, for examples, brachinites, angrites, Martians and the Antarctic
collections have more acapulcoites, aubrites, and some carbonaceous. But,
the number of samples doesn't really matter.

The number of scientific publications  10X means little in terms of
scientific significance. The use of Antarctic specimens is largely biased if
you consider the following:

1) NSF funded Antarctic samples are more easily obtained for research
compared with trying to obtain samples from collectors, dealers and
repository collections and they are usually prepared for instant study (thin
sections, cleaned, diced, boxed, etc.).
2) NSF has put pressure on various institutions to either publish more on
the 1000s of Antarctic meteorites, obtained with NSF funding, or lose
support for future Expeditions.
3) There is considerable bias among some researchers to not use Desert
samples for political reasons and the lack of exact find locations (Nomads
do not use GPS instruments, not that this means much). Some museums are
extremely biased against dirty desert meteorites and will not let them in
the door, thus depriving researchers for easy access to samples for study -
a very prominent Federally funded museum comes to mind.
4) The Japanese publish almost exclusively on their Antarctic meteorites,
not Desert specimens.
5) More and more  research papers deal with both Desert and Antarctic
samples and that tact is becoming more prevalent with time as bias
diminishes and the reality of desert significance enters the mind set. I
don't know how you factor that into the numbers game.
6) A shot at more valuable scientifically - if not for the valuable lunar
samples collected from the deserts, we would know much less about the Moon -
see the Korotev web site on Lunars. And, and we know a Hell of a lot more
about Mars from Desert Martians - See Irving web site on Martians.

Bottom line -  geography has little to do with a meteorite's significance.
As a colleague of mine said A meteorite doesn't care where it lands.

Regards, Ted



On 1/19/10 5:46 AM, Jeff Grossman jgross...@usgs.gov wrote:

 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


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Re: [meteorite-list] Pairing discussion/questions

2010-01-19 Thread Jeff Grossman
I can now report with some authority that the total cost of 30+ years 
of collecting by ANSMET has been in the range of $20 
million.  Considering the record of scientific achievements that has 
been built on this collection of 20,000 specimens, I would have to 
say it has been a bargain.


Jeff

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 Geological Survey  fax:   (703) 648-6383
954 National Center
Reston, VA 20192, USA


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Re: [meteorite-list] NWA 4024/2680

2010-01-19 Thread Marcin Cimala

Hi Marcin and List,

oh NWA 5980 is your number of this same material?
What was the result of classification?


I was not sure what it is. I hoped its something similar to Udei Station but 
then I have seen same material in Ensisheim (it was propably NWA4024). I was 
surprized that its winonaite. But lab results confirmed this.


-[ MARCIN CIMALA ]-[ I.M.C.A.#3667 ]-
http://www.Meteoryty.pl marcin(at)meteoryty.pl
http://www.PolandMET.com   marcin(at)polandmet.com
http://www.Gao-Guenie.com  GSM: +48 (793) 567667
[ Member of Polish Meteoritical Society ]



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Re: [meteorite-list] Pairing discussion/questions

2010-01-19 Thread Adam Hupe
Thank you, Ted for pointing out that a meteorite doesn't care where it lands. I 
noticed that this bias concerning Antarctic versus NWA finds is disappearing 
with the current generation of scientists.  Years ago at the LPSC in Houston, 
about one and ten papers concerning planetary meteorites mentioned NWA. The 
last time I went to this conference, over half the papers that dealt with 
planetary meteorites included NWA specimens. When talking to the up and coming 
planetary scientists, I observed that they were equally enthusiastic about 
specimens and have not developed any bias whatsoever.

I have seen both Antarctic and NWA specimens and I am equally impressed with 
both. I saw a freezer and a nitrogen filled case full of Antarctic specimens at 
the Antarctic Laboratory when I visited it a couple of years ago.  I failed to 
see a difference other than the the Antarctic pieces were treated much better 
in the handling and preservation department. I observed heavy weathering on 
most of the pieces but they were preserved in the same manner as the few fresh 
pieces I saw.  They just weathered differently then the NWA material with a lot 
of evaporates and salt clinging to them. NWA material, on the other hand, 
develops caliche deposits and really weathered examples tend to crack or 
fragment.  In my opinion, both locations are equally capable of producing fresh 
and desirable specimens.


Best Regards,

Adam

  



- Original Message 
From: Ted Bunch tbe...@cableone.net
To: Jeff Grossman jgross...@usgs.gov; Meteorite-list 
meteorite-list@meteoritecentral.com
Sent: Tue, January 19, 2010 7:54:23 AM
Subject: Re: [meteorite-list] Pairing discussion/questions

Jeff - your statement from below  Also, don't overlook the fact that
Antarctic meteorite have proven to be vastly more valuable scientifically
than NWA meteorites is misleading and somewhat biased. Meteorites of the
various classes are nearly equally represented in the Antarctic and Desert
collections. Some classes are better represented from the desert
collections, for examples, brachinites, angrites, Martians and the Antarctic
collections have more acapulcoites, aubrites, and some carbonaceous. But,
the number of samples doesn't really matter.

The number of scientific publications  10X means little in terms of
scientific significance. The use of Antarctic specimens is largely biased if
you consider the following:

1) NSF funded Antarctic samples are more easily obtained for research
compared with trying to obtain samples from collectors, dealers and
repository collections and they are usually prepared for instant study (thin
sections, cleaned, diced, boxed, etc.).
2) NSF has put pressure on various institutions to either publish more on
the 1000s of Antarctic meteorites, obtained with NSF funding, or lose
support for future Expeditions.
3) There is considerable bias among some researchers to not use Desert
samples for political reasons and the lack of exact find locations (Nomads
do not use GPS instruments, not that this means much). Some museums are
extremely biased against dirty desert meteorites and will not let them in
the door, thus depriving researchers for easy access to samples for study -
a very prominent Federally funded museum comes to mind.
4) The Japanese publish almost exclusively on their Antarctic meteorites,
not Desert specimens.
5) More and more  research papers deal with both Desert and Antarctic
samples and that tact is becoming more prevalent with time as bias
diminishes and the reality of desert significance enters the mind set. I
don't know how you factor that into the numbers game.
6) A shot at more valuable scientifically - if not for the valuable lunar
samples collected from the deserts, we would know much less about the Moon -
see the Korotev web site on Lunars. And, and we know a Hell of a lot more
about Mars from Desert Martians - See Irving web site on Martians.

Bottom line -  geography has little to do with a meteorite's significance.
As a colleague of mine said A meteorite doesn't care where it lands.

Regards, Ted



On 1/19/10 5:46 AM, Jeff Grossman jgross...@usgs.gov wrote:

 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 

Re: [meteorite-list] Impact on Value Being Unclassified

2010-01-19 Thread Greg Catterton
So many sell material that is self paired its not funny.
It comes down to WHO is selling it in my opinion as to how much fuss is raised.
How many of the NWA martians are out there with solid documentation as to 
actual scientific pairing? about 20% maybe, if that much?
In my opinion an NWA  martian is just as valuable as NWA pick your number. 
I have never purchased a meteorite with actual testing information, so by the 
opinion of some, its not official as not documentation came with it.

I think more dealers need to get the people testing to provide them with actual 
paperwork to go with the material. For putting out 20% they should provide 
more. Even if its only from type sample testing, more documentation is better 
then an ID card on BC paper. 

Greg C.

--- On Tue, 1/19/10, Greg Stanley stanleygr...@hotmail.com wrote:

 From: Greg Stanley stanleygr...@hotmail.com
 Subject: [meteorite-list] Impact on Value Being Unclassified
 To: meteorite-list@meteoritecentral.com
 Date: Tuesday, January 19, 2010, 12:06 PM
 
 List:
 
 This brings up a question: If a meteorite in unclassified,
 how does it affect the value? I would think considerably, as
 most collectors desire documentation for their pieces, as
 any collector does.  However, others may not care if they
 can get (a martian or lunar) for less money; but with higher
 risk.  I would think that most dealers would want to get
 everything classified, as they could get more money.  I can
 certainly understand that the nomads want to keep their
 locations secret, but the dealer should still get the finds
 classified, and find out if certain pieces were found
 together.  I think over time, the unclassified stones will
 lose value, while the classified stones will increase in
 value.  I think it's a shame that so many stones get
 unclassified, it's like have old paintings or works of are
 unsigned.
 
 Just my Thoughts,
 
 Greg S.
     
 
       
   
 _
 Hotmail: Trusted email with Microsoft’s powerful SPAM
 protection.
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[meteorite-list] Testing Documentation - NWA 5799 Documentation

2010-01-19 Thread Greg Catterton
This is what I am able to get from the person that does my testing - 
It is the Documentation for NWA 5799 - A very nice, but ordinary LL4
http://i27.photobucket.com/albums/c165/jedisdiamond/NWA5799p1.jpg
http://i27.photobucket.com/albums/c165/jedisdiamond/NWA5799p2.jpg
http://i27.photobucket.com/albums/c165/jedisdiamond/NWA5799p3.jpg
http://i27.photobucket.com/albums/c165/jedisdiamond/NWA5799p4.jpg

While I know this is not the norm, I ask why not? Why can I get this, but none 
of the people with all these well known contacts cant? How hard would it be to 
provide some testing information to the person submitting the material? Why is 
this not mandatory? 

What is the cost of a few sheets of paper and a couple minutes to print it out?
In my opinion, if it does not come with documentation like this, it is not as 
valuable as it could be. 
Sure it may not be spot on exact as to the sample sold, but its far better then 
any ID card.
I know I have brought this up before, but from some comments about pairing and 
testing, this again seems a good time to bring it up again...

To all dealers/Testers out there, why not offer more? Cost is nothing compared 
to added value the paperwork adds. Make copies and include it with the 
material... add the extra 30 cent it may cost to do if your profit margins are 
not good...

In my opinion, this is real documentation, something I have never got from 
anyone I have ever bought from. 

The bottom line is, If I can get this, for an LL Chondrite, Why cant you guys 
get it? Why is this not the normal thing to do? 
Is it not better?

Greg C.




--- On Tue, 1/19/10, Greg Catterton star_wars_collec...@yahoo.com wrote:

 From: Greg Catterton star_wars_collec...@yahoo.com
 Subject: Re: [meteorite-list] Impact on Value Being Unclassified
 To: Greg Stanley stanleygr...@hotmail.com
 Cc: meteorite-list@meteoritecentral.com
 Date: Tuesday, January 19, 2010, 12:14 PM
 So many sell material that is self
 paired its not funny.
 It comes down to WHO is selling it in my opinion as to how
 much fuss is raised.
 How many of the NWA martians are out there with solid
 documentation as to actual scientific pairing? about 20%
 maybe, if that much?
 In my opinion an NWA  martian is just as valuable as
 NWA pick your number. 
 I have never purchased a meteorite with actual testing
 information, so by the opinion of some, its not official as
 not documentation came with it.
 
 I think more dealers need to get the people testing to
 provide them with actual paperwork to go with the material.
 For putting out 20% they should provide more. Even if its
 only from type sample testing, more documentation is better
 then an ID card on BC paper. 
 
 Greg C.
 
 --- On Tue, 1/19/10, Greg Stanley stanleygr...@hotmail.com
 wrote:
 
  From: Greg Stanley stanleygr...@hotmail.com
  Subject: [meteorite-list] Impact on Value Being
 Unclassified
  To: meteorite-list@meteoritecentral.com
  Date: Tuesday, January 19, 2010, 12:06 PM
  
  List:
  
  This brings up a question: If a meteorite in
 unclassified,
  how does it affect the value? I would think
 considerably, as
  most collectors desire documentation for their pieces,
 as
  any collector does.  However, others may not care if
 they
  can get (a martian or lunar) for less money; but with
 higher
  risk.  I would think that most dealers would want to
 get
  everything classified, as they could get more money. 
 I can
  certainly understand that the nomads want to keep
 their
  locations secret, but the dealer should still get the
 finds
  classified, and find out if certain pieces were found
  together.  I think over time, the unclassified stones
 will
  lose value, while the classified stones will increase
 in
  value.  I think it's a shame that so many stones get
  unclassified, it's like have old paintings or works of
 are
  unsigned.
  
  Just my Thoughts,
  
  Greg S.
      
  
        
    
 
 _
  Hotmail: Trusted email with Microsoft’s powerful
 SPAM
  protection.
  http://clk.atdmt.com/GBL/go/196390706/direct/01/
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Re: [meteorite-list] Pairing discussion/questions

2010-01-19 Thread Jeff Grossman
This is not about enthusiasm or generations of scientists.  This is 
about specimen availability and curation.  With extremely rare classes, 
like lunar meteorites, scientists do try to obtain every specimen they 
possibly can, and there has been a lot of work done on NWA meteorites.  
However, with virtually all other types of meteorites, this is not the 
case.  For these, Antarctic meteorites receive much more attention 
because the samples are well-curated and easily available.


As far as your and Ted's assertion that there is bias...  You imply 
that workers are choosing one specimen over another simply because of 
where it comes from.  I don't know of any scientist who would do that.  
People tend to work on the material to which they have access, and avoid 
making extra effort to purchase or search for other material unless that 
have to.  The simple fact is that access to NWA samples is relatively 
poor.  Many museums don't have large collections of NWAs (e.g., in the 
United States, the SI, AMNH, FMNH), the reasons for which are irrelevant 
to this discussion.  Types specimens tend to be small even in 
institutions that have them.  I am not alone, I am sure, in reporting 
that I have had serious difficulty getting research material for many 
hot-desert meteorites (including those from Oman and NWA), but nearly 
all my requests for Antarctic meteorites have been fulfilled.  These are 
the reasons that NWAs are relatively understudied and, I would argue, 
less valuable to science in general.


jeff



On 2010-01-19 12:00 PM, Adam Hupe wrote:

Thank you, Ted for pointing out that a meteorite doesn't care where it lands. I 
noticed that this bias concerning Antarctic versus NWA finds is disappearing 
with the current generation of scientists.  Years ago at the LPSC in Houston, 
about one and ten papers concerning planetary meteorites mentioned NWA. The 
last time I went to this conference, over half the papers that dealt with 
planetary meteorites included NWA specimens. When talking to the up and coming 
planetary scientists, I observed that they were equally enthusiastic about 
specimens and have not developed any bias whatsoever.

I have seen both Antarctic and NWA specimens and I am equally impressed with 
both. I saw a freezer and a nitrogen filled case full of Antarctic specimens at 
the Antarctic Laboratory when I visited it a couple of years ago.  I failed to 
see a difference other than the the Antarctic pieces were treated much better 
in the handling and preservation department. I observed heavy weathering on 
most of the pieces but they were preserved in the same manner as the few fresh 
pieces I saw.  They just weathered differently then the NWA material with a lot 
of evaporates and salt clinging to them. NWA material, on the other hand, 
develops caliche deposits and really weathered examples tend to crack or 
fragment.  In my opinion, both locations are equally capable of producing fresh 
and desirable specimens.


Best Regards,

Adam





- Original Message 
From: Ted Bunchtbe...@cableone.net
To: Jeff Grossmanjgross...@usgs.gov; 
Meteorite-listmeteorite-list@meteoritecentral.com
Sent: Tue, January 19, 2010 7:54:23 AM
Subject: Re: [meteorite-list] Pairing discussion/questions

Jeff - your statement from below  Also, don't overlook the fact that
Antarctic meteorite have proven to be vastly more valuable scientifically
than NWA meteorites is misleading and somewhat biased. Meteorites of the
various classes are nearly equally represented in the Antarctic and Desert
collections. Some classes are better represented from the desert
collections, for examples, brachinites, angrites, Martians and the Antarctic
collections have more acapulcoites, aubrites, and some carbonaceous. But,
the number of samples doesn't really matter.

The number of scientific publications   10X means little in terms of
scientific significance. The use of Antarctic specimens is largely biased if
you consider the following:

1) NSF funded Antarctic samples are more easily obtained for research
compared with trying to obtain samples from collectors, dealers and
repository collections and they are usually prepared for instant study (thin
sections, cleaned, diced, boxed, etc.).
2) NSF has put pressure on various institutions to either publish more on
the 1000s of Antarctic meteorites, obtained with NSF funding, or lose
support for future Expeditions.
3) There is considerable bias among some researchers to not use Desert
samples for political reasons and the lack of exact find locations (Nomads
do not use GPS instruments, not that this means much). Some museums are
extremely biased against dirty desert meteorites and will not let them in
the door, thus depriving researchers for easy access to samples for study -
a very prominent Federally funded museum comes to mind.
4) The Japanese publish almost exclusively on their Antarctic meteorites,
not Desert specimens.
5) More and more  research papers deal with both 

[meteorite-list] Possible LL5 polymict Breccia for study/educational/testing use

2010-01-19 Thread Greg Catterton
Hi to all, I am doing more cutting on a 1086g complete stone.
This is possibly an LL5 polymict breccia.
I will have some small part slices and cutting debris that may be good for 
testing, study, or simply a type sample.
It is from NWA.

I would like to offer the first 10 people to reply some of this - no 
collectors, I would like this to go to places that can use them for study, 
research and educational use. If more then 10 want some, I may make more 
available, email me.

I will offer part slices that would make good thin sections.

Classification is being done on this by Ted Bunch, he is busy and had some 
equipment issues, so it may take time to get a number. No classification is 
needed however.


Greg C.


  
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Re: [meteorite-list] Pairing discussion/questions

2010-01-19 Thread Adam Hupe
Hi Jeff and List,

I agree with most of what you stated in your last post although I believe there 
is a real bias among a very few scientists, and certainly a few museums.

Access to planetary material , Angrites and other rare material from NWA is 
supposed to be a simple matter of contacting the repository. There has been 
many times, my brother and I have provided additional material beyond type 
specimen  requirements in order to satisfy science.  My brother has gone as far 
as allowing having a sizable core taken from a large Angrite individual at a 
great lose in commercial value.  I donated more than twice the requirement for 
NWA 5000 and have given scientists access to the main mass.  We do this because 
we recognize that science is the most important aspect in qualifying 
meteorites. Without it, they are fairly worthless.  There are other collectors 
and dealers who have done the same when asked.  For the most part, collectors 
and dealers would love to have their hot desert finds studied.  Then there are 
a few who are stingy in regards to parting with samples.

I totally disagree with the following statement:

These are the reasons that NWAs are relatively understudied and, I would argue, 
less valuable to science in general.

I believe the hot desert finds are every bit as important to science as the the 
Antarctic finds.  Acceptance and access of hot desert finds has improved 
dramatically the last ten years.  There are several surprises yet to come, from 
both Antarctic and NWA. To value one over the other is demonstrating a bias in 
my opinion.

Best Regards,

Adam
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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



-Ursprüngliche Nachricht-
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 

[meteorite-list] TC3 2008 : 2 french and 1 belgian meteorite hunters imprisoned in Sudan

2010-01-19 Thread Pelé Pierre-Marie
Hello,  

I just read an article about two french and one belgian tourists who were 
arrested two weeks ago in Sudan because of having in their possession samples 
of the TC3 2008 meteorite.

You can read the article here :
http://translate.google.fr/translate?u=http%3A%2F%2Fwww.google.com%2Fhostednews%2Fafp%2Farticle%2FALeqM5h2LgyLBZP-1Nlc6tbDS4FhkwI_8wsl=frtl=enhl=ie=UTF-8

I don't know who they are ?

Pierre-Marie Pele
www.meteor-center.com


  

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[meteorite-list] Meteorite Pairing Discussions-Still Looking for Answers

2010-01-19 Thread Thomas Webb


--- On Mon, 1/18/10, Thomas Webb webb...@yahoo.com wrote:

 From: Thomas Webb webb...@yahoo.com
 Subject: [meteorite-list] Meteorite Pairing Discussions
 To: meteorite-list@meteoritecentral.com, Martin Altmann 
 altm...@meteorite-martin.de
 Date: Monday, January 18, 2010, 9:04 PM
 List,
 Martin wrote--
 - Even if you're absolutely sure, that one of your stones
 is paired to one
 or several existing NWA-numbers, you are not allowed in no
 case to use one
 of these numbers.
 
 I think I understand the reasoning behind what has been put
 forth in this discussion so far and abide with it in my own
 dealings, however, I must wonder why practically everyone on
 the list who deals in meteorites has not had their probably
 paired with NWA 869 stones classified with a new number
 rather than just listing them as NWA 869 even though they
 bought them as unclassified and probably paired
 with.  Is there some hypocrisy here?  Is it OK to
 make an eyeball pairing with 869 but not other NWA's? 
 Does no one care on this one simply because there is so much
 of it, so the rule does not apply?  Could it be that no
 one cares about getting a new number and classification if
 it's a meteorite that sells for pennies per gram, but if it
 sells for many dollars or hundreds of dollars per gram, then
 it becomes important?  Is it OK to bend or break the
 rules in some cases but not others?  Does greed ever
 enter into the equation?
 
 I've asked a lot of questions.  I'm certain there's
 someone here who can give reasonable answers.
 
 My best,
 Thomas
 
 
       
 
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Re: [meteorite-list] Pairing discussion/questions

2010-01-19 Thread Martin Altmann
Jason,

first of all, I do not justify anybody's action,
second, I can't discuss based upon hear-say and rumours, for that the time
of all of us, is too pity.
If you deal accusations, you have to deliver facts (the list rules require
that too).

But you're merely downplaying the importance of information such as
where they were found, etc, without even justifying it.

You have excessive strewnfield mapping for Libya, partially for Oman too.

The question of terrestrial weathering is one of the main occupation of the
Suisse-Omani team.
As you see, it can be done, totally independent from that what any private
dealer, hunter or collector is doing.
That it isn't done, you can't accuse the hunters of, as long as there is
worldwide only a single public financed expedition team doing that job
periodically in the desert (once per year, a very few people, for a very few
weeks).
Meteorite science is, like most forms of basic research, see astronomy, see
physics, see spaceflight -  a public task.

But Oman's hardly giong to send police over to reclaim rocks

Here the principle is decisive.
A crime will stay a crime, when law tells it is a crime, no matter whether
it is prosecuted or not.

In the recent years, we see the fatal development, that in so many countries
those people, who tapped these countries as new and most productive
meteorite resources, those people, who found so far almost all meteorites
there on their own risks and expenses and those people, who did the field
work, the official side was not willing to do, to pay or failed with their
efforts,
those people, who found and delivered all these stones, which triggered that
enormous boost in meteoritics and planetary science of the last 20 years,
and that at a small fraction of the cost, science had spent to come to
similar results respectively a society would have to spend -

we see, that these people now are more and more criminalized or pushed in a
gray area due to the introduction of restrictive meteorite laws.

The aftermath is disastrous.
If you had checked the catalogues of the public historic collections and the
universities, you would know, that 80 or 90% of all (non-antarctic)
meteorites stem directly or indirectly from private people.

That is the reason, why we have all in all no new finds in Australia,
that the find numbers totally broke down in Libya, that we don't have
meteorites in Egypt, that NWA is going to an end and that we will have 90%
or even less finds in Oman, if the laws there would be enforced.

With the recovery of new falls - btw. touching your contamination argument,
but also to seize the recommendation of the UNESCO meteorite working group,
where it was consensus already in the 1960ies, that it is of crucial
importance and that all shall be done, to recover the material as fast as
possible after it fell - there with the new falls you have the very same.
All in all not the scientists are recovering them or are going to search for
them, but the private people.

The current situation caused by those many new laws of the last 20-30 years 
and especially in our decade is unbearable
and very harmful for the continuity of that branch of science.

the place where a meteorite falls is irrelevant.

I never suggested that.

Maybe there's 100kg more of NWA 2737 out there, but we'll never know
because that information is now lost

Right. But righter, without hunters, dealers we wouldn't know at all, that
there is a NWA 2737   ;-?

A bird in the hand is worth two in the bush, is in German,
The sparrow in the hand is better than the dove on the roof.

...but how shall I say, it is to a certain degree a luxury problem,
if you'd concede to me a more general and perhaps more antiquated
perspective.


In 1981, when I acquired my first meteorite,
there were all in all - non-antarctic:

1765 recognized meteorite finds
And
 935 recognized observed falls.

From Ur and Nogata on. 


Now only 20 years later, we have, NEW and published, additionally and
non-antarctic, we have more:

More than 
8000 new meteorite finds

And
151 observed falls


So. And the very very most of these finds and numbers were made by private
dealers, hunters, collectors. That you have to recognize (as well as those
have to register, who want to kick off the private sector).

1765 finds 3000 years before,
8000 finds in 20 years.

Among this 8000 you find a lot of very well documented ones.
You find among them more excellent documented finds, than all the meteorites
in history together were documented before.

There.

That's what I call a performance.

But you're merely downplaying the importance of information such as

Innuendo.

I say, we aren't living in a perfect world of elves and dwarves,
I say - now you know the figures - that it is incredibly ridiculous to
bemoan lacking find data of a part of these finds,
because the number, the weights, the diversity, the low costs of these finds

outweigh hundredfold the incomplete data.

Strewnfield mapping, weathering studies - 

Re: [meteorite-list] Pairing discussion/questions

2010-01-19 Thread Alexander Seidel
High-grade, profound discussion apart from certain personal disagreements. 
There surely is more to it than what just meets the eye, regarding the bottom 
line.

Keep on talking, guys. I am discovering valid arguments on both ends of the 
rope here, and can only hope that the discussion will be more refined as time 
goes on.

This is not boring or unneeded at all - this is an overdue conversation which I 
(and others) are pleased to listen to, and may be, even interfere at a point. 

For the benefit not only of a hobby (P.S.: I am just a collector, and neither a 
dealer nor a meteorite scientist), but for an overall good development of the 
field of meteoritics from a broader perspective, and in historical context and 
continuity.

Alex
Berlin/Germany
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[meteorite-list] Meteorite Pairing Discussions-Still Looking for Answers

2010-01-19 Thread Carl 's

Hi Thomas, All,

You've brought up some good points. I had asked a similar question several 
months ago but got mostly silence. Based on what was mentioned earlier, only 
the stones that were originally collected and classified can be called NWA 869. 
So like what Thomas said, all others should have the designation of Probably 
paired with NWA 869 or NWA 869 paired. I'm sure there are more pairings but NWA 
787/900 are the only ones I can find (see Jeff Kuykens' website):
http://www.meteorites.com.au/nwa869/

But also, note NWA 869 is from a known strewnfield in the Tindouf, Algeria 
area. Maybe, like the Franconia strewnfield, dealers and collectors are 
relatively sure these are what they claim it is? See also what Eric Twelker 
says in his website:
http://www.meteoritemarket.com/NWA869.htm

Any thoughts anyone? Thomas and I would like to hear more from others on this.

Carl



Thomas wrote:
 I think I understand the reasoning behind what has been put
 forth in this discussion so far and abide with it in my own
 dealings, however, I must wonder why practically everyone on
 the list who deals in meteorites has not had their probably
 paired with NWA 869 stones classified with a new number
 rather than just listing them as NWA 869 even though they
 bought them as unclassified and probably paired
 with.? Is there some hypocrisy here?? Is it OK to
 make an eyeball pairing with 869 but not other NWA's??
 Does no one care on this one simply because there is so much
 of it, so the rule does not apply?? Could it be that no
 one cares about getting a new number and classification if
 it's a meteorite that sells for pennies per gram, but if it
 sells for many dollars or hundreds of dollars per gram, then
 it becomes important?? ...
  
_
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http://clk.atdmt.com/GBL/go/196390707/direct/01/
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[meteorite-list] NatGeo Channel Ancient Asteroid

2010-01-19 Thread Richard Kowalski
For those of you who have the National Geographic Channel, I just noticed that 
their program Ancient Asteroid, which is a program about Libyan Desert Glass 
and its origins, will be re-broadcast tonight.

I see it will also be re-run again on Sunday and once more next Tuesday

Here's the show's website.

http://channel.nationalgeographic.com/episode/ancient-asteroid-2671/Overview


--
Richard Kowalski
http://fullmoonphotography.net
IMCA #1081


  
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[meteorite-list] Lucky 13 Auctions Ending - AD

2010-01-19 Thread Greg Hupe

Dear List Members,

In about 24 hours you will find 13 meteorite auctions of mine ending on 
eBay, all under seller name, NaturesVault. There will be 13 Lucky Winners 
this week of some pretty neat items! All can be found here, and as 
anticipated, many still at the 99-cent opening price: 
http://search.ebay.com/_W0QQsassZnaturesvault


A couple Highlights:
NWA 1877 Olivine Diogenite, this week's talk of the town as for Pairing 
Coat-Tailers to this Original Class!

http://cgi.ebay.com/ws/eBayISAPI.dll?ViewItemitem=350304898920ssPageName=STRK:MESELX:IT
NWA 1879 Mesosiderite 60g Slice (Almost Out!)
http://cgi.ebay.com/ws/eBayISAPI.dll?ViewItemitem=350304899780ssPageName=STRK:MESELX:IT
NWA 2828 Paleo EL3 (This is the one Al Haggounia is paired to, definitely 
NOT an Aubrite, but Cool all the same!!!)

http://cgi.ebay.com/ws/eBayISAPI.dll?ViewItemitem=350304900538ssPageName=STRK:MESELX:IT

...Angrites, Ungrouped, others...and then...

NWA 4800 CK5 End Cut (LAST ONE!)
http://cgi.ebay.com/ws/eBayISAPI.dll?ViewItemitem=170432073795ssPageName=STRK:MESELX:IT
NWA 4930 'Paired' Martian Individual
http://cgi.ebay.com/ws/eBayISAPI.dll?ViewItemitem=170432074505ssPageName=STRK:MESELX:IT
Bassikounou Individual w/ 100% Fusion Crust
http://cgi.ebay.com/ws/eBayISAPI.dll?ViewItemitem=170432076097ssPageName=STRK:MESELX:IT
Muonionalusta 315g Complete Slice (LAST SLICE I HAVE!)
http://cgi.ebay.com/ws/eBayISAPI.dll?ViewItemitem=350304907608ssPageName=STRK:MESELX:IT

I wish all of the bidders, Good Luck, and Thank You for checking out my 
auctions!


Best regards,
Greg


Greg Hupe
The Hupe Collection
NaturesVault (eBay)
gmh...@htn.net
www.LunarRock.com
IMCA 3163

Click here for my current eBay auctions: 
http://search.ebay.com/_W0QQsassZnaturesvault



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[meteorite-list] Paper on chondrule formation and synthetic chondrules

2010-01-19 Thread starsandscopes


Hi List,  I thought some of you might enjoy this portion of a science  
paper on meteorite chondrules.  It is part of a paper on microscopes posted  in 
Molecular Expressions (An online microscope site)  The first half of the  
paper is on microscopes so many of you will want to skip that part.
Tom  Phillips

PHOTOMICROGRAPHY IN THE
GEOLOGICAL SCIENCES 
Michael W.  Davidson
Institute of Molecular Biophysics
Center for Materials Research  and Technology (MARTECH)
National High Magnetic Field Laboratory  (NHMFL)
Supercomputer Computations Research Institute (SCRI)
Florida State  University, Tallahassee, Florida 32306
Telephone: 850-644-0542 Fax:  850-644-8920

Gary E. Lofgren
Planetary Materials Branch
Solar  System Exploration Division
Code SN2
NASA Johnson Space Center
Houston,  Texas 77058
Telephone: 713-483-6187 Fax: 713-483-2696

The whole  article is at 
http://micro.magnet.fsu.edu/publications/pages/journal.html  



Chondrules are small spheres (.1 to 10mm in diameter) which are  the major 
constituent of chondritic meteorites. Chondrites are considered  samples of 
primitive solar system materials. If we can understand how chondrules  form, 
we will have an important clue to the early history of our solar system.  
Most chondrules have an igneous texture which forms by crystal growth 
(usually  rapid) from a supercooled melt. Such textures are commonly described 
as  
porphyritic (large, equant crystals in a fine grained matrix), barred 
(dendrites  comprised of parallel thin blades or plates), or radiating (sprays 
of 
fine  fibers).
The models proposed for formation of chondrules can be divided into  two 
groups (McSween, 1977). In one group of models, chondrules form by melting  
and subsequent crystallization of preexisting, largely crystalline material 
from  the solar nebula. The primary differences between these models are the 
kinds of  materials which are melted and the nature of the sources of heat 
for the  melting. In the other group of models, chondrules form by 
condensation of  liquids from the solar nebula gas which then crystallize upon 
cooling. 
 Variations between these models result from differences in the 
condensation  sequence of the minerals and melts and the temperatures of 
nucleation.
One  means of testing models of chondrule formation is to determine the 
conditions  necessary to duplicate these textures by experimentally 
crystallizing chondrule  melts in the laboratory. Efforts to reproduce the 
textures of 
chondrules  experimentally have been successful only when we began to 
understand the  important role that heterogeneous nucleation plays in the 
development of igneous  rock textures. Unless heterogeneous nuclei are present 
in 
the chondrule melt,  porphyritic textures will not be produced. The dendritic 
or radiating textures  will form instead.
The treatment of heterogeneous nucleation follows the  model developed by 
Turnbull (1950) to explain many of the characteristics of  heterogeneous 
nucleation. This model was applied to heterogeneous nucleation in  basaltic 
systems by Lofgren (1983). Simply stated, the model says that in any  
steady-state melt at a given temperature there is a characteristic distribution 
 of 
embryos. The embryo is crystalline material which is smaller than the  
critical size necessary to be a stable nucleus and cause nucleation. It is a  
subcritical-sized potential heterogeneous nucleus. Embryos exist whether 
stable,  
supercritically-sized nuclei are present or not. If a melt is sufficiently  
superheated, embryos can be eliminated. Nucleation would then require a 
surface,  presumably the container and the barrier to nucleation would be much 
higher than  in the case where embryos were present. Qualitatively, such 
nucleation would  resemble homogeneous nucleation; but, if a surface is 
available, the energy  barrier would be much lower than for homogeneous 
nucleation. 
Glasses would form  from chondrule melts most readily if they are 
superheated, thus destroying the  embryos and increasing the barrier to 
nucleation. 
Lower melting temperatures  would allow embryos to be retained. These can 
then grow upon cooling and become  nuclei. Embryos also can become nuclei 
without changing size, because the size  at which an embryo becomes a nucleus 
depends upon the degree of supercooling in  the melt. Thus, an increase in the 
degree of supercooling can cause an embryo to  become a nucleus and 
nucleation to occur.
If relict crystals are present in  the melt at the initiation of cooling, 
the more equilibrium-like crystals  typical of porphyritic textures are 
formed. When such experiments are quenched,  the final product contains glass 
or 
fine grained material, often dendritic,  enclosing the equilibrium 
phenocrysts. An example of this texture produced in  experiments is shown in 
Figure 
7. Equant, well formed crystals of olivine are  set in a glassy matrix with a 
few dendrites present. In the natural prophyritic  

Re: [meteorite-list] Paper on chondrule formation and synthetic chondrules

2010-01-19 Thread Dave Myers
Thanks,

That info. is great! I love the CV3 and the LL3-6, That show hundreds of 
chondrules,  I even like them better than stoney-irons! There 2nd!
Only wish I could aford them! ..LOL  

Thanks for the info.

Dave Myers



--- On Tue, 1/19/10, starsandsco...@aol.com starsandsco...@aol.com wrote:

 From: starsandsco...@aol.com starsandsco...@aol.com
 Subject: [meteorite-list] Paper on chondrule formation and synthetic 
 chondrules
 To: meteorite-list@meteoritecentral.com
 Date: Tuesday, January 19, 2010, 11:54 PM
 
 
 Hi List,  I thought some of you might enjoy this
 portion of a science  
 paper on meteorite chondrules.  It is part of a paper
 on microscopes posted  in 
 Molecular Expressions (An online microscope site)  The
 first half of the  
 paper is on microscopes so many of you will want to skip
 that part.
 Tom  Phillips
 
 PHOTOMICROGRAPHY IN THE
 GEOLOGICAL SCIENCES 
 Michael W.  Davidson
 Institute of Molecular Biophysics
 Center for Materials Research  and Technology
 (MARTECH)
 National High Magnetic Field Laboratory  (NHMFL)
 Supercomputer Computations Research Institute (SCRI)
 Florida State  University, Tallahassee, Florida 32306
 Telephone: 850-644-0542 Fax:  850-644-8920
 
 Gary E. Lofgren
 Planetary Materials Branch
 Solar  System Exploration Division
 Code SN2
 NASA Johnson Space Center
 Houston,  Texas 77058
 Telephone: 713-483-6187 Fax: 713-483-2696
 
 The whole  article is at 
 http://micro.magnet.fsu.edu/publications/pages/journal.html 
 
 
 
 
 Chondrules are small spheres (.1 to 10mm in diameter) which
 are  the major 
 constituent of chondritic meteorites. Chondrites are
 considered  samples of 
 primitive solar system materials. If we can understand how
 chondrules  form, 
 we will have an important clue to the early history of our
 solar system.  
 Most chondrules have an igneous texture which forms by
 crystal growth 
 (usually  rapid) from a supercooled melt. Such
 textures are commonly described as  
 porphyritic (large, equant crystals in a fine grained
 matrix), barred 
 (dendrites  comprised of parallel thin blades or
 plates), or radiating (sprays of 
 fine  fibers).
 The models proposed for formation of chondrules can be
 divided into  two 
 groups (McSween, 1977). In one group of models, chondrules
 form by melting  
 and subsequent crystallization of preexisting, largely
 crystalline material 
 from  the solar nebula. The primary differences
 between these models are the 
 kinds of  materials which are melted and the nature of
 the sources of heat 
 for the  melting. In the other group of models,
 chondrules form by 
 condensation of  liquids from the solar nebula gas
 which then crystallize upon cooling. 
  Variations between these models result from differences in
 the 
 condensation  sequence of the minerals and melts and
 the temperatures of nucleation.
 One  means of testing models of chondrule formation is
 to determine the 
 conditions  necessary to duplicate these textures by
 experimentally 
 crystallizing chondrule  melts in the laboratory.
 Efforts to reproduce the textures of 
 chondrules  experimentally have been successful only
 when we began to 
 understand the  important role that heterogeneous
 nucleation plays in the 
 development of igneous  rock textures. Unless
 heterogeneous nuclei are present in 
 the chondrule melt,  porphyritic textures will not be
 produced. The dendritic 
 or radiating textures  will form instead.
 The treatment of heterogeneous nucleation follows the 
 model developed by 
 Turnbull (1950) to explain many of the characteristics
 of  heterogeneous 
 nucleation. This model was applied to heterogeneous
 nucleation in  basaltic 
 systems by Lofgren (1983). Simply stated, the model says
 that in any  
 steady-state melt at a given temperature there is a
 characteristic distribution  of 
 embryos. The embryo is crystalline material which is
 smaller than the  
 critical size necessary to be a stable nucleus and cause
 nucleation. It is a  
 subcritical-sized potential heterogeneous nucleus. Embryos
 exist whether stable,  
 supercritically-sized nuclei are present or not. If a melt
 is sufficiently  
 superheated, embryos can be eliminated. Nucleation would
 then require a 
 surface,  presumably the container and the barrier to
 nucleation would be much 
 higher than  in the case where embryos were present.
 Qualitatively, such 
 nucleation would  resemble homogeneous nucleation;
 but, if a surface is 
 available, the energy  barrier would be much lower
 than for homogeneous nucleation. 
 Glasses would form  from chondrule melts most readily
 if they are 
 superheated, thus destroying the  embryos and
 increasing the barrier to nucleation. 
 Lower melting temperatures  would allow embryos to be
 retained. These can 
 then grow upon cooling and become  nuclei. Embryos
 also can become nuclei 
 without changing size, because the size  at which an
 embryo becomes a nucleus 
 depends upon the degree of supercooling in  the melt.
 

[meteorite-list] (ad) half off on everytning

2010-01-19 Thread steve arnold
Hi list.I really want to move these pieces so they are all half off from the 
price I gave them.The 60 gram unclassed L3 type is sold.So off list and free 
shipping.
 Steve R. Arnold, Chicago!! chicagometeorites.net/ 
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[meteorite-list] Space rocks land tourists in Sudanese jail

2010-01-19 Thread Tom Randall (KB2SMS)


http://www.abc.net.au/news/stories/2010/01/20/2796743.htm



http://home.roadrunner.com/~kb2sms/

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[meteorite-list] Setting

2010-01-19 Thread Pete Shugar

I can't get this figured out to save my hinnie.
How do you get the list to show your own posts
to the list. 
When I first got on the list about 3 years ago,

I saw my own posts, now nothing.
Many is the time I post to the list, only to
have my post ignored. At least if I can see my posts
then I know they were just ignored instead of never 
making it to the list.


I reiterate, Since Tahoka has never been classified,
would I be out of line to acquire a sample and send it in
to be classified?
Pete

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[meteorite-list] Weird Iron Sulfide Barred Chondrule Looking Feature

2010-01-19 Thread starsandscopes


Hi List,  I just ran onto an Iron Sulfide  inclusion in an unclassified 
impact melt.  It is structured like a barred  chondrule.  I have never seen any 
like it before.

Has any one else  seen this feature?

I have some micrographs if any one wants to look just  email me.  I will 
post images to my Gallery but that will likely take some  time and I am 
interested in your observations while I am still working on  it.

Tom Phillips  

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Re: [meteorite-list] Setting

2010-01-19 Thread Richard Kowalski
Login here:

http://six.pairlist.net/mailman/listinfo/meteorite-list

using the unsubscribe or edit options button at the bottom of the page

Then click on the Yes radio button for the Receive your own posts to the 
list? option.

and then the Submit my options: button at the bottom of the page.


--
Richard Kowalski
http://fullmoonphotography.net
IMCA #1081


--- On Tue, 1/19/10, Pete Shugar pshu...@clearwire.net wrote:

 From: Pete Shugar pshu...@clearwire.net
 Subject: [meteorite-list] Setting
 To: meteorite-list@meteoritecentral.com
 Date: Tuesday, January 19, 2010, 8:18 PM
 I can't get this figured out to save
 my hinnie.
 How do you get the list to show your own posts
 to the list. When I first got on the list about 3 years
 ago,
 I saw my own posts, now nothing.
 Many is the time I post to the list, only to
 have my post ignored. At least if I can see my posts
 then I know they were just ignored instead of never making
 it to the list.
 
 I reiterate, Since Tahoka has never been classified,
 would I be out of line to acquire a sample and send it in
 to be classified?
 Pete
 
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[meteorite-list] PA Fireball Jul09 - Search Update

2010-01-19 Thread Mike Hankey
Hello List,

I just posted a pretty big update on the PA Fireball search (yes I'm
still searching).

http://www.mikesastrophotos.com/baltimore-pa-meteor/mason-dixon-update-new-rob-matson-trajectory/

Most of the post is about some AMAZING and very interesting work Rob
Matson did with the fireball data back in November.

The highlights are:
 - improved 3d trajectory based on analysis of high quality videos
 - 12 radar returns detected and back plotted
 - new wind blown coordinates calculated with real jet stream 
surface windspeeds
 - maps of estimated strewn field, observer angles  ground track
 - how to unscientifically plot a fireball using google earth

I came into this new information in November and between the snow and
holidays I have barely scratched the surface on the search area.
Conditions are currently the best they will ever be to hunt down these
meteorites. The majority of the fields are still un-plowed, we have
really good access to these fields until early May. They will start
plowing more than 1/2 of the fields in mid March.

If anyone is still interested in hunting this down or reviewing the
trajectory info contact me and I will send you the Google KMZ and
share all my info with you.

I really want US to find this thing and I haven't given up yet.

Thanks,

Mike

PS I'll be in Tuscon between Feb 2 and Feb 7. If anyone wants to meet
up shoot me an email.
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[meteorite-list] Future meteorites! All you need do is wait a few million years.

2010-01-19 Thread Darren Garrison
http://www.skyandtelescope.com/news/82074747.html


A Strange Comet Among the Asteroids
January 7th's announcement that the LINEAR telescope had spotted a new periodic
comet wasn't all that interesting: a 20th-magnitude blip out in the asteroid
belt in a benign orbit that wouldn't come anywhere near Earth. Designated P/2010
A2 (LINEAR) by the IAU's Minor Planet Center, it was just another notch on the
finderscope for this discovery machine near Socorro, New Mexico, which has
chalked up 77 periodic comets (and a couple hundred one-timers) since coming
online in 1998.

But as other observers chipped in positions over the next week, it became clear
that this was an object worth watching. For one thing, the now-precise orbit was
looking less like a comet's and more like an asteroid's. And images of the
interloper showed a tail growing in length yet without a clearly defined head.
The online chatter got more animated — just what was this, anyway?

On January 14th, Javier Licandro and others used the Nordic Optical Telescope in
the Canary Islands to get a better view, and they discovered something
completely unexpected: a small asteroid lay 2 arcseconds to P/2010 A2's east and
was moving along with it. Moreover, the comet showed no central condensation
and looked more like a narrow dust swarm about 110,000 miles (177,000 km) long.

Licandro quickly enlisted the biggest aperture in the island's observatory
complex: the Gran Telescopio Canarias. Dozens of images taken three days ago
using its immense 34-foot (10.4-m) aperture confirm that the comet is being
shadowed. It's hard not to conclude that we are watching the aftermath of a
collision in the asteroid belt. But it's still too early to know for sure.
Licandro and his colleagues are analyzing the GTC images carefully — and they
hope to make them public soon.

Meanwhile, comet specialists are hoping to observe the strange goings-on with
both the Hubble and Spitzer space telescopes. Neither has been given the green
light yet, but if/when that happens the observations would be made within the
next few days. According to Caltech astronomer William Reach, Spitzer no longer
has the ability to look deep in the infrared, but it can still record at 3.6 and
4.5 microns, where the cometary gases carbon monoxide and carbon dioxide have
strong emissions.


http://www.astroarts.jp/news/2010/01/19linear/p2010a2.jpg
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[meteorite-list] AD: eBay auctions ending Friday, 2kg Muonio slice, 52gm Ash Creek, Glorieta Pallasite

2010-01-19 Thread Robert Ward
Hello List members, I have three items ending Friday evening, a 2 Kilo
Muonionalusta slice, a 52.9 gram Ash Creek ( West ) stone, and a 258
gram Glorieta Mountain Pallasite end piece, all are very nice
specimens out of my personal collection. Because of recent
acquisitions, and limited case room for duplicate locations in my
collection I have decided to offer these pieces. Please check out the
items on this page.  Robert Ward
http://members.ebay.com/ws/eBayISAPI.dll?ViewUserPageuserid=ironfromthesky
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[meteorite-list] Test

2010-01-19 Thread Pete Shugar

Test--Please delete
Pete

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[meteorite-list] Tucson Meteorite Auction Final Call (AD)

2010-01-19 Thread Michael Blood
Hi All,
This is the final call for entries (MUST be of high quality)
Before I create the PRINTABLE edition of the Catalog within
The next couple of days.

ALSO: Some absentee bids have come in and there is now
Only about a week left for all ABSENTEE BIDS  to be accepted -
send them in NOW, please.

Though there are only 75 items listed right now, I have always
Had a number of people enter LARGE items the day of the auction.
So, even with only 75 items, you can be sure there is going to be
A wide variety of specimens and price ranges.
Twink is bringing her specimen loaded Gold Basin Cake, food
And drink are available. Come early, have funand do I here the
Original Steve Arnold calling out, I bid a dollar! ?

Looking foreword to seeing you there, Michael



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[meteorite-list] Rocks from Space Picture of the Day - January 20, 2010

2010-01-19 Thread Michael Johnson
http://www.rocksfromspace.org/January_20_2010.html

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[meteorite-list] Who going to Tucson?

2010-01-19 Thread Arizona Keith

Hello List

Who's going to Tucson Show this year? Who can I expect to see? 
Hope to see all of you that can make it to this year show.


Keith V.
Chandler AZ
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[meteorite-list] AD- KREEP Lunar! NWA 4485

2010-01-19 Thread Dave Harris

Hi,
Long time lurker here... just a quicky ad for a 0.315g part slice of NWA 
4485 on Fleabay.


http://cgi.ebay.com/ws/eBayISAPI.dll?ViewItemitem=270518081528ssPageName=STRK:MESELX:IT


thanks for your interests!



dave harris
IMCA #0092
Sec.BIMS.
www.bimsociety.org

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[meteorite-list] OSIRIS-REx - One of Three Finalists for Next NASA Mission

2010-01-19 Thread Richard Kowalski
A short video interview with Mike Drake, LPL Director and mission PI and Dante 
Lauretta, Deputy PI about the proposed OSIRIS-Rex mission to asteroid 1999 RQ36


http://uanews.org/node/29491



--
Richard Kowalski
Catalina Sky Survey
Lunar and Planetary Laboratory
University of Arizona
Tucson, AZ  85721
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