[meteorite-list] LOVINA REVISITED

2014-02-14 Thread Darryl Pitt


Hi, 

For those who have followed the saga of Lovina:

Found in Bali, Indonesia, Lovina was classified as an ungrouped iron in early 
2008; at the end of the same year I acquired the entire mass. Lovina's hallmark 
feature are ziggurat (pyramidal) structures which measure up to two 
centimeters.  It seems these structures formed while Lovina was in solution in 
the tropical shallows from which it was recovered.  I had been offering 
specimens for sale when the Smithsonian expressed interest in acquiring the 
main mass in late 2009—and I first stopped selling specimens when Tim McCoy 
doubted Lovina's meteoricity.  Sales recommenced when new evidence from an 
esteemed colleague of Tim's resulted in the determination Lovina was indeed a 
meteorite. Months later sales were again discontinued—through this day—when 
additional news from multiple sources (Wasson, Nishiizuma) rolled in which 
contradicted the positive findings. 

Lovina bears uncanny similarities to the composition of an iron meteorite.  If 
this wasn't a meteorite, what was it? I had heard several theories, and I had 
gone to lengths to have the same verified. Some scientists felt it was slag—a 
notion dismissed by most. Others would only speak to me off-record, as they 
felt their hypothesis might be ridiculed by colleagues. One thing I've learned 
is that if there is doubt about the meteoricity of an object, it is not easy to 
find a meteoriticist to do more work on it. 

Well, early last year I was so grateful to meet Qingzhu Yin of University 
California at Davis and Yangting Lin of the Key Laboratory of the Earth's Deep 
Interior in Beijing. Yangting's affiliation in particular was of great interest 
to me given a couple of the seemingly rogue hypotheses to which I previously 
alluded. A dinner in Beijing with Qingzhu and Yangting—at which Lovina 
dominated the conversation—resulted in Qingzhu's profound interest in Lovina; 
an interest which culminated in an LPSC abstract entitled New Insights Into 
the Origin of Lovina, a Mystery Metal, which can be seen here:  
http://www.hou.usra.edu/meetings/lpsc2014/pdf/1434.pdf

Verdict: while it was determined not to be a meteorite by Qingzhu and his 
co-authors, Lovina is nonetheless an important find that is extraordinarily 
rare. The section of the mass with ziggurats has been preserved intact; it is 
certain a museum is in its future. 


All best / Darryl



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[meteorite-list] LOVINA REVISITED

2009-12-09 Thread Darryl Pitt


Well, I had an interesting day today

This morning I met with Roy Clarke, Linda Welzenbach, Cari Corrigan,  
Glen MacPherson, and Tim McCoy at the Smithsonian.   During our get- 
together Tim made several observations as to why Lovina could very  
well not be what it has been made out to be---which is to say, a  
meteorite---and why more work must be done.


In Tim's words

1)   The sulfides are not simply troilite and appear optically to be  
multiple phases, including one that looks like the Ni-rich sulfide  
pentlandite.


2)  Although the presence of the octahedrons has been attributed to  
weathering, the structure of the remainder of the meteorite shows fine  
stringers of sulfide, not large areas that would easily weather out  
leaving such octahedron.


3)  On one polished slice, the sulfides clearly wrap around one of the  
indentations, rather than the cross-cutting relationship one might  
expect from a significantly weathered iron meteorite.


4)  The composition given - high Ni coupled with moderately high Ga  
and Ge - is difficult to reconcile with a meteorite composition.
Iron meteorites acquire high Ni concentrations through 1 of 3  
mechanisms.  Oxidation simply changes iron to FeO, leaving Ni behind.   
This can produce high-Ni irons with modest Ga and Ge. Nebular  
condensation can also produce high-Ni iron which then melts to form  
cores in which high-Ni iron meteorites form.  This process, however,  
occurs at high temperature where the volatile elements Ga and Ge are  
depleted.  Finally, you can produce high Ni through fractional  
crystallization.  Ni prefers the solid phase when a core crystallizes,  
so early irons are low in Ni and later crystallizing ones are high in  
Ni.  However, Ga and Ge behave opposite of Ni, so low Ni irons are  
high in Ga and Ge and high Ni irons are low and Ga and Ge.   The  
published Ga and Ge values are at least a factor of 15 higher than  
reported for similar iron meteorites.


5)  The holes exposed in the center of the specimen are not the shape  
one would expect of weathering, but seem circular.  Circular vugs are  
commonly produced in slags when gases try to escape.


There was more...including the fact that Indonesia is a nickel-rich  
locality as well as Tim's conclusion that Lovina was most likely a  
highly weathered example of a smelted Ni-rich sulfide.


Sales have been suspended and monies are in the process of being  
returned.  Further testing will be done to confirm Lovina's place of  
origin and the results will be posted to the list by mid-January.


I think I'll go see the new Clooney film Up In The Air.   Ohhh---and  
might anyone want an inexpensive 13 kg specimen of Willamette for  
Christmas?!



And how was your day?   ;-)


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Re: [meteorite-list] LOVINA REVISITED

2009-12-09 Thread Matthias Bärmann

Hello Darryl,

gosh, so you've to arrange yourself with the fact that perhaps you only have 
a part of the spaceship which tried to escape from the sinking Atlantis 
instead of a meteorite. In any case: it still looks fantastic.


Best regards,

Matthias

- Original Message - 
From: Darryl Pitt dar...@dof3.com

To: Adam List meteorite-list@meteoritecentral.com
Sent: Wednesday, December 09, 2009 9:15 AM
Subject: [meteorite-list] LOVINA REVISITED




Well, I had an interesting day today

This morning I met with Roy Clarke, Linda Welzenbach, Cari Corrigan,  Glen 
MacPherson, and Tim McCoy at the Smithsonian.   During our get- together 
Tim made several observations as to why Lovina could very  well not be 
what it has been made out to be---which is to say, a  meteorite---and why 
more work must be done.


In Tim's words

1)   The sulfides are not simply troilite and appear optically to be 
multiple phases, including one that looks like the Ni-rich sulfide 
pentlandite.


2)  Although the presence of the octahedrons has been attributed to 
weathering, the structure of the remainder of the meteorite shows fine 
stringers of sulfide, not large areas that would easily weather out 
leaving such octahedron.


3)  On one polished slice, the sulfides clearly wrap around one of the 
indentations, rather than the cross-cutting relationship one might  expect 
from a significantly weathered iron meteorite.


4)  The composition given - high Ni coupled with moderately high Ga  and 
Ge - is difficult to reconcile with a meteorite composition.Iron 
meteorites acquire high Ni concentrations through 1 of 3  mechanisms. 
Oxidation simply changes iron to FeO, leaving Ni behind.   This can 
produce high-Ni irons with modest Ga and Ge. Nebular  condensation can 
also produce high-Ni iron which then melts to form  cores in which high-Ni 
iron meteorites form.  This process, however,  occurs at high temperature 
where the volatile elements Ga and Ge are  depleted.  Finally, you can 
produce high Ni through fractional  crystallization.  Ni prefers the solid 
phase when a core crystallizes,  so early irons are low in Ni and later 
crystallizing ones are high in  Ni.  However, Ga and Ge behave opposite of 
Ni, so low Ni irons are  high in Ga and Ge and high Ni irons are low and 
Ga and Ge.   The  published Ga and Ge values are at least a factor of 15 
higher than  reported for similar iron meteorites.


5)  The holes exposed in the center of the specimen are not the shape  one 
would expect of weathering, but seem circular.  Circular vugs are 
commonly produced in slags when gases try to escape.


There was more...including the fact that Indonesia is a nickel-rich 
locality as well as Tim's conclusion that Lovina was most likely a  highly 
weathered example of a smelted Ni-rich sulfide.


Sales have been suspended and monies are in the process of being 
returned.  Further testing will be done to confirm Lovina's place of 
origin and the results will be posted to the list by mid-January.


I think I'll go see the new Clooney film Up In The Air.   Ohhh---and 
might anyone want an inexpensive 13 kg specimen of Willamette for 
Christmas?!



And how was your day?   ;-)


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Re: [meteorite-list] LOVINA REVISITED

2009-12-09 Thread i...@niger-meteorite-recon.de
Thank you for the new evaluation Darryl.

Although this is a regrettable development one must not forget that you took
the initial risk of acquiring such exotic material, which alone is a
remarkable achievement. I very much hope that this experience does not
discourage you to venture similar acquisitions in the future. If it wasn't for
people like you, most meteorites of similar caliber would never see the light of
public. Set backs are a natural part of this business and there are very few
dealers who would not subscribe to that.

Svend



   

Darryl Pitt dar...@dof3.com hat am 9. Dezember 2009 um 09:15 geschrieben:

 
 Well, I had an interesting day today
 
 This morning I met with Roy Clarke, Linda Welzenbach, Cari Corrigan,  
 Glen MacPherson, and Tim McCoy at the Smithsonian.   During our get- 
 together Tim made several observations as to why Lovina could very  
 well not be what it has been made out to be---which is to say, a  
 meteorite---and why more work must be done.
 
 In Tim's words
 
 1)   The sulfides are not simply troilite and appear optically to be  
 multiple phases, including one that looks like the Ni-rich sulfide  
 pentlandite.
 
 2)  Although the presence of the octahedrons has been attributed to  
 weathering, the structure of the remainder of the meteorite shows fine  
 stringers of sulfide, not large areas that would easily weather out  
 leaving such octahedron.
 
 3)  On one polished slice, the sulfides clearly wrap around one of the  
 indentations, rather than the cross-cutting relationship one might  
 expect from a significantly weathered iron meteorite.
 
 4)  The composition given - high Ni coupled with moderately high Ga  
 and Ge - is difficult to reconcile with a meteorite composition.    
 Iron meteorites acquire high Ni concentrations through 1 of 3  
 mechanisms.  Oxidation simply changes iron to FeO, leaving Ni behind.   
 This can produce high-Ni irons with modest Ga and Ge. Nebular  
 condensation can also produce high-Ni iron which then melts to form  
 cores in which high-Ni iron meteorites form.  This process, however,  
 occurs at high temperature where the volatile elements Ga and Ge are  
 depleted.  Finally, you can produce high Ni through fractional  
 crystallization.  Ni prefers the solid phase when a core crystallizes,  
 so early irons are low in Ni and later crystallizing ones are high in  
 Ni.  However, Ga and Ge behave opposite of Ni, so low Ni irons are  
 high in Ga and Ge and high Ni irons are low and Ga and Ge.   The  
 published Ga and Ge values are at least a factor of 15 higher than  
 reported for similar iron meteorites.
 
 5)  The holes exposed in the center of the specimen are not the shape  
 one would expect of weathering, but seem circular.  Circular vugs are  
 commonly produced in slags when gases try to escape.
 
 There was more...including the fact that Indonesia is a nickel-rich  
 locality as well as Tim's conclusion that Lovina was most likely a  
 highly weathered example of a smelted Ni-rich sulfide.
 
 Sales have been suspended and monies are in the process of being  
 returned.  Further testing will be done to confirm Lovina's place of  
 origin and the results will be posted to the list by mid-January.
 
 I think I'll go see the new Clooney film Up In The Air.   Ohhh---and  
 might anyone want an inexpensive 13 kg specimen of Willamette for  
 Christmas?!
 
 
 And how was your day?   ;-)
 
 
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Re: [meteorite-list] LOVINA REVISITED

2009-12-09 Thread Darryl Pitt



Thanks for your kind words, Svend, but you're giving me far more  
credit than I deserve.  I did not shepherd Lovina through the  
certification process.  My acquisition simply would not have occurred  
had Lovina not been previously certified as a meteorite.


Please see the relevant article in Lunar and Planetary Science:  
http://www.lpi.usra.edu/meetings/lpsc2008/pdf/2412.pdf




On Dec 9, 2009, at 7:08 AM, i...@niger-meteorite-recon.de wrote:


Thank you for the new evaluation Darryl.

Although this is a regrettable development one must not forget that  
you took

the initial risk of acquiring such exotic material, which alone is a
remarkable achievement. I very much hope that this experience does not
discourage you to venture similar acquisitions in the future. If it  
wasn't for
people like you, most meteorites of similar caliber would never see  
the light of
public. Set backs are a natural part of this business and there are  
very few

dealers who would not subscribe to that.

Svend





Darryl Pitt dar...@dof3.com hat am 9. Dezember 2009 um 09:15  
geschrieben:




Well, I had an interesting day today

This morning I met with Roy Clarke, Linda Welzenbach, Cari Corrigan,
Glen MacPherson, and Tim McCoy at the Smithsonian.   During our get-
together Tim made several observations as to why Lovina could very
well not be what it has been made out to be---which is to say, a
meteorite---and why more work must be done.

In Tim's words

1)   The sulfides are not simply troilite and appear optically to be
multiple phases, including one that looks like the Ni-rich sulfide
pentlandite.

2)  Although the presence of the octahedrons has been attributed to
weathering, the structure of the remainder of the meteorite shows  
fine

stringers of sulfide, not large areas that would easily weather out
leaving such octahedron.

3)  On one polished slice, the sulfides clearly wrap around one of  
the

indentations, rather than the cross-cutting relationship one might
expect from a significantly weathered iron meteorite.

4)  The composition given - high Ni coupled with moderately high Ga
and Ge - is difficult to reconcile with a meteorite composition.
Iron meteorites acquire high Ni concentrations through 1 of 3
mechanisms.  Oxidation simply changes iron to FeO, leaving Ni behind.
This can produce high-Ni irons with modest Ga and Ge. Nebular
condensation can also produce high-Ni iron which then melts to form
cores in which high-Ni iron meteorites form.  This process, however,
occurs at high temperature where the volatile elements Ga and Ge are
depleted.  Finally, you can produce high Ni through fractional
crystallization.  Ni prefers the solid phase when a core  
crystallizes,

so early irons are low in Ni and later crystallizing ones are high in
Ni.  However, Ga and Ge behave opposite of Ni, so low Ni irons are
high in Ga and Ge and high Ni irons are low and Ga and Ge.   The
published Ga and Ge values are at least a factor of 15 higher than
reported for similar iron meteorites.

5)  The holes exposed in the center of the specimen are not the shape
one would expect of weathering, but seem circular.  Circular vugs are
commonly produced in slags when gases try to escape.

There was more...including the fact that Indonesia is a nickel-rich
locality as well as Tim's conclusion that Lovina was most likely a
highly weathered example of a smelted Ni-rich sulfide.

Sales have been suspended and monies are in the process of being
returned.  Further testing will be done to confirm Lovina's place of
origin and the results will be posted to the list by mid-January.

I think I'll go see the new Clooney film Up In The Air.   Ohhh--- 
and

might anyone want an inexpensive 13 kg specimen of Willamette for
Christmas?!


And how was your day?   ;-)


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