Re: [meteorite-list] EETA 79001 and the Martian Atmosphere

2011-02-11 Thread Jeff Kuyken
It's been quite a few years since I've looked up close at this piece but 
here's a Ureilite with something similar.


http://www.meteorites.com.au/features/nwa2624.html

Cheers,

Jeff


- Original Message - 
From: Richard Montgomery rickm...@earthlink.net
To: cdtuc...@cox.net; Martin Altmann altm...@meteorite-martin.de; 
meteorite-list@meteoritecentral.com

Sent: Thursday, February 10, 2011 6:42 AM
Subject: Re: [meteorite-list] EETA 79001 and the Martian Atmosphere


Hi List.  (Sorry if this is a duplicate post.)  I have the remnants of a 
550gr Brahin slice that definitely has bubbles in the olivine in a few 
spots.  Any comments?



- Original Message - 
From: cdtuc...@cox.net
To: Martin Altmann altm...@meteorite-martin.de; 
meteorite-list@meteoritecentral.com

Sent: Wednesday, February 09, 2011 11:24 AM
Subject: Re: [meteorite-list] EETA 79001 and the Martian Atmosphere



Martin,List,
Interesting that you mention bubbles in Maskelynite.
I have a great picture taken by Tom Phillips of an amazing River Of 
Maskelynite With Bubbles
Although this is from an unclassified meteorite it does check out pretty 
well both visually in thin section but, the chemistry is also correct for 
either a Lunar or a Martian meteorite,

I'm sure Blain won't mind me mentioning that;
At this Tucson Gem Show  Blain Reed has acquired an amazing piece of 
hardware.
It is called an XRF for X-ray Florescence. This is a hand held portable 
gun like instrument that when held up to the rock gives you an average of 
the chemistry it sniffs out of the rock.
Blain was kind enough to use this machine  to collect reading from known 
Lunar rocks in his collection (this way he knows they are in fact 
Lunar's) With this info he can compare the Known data with new 
Candidates. This for a small fee and it only takes about a minute. 
AMAZING . Blain rocks.
In this way he has determined that this rock I show here with the river 
Of Maskelynite and Bubbles has a very good chance at being either Lunar 
of Martian. Apparently they are quite similar in this way.

Although, The Numbers are dead on Lunar for this one. .
Not only are the bulk amounts correct but so, are the Ratios. Especially 
the Fe/ Mn and so forth.

Please see the attached pics and share your opinion.
Any Scientists out there want to take a look?
I also have another that Tom Phillips photographed that also checks out 
both Chemically and petrographically as Lunar or Martian  but, with no 
visible river yet? It looks like mostly Olivine? But this ones Fe/Mn is 
definitely in the Martian Range. Very Cool.


http://www.flickr.com/photos/13030472@N07/?saved=1

Any and all comments welcome.
Email for more pics.
Best regards,
Carl
Carl or Debbie Esparza
Meteoritemax


 Martin Altmann altm...@meteorite-martin.de wrote:

Hi Walter,

only a remark...   for not being the same thing like with the ominous 
purple

halite-crystals containing liquid water in Zag,
which are described in literature - but so far noone of the 
collectors

ever found one in any of their 175kgs of slices...  :-)

Those inclusions in the Martian shock glasses - you can really have them 
as

a collector too!!

The fresh-shergottite-series - NWA 2975/2986/4766 seq..
there the maskelynite is still so fresh, that it is translucent.
So it's possible without special equipment and special preparation to 
spot

these inclusions in the maskelynite with a simple microscope under low
magnification in cut surfaces.

And you know what? Here and there these maskelynite patches contain 
little

bubbles!

A while ago a collector loaded up a photo he made from such a bubble out 
of

that NWA-series in the German forum.

Fascinating isn't it?

So, dear collectors, I'm sure many of you have samples form that 
Martian,

let's hunt for bubbles!


Best!
Martin

-Ursprüngliche Nachricht-
Von: meteorite-list-boun...@meteoritecentral.com
[mailto:meteorite-list-boun...@meteoritecentral.com] Im Auftrag von 
Walter

Branch
Gesendet: Mittwoch, 9. Februar 2011 04:31
An: MeteorList
Betreff: [meteorite-list] EETA 79001 and the Martian Atmosphere

Hello Everyone,

I feel like an idiot.

I know that trapped atmospheric gases have been found in some martian
meteorites but for some unexplained reason, I had always thought that 
the
gases had been incorporated in the rock at the time of formation. I 
always
wondered how gases from the martian atmosphere could have been trapped 
in a
rock at the time it formed, particularly an igneous rock in an 
underground

magma chamber.

Well, thanks to William Cassidy, the man who founded ANSMET, I now 
realize
my assumption was wrong. Cassidy makes it clear that gasses became 
trapped
in martian rocks at the time of the impact which launched the rock from 
the
surface. The rather lengthy quote below is from Cassidy's book 
Meteorites,

Ice and Antarctica an excellent book (see more after the quote).

From pages 119-121

EETA 79001 was an important find for another reason. It contained

Re: [meteorite-list] EETA 79001 and the Martian Atmosphere

2011-02-09 Thread Martin Altmann
Hi Walter,

only a remark...   for not being the same thing like with the ominous purple
halite-crystals containing liquid water in Zag,
which are described in literature - but so far noone of the collectors
ever found one in any of their 175kgs of slices...  :-)

Those inclusions in the Martian shock glasses - you can really have them as
a collector too!!

The fresh-shergottite-series - NWA 2975/2986/4766 seq..
there the maskelynite is still so fresh, that it is translucent.
So it's possible without special equipment and special preparation to spot
these inclusions in the maskelynite with a simple microscope under low
magnification in cut surfaces.

And you know what? Here and there these maskelynite patches contain little
bubbles!

A while ago a collector loaded up a photo he made from such a bubble out of
that NWA-series in the German forum.

Fascinating isn't it?

So, dear collectors, I'm sure many of you have samples form that Martian,
let's hunt for bubbles!


Best!
Martin

-Ursprüngliche Nachricht-
Von: meteorite-list-boun...@meteoritecentral.com
[mailto:meteorite-list-boun...@meteoritecentral.com] Im Auftrag von Walter
Branch
Gesendet: Mittwoch, 9. Februar 2011 04:31
An: MeteorList
Betreff: [meteorite-list] EETA 79001 and the Martian Atmosphere

Hello Everyone,

I feel like an idiot.

I know that trapped atmospheric gases have been found in some martian 
meteorites but for some unexplained reason, I had always thought that the 
gases had been incorporated in the rock at the time of formation. I always 
wondered how gases from the martian atmosphere could have been trapped in a 
rock at the time it formed, particularly an igneous rock in an underground 
magma chamber.

Well, thanks to William Cassidy, the man who founded ANSMET, I now realize 
my assumption was wrong. Cassidy makes it clear that gasses became trapped 
in martian rocks at the time of the impact which launched the rock from the 
surface. The rather lengthy quote below is from Cassidy's book Meteorites, 
Ice and Antarctica an excellent book (see more after the quote).

From pages 119-121

EETA 79001 was an important find for another reason. It contained proof that

SNC meteorites come from Mars. This meteorite had been highly shocked during

the impact that ejected it from the martian surface, and one of the shock 
effects was to produce pods of glass that had been melted from the 
constituent minerals of the meteorite by the transient heating generated by 
shock pressures. The melts that were formed were partly injected along 
cracks in the rock and partly retained as molten beads at the sites where 
they formed. Cooling occurred immediately behind the shock wave and the 
beads were chilled to glass before they could crystalize. Apparently the 
crater forming asteroid had built up a lense off compressed atmosphere in 
front of it during it's lengthy trajectory toward the surface of the planet.

When it struck the surface it injected highly compressed air into the target

rock, and some of this was trapped in the shock-melted inclusions. We know 
the composition of the martian atmosphere from measurements made by Viking 
Landers I and II. When some of the glass inclusions were picked out of EETA 
79001 and remelted, the gave up their dissolved gases. These gasses when 
analyzed and corrected for slight terrestrial contamination, contained 
nitrogen and carbon dioxide in the same abundances as the atmosphere of 
Mars; they also had isotopes of argon, neon, , krypton, and xenon in the 
same abundances as does the martian atmosphere. This neat bit of detective 
work by a number of workers, for the first time tied a SNC meteorite 
directly to the planet Mars and, through this meteorite, to all the other 
meteorites.

I love Cassidy's book. If you like meteorites in general, martian and lunar 
meteorites (like me) and are curious about the ANSMET program and you don't 
have a copy of this book, you are really missing out. The book is a gold 
mine of information regarding ANSMET. It is very readable, technical in some

places, humorous in others and poignant in others. Some books I love holding

and reading and this is one of those books. It is hardbound with glossy 
pages and nicely illustrated. I like the physical proportion of the book and

I even like the dust jacket (I usually abhor dust jackets).

Anyway, many thanks to Dr. Cassidy for clearing that up with me and thanks 
for writing such a wonderful book.

-Walter Branch

__
Visit the Archives at
http://www.meteoritecentral.com/mailing-list-archives.html
Meteorite-list mailing list
Meteorite-list@meteoritecentral.com
http://six.pairlist.net/mailman/listinfo/meteorite-list

__
Visit the Archives at http://www.meteoritecentral.com/mailing-list-archives.html
Meteorite-list mailing list
Meteorite-list@meteoritecentral.com
http://six.pairlist.net/mailman/listinfo/meteorite-list


Re: [meteorite-list] EETA 79001 and the Martian Atmosphere

2011-02-09 Thread cdtucson
Martin,List,
Interesting that you mention bubbles in Maskelynite.
I have a great picture taken by Tom Phillips of an amazing River Of 
Maskelynite With Bubbles
Although this is from an unclassified meteorite it does check out pretty well 
both visually in thin section but, the chemistry is also correct for either a 
Lunar or a Martian meteorite,
I'm sure Blain won't mind me mentioning that;
At this Tucson Gem Show  Blain Reed has acquired an amazing piece of hardware.
It is called an XRF for X-ray Florescence. This is a hand held portable gun 
like instrument that when held up to the rock gives you an average of the 
chemistry it sniffs out of the rock. 
Blain was kind enough to use this machine  to collect reading from known Lunar 
rocks in his collection (this way he knows they are in fact Lunar's) With this 
info he can compare the Known data with new Candidates. This for a small fee 
and it only takes about a minute. AMAZING . Blain rocks.
In this way he has determined that this rock I show here with the river Of 
Maskelynite and Bubbles has a very good chance at being either Lunar of 
Martian. Apparently they are quite similar in this way. 
Although, The Numbers are dead on Lunar for this one. . 
Not only are the bulk amounts correct but so, are the Ratios. Especially the 
Fe/ Mn and so forth. 
Please see the attached pics and share your opinion.
Any Scientists out there want to take a look?
I also have another that Tom Phillips photographed that also checks out both 
Chemically and petrographically as Lunar or Martian  but, with no visible river 
yet? It looks like mostly Olivine? But this ones Fe/Mn is definitely in the 
Martian Range. Very Cool.

 http://www.flickr.com/photos/13030472@N07/?saved=1

Any and all comments welcome.
Email for more pics. 
Best regards,
Carl
Carl or Debbie Esparza
Meteoritemax


 Martin Altmann altm...@meteorite-martin.de wrote: 
 Hi Walter,
 
 only a remark...   for not being the same thing like with the ominous purple
 halite-crystals containing liquid water in Zag,
 which are described in literature - but so far noone of the collectors
 ever found one in any of their 175kgs of slices...  :-)
 
 Those inclusions in the Martian shock glasses - you can really have them as
 a collector too!!
 
 The fresh-shergottite-series - NWA 2975/2986/4766 seq..
 there the maskelynite is still so fresh, that it is translucent.
 So it's possible without special equipment and special preparation to spot
 these inclusions in the maskelynite with a simple microscope under low
 magnification in cut surfaces.
 
 And you know what? Here and there these maskelynite patches contain little
 bubbles!
 
 A while ago a collector loaded up a photo he made from such a bubble out of
 that NWA-series in the German forum.
 
 Fascinating isn't it?
 
 So, dear collectors, I'm sure many of you have samples form that Martian,
 let's hunt for bubbles!
 
 
 Best!
 Martin
 
 -Ursprüngliche Nachricht-
 Von: meteorite-list-boun...@meteoritecentral.com
 [mailto:meteorite-list-boun...@meteoritecentral.com] Im Auftrag von Walter
 Branch
 Gesendet: Mittwoch, 9. Februar 2011 04:31
 An: MeteorList
 Betreff: [meteorite-list] EETA 79001 and the Martian Atmosphere
 
 Hello Everyone,
 
 I feel like an idiot.
 
 I know that trapped atmospheric gases have been found in some martian 
 meteorites but for some unexplained reason, I had always thought that the 
 gases had been incorporated in the rock at the time of formation. I always 
 wondered how gases from the martian atmosphere could have been trapped in a 
 rock at the time it formed, particularly an igneous rock in an underground 
 magma chamber.
 
 Well, thanks to William Cassidy, the man who founded ANSMET, I now realize 
 my assumption was wrong. Cassidy makes it clear that gasses became trapped 
 in martian rocks at the time of the impact which launched the rock from the 
 surface. The rather lengthy quote below is from Cassidy's book Meteorites, 
 Ice and Antarctica an excellent book (see more after the quote).
 
 From pages 119-121
 
 EETA 79001 was an important find for another reason. It contained proof that
 
 SNC meteorites come from Mars. This meteorite had been highly shocked during
 
 the impact that ejected it from the martian surface, and one of the shock 
 effects was to produce pods of glass that had been melted from the 
 constituent minerals of the meteorite by the transient heating generated by 
 shock pressures. The melts that were formed were partly injected along 
 cracks in the rock and partly retained as molten beads at the sites where 
 they formed. Cooling occurred immediately behind the shock wave and the 
 beads were chilled to glass before they could crystalize. Apparently the 
 crater forming asteroid had built up a lense off compressed atmosphere in 
 front of it during it's lengthy trajectory toward the surface of the planet.
 
 When it struck the surface it injected highly compressed air into the target
 
 rock

Re: [meteorite-list] EETA 79001 and the Martian Atmosphere

2011-02-09 Thread Richard Montgomery
Hi List.  (Sorry if this is a duplicate post.)  I have the remnants of a 
550gr Brahin slice that definitely has bubbles in the olivine in a few 
spots.  Any comments?



- Original Message - 
From: cdtuc...@cox.net
To: Martin Altmann altm...@meteorite-martin.de; 
meteorite-list@meteoritecentral.com

Sent: Wednesday, February 09, 2011 11:24 AM
Subject: Re: [meteorite-list] EETA 79001 and the Martian Atmosphere



Martin,List,
Interesting that you mention bubbles in Maskelynite.
I have a great picture taken by Tom Phillips of an amazing River Of 
Maskelynite With Bubbles
Although this is from an unclassified meteorite it does check out pretty 
well both visually in thin section but, the chemistry is also correct for 
either a Lunar or a Martian meteorite,

I'm sure Blain won't mind me mentioning that;
At this Tucson Gem Show  Blain Reed has acquired an amazing piece of 
hardware.
It is called an XRF for X-ray Florescence. This is a hand held portable 
gun like instrument that when held up to the rock gives you an average of 
the chemistry it sniffs out of the rock.
Blain was kind enough to use this machine  to collect reading from known 
Lunar rocks in his collection (this way he knows they are in fact Lunar's) 
With this info he can compare the Known data with new Candidates. This for 
a small fee and it only takes about a minute. AMAZING . Blain rocks.
In this way he has determined that this rock I show here with the river 
Of Maskelynite and Bubbles has a very good chance at being either Lunar 
of Martian. Apparently they are quite similar in this way.

Although, The Numbers are dead on Lunar for this one. .
Not only are the bulk amounts correct but so, are the Ratios. Especially 
the Fe/ Mn and so forth.

Please see the attached pics and share your opinion.
Any Scientists out there want to take a look?
I also have another that Tom Phillips photographed that also checks out 
both Chemically and petrographically as Lunar or Martian  but, with no 
visible river yet? It looks like mostly Olivine? But this ones Fe/Mn is 
definitely in the Martian Range. Very Cool.


http://www.flickr.com/photos/13030472@N07/?saved=1

Any and all comments welcome.
Email for more pics.
Best regards,
Carl
Carl or Debbie Esparza
Meteoritemax


 Martin Altmann altm...@meteorite-martin.de wrote:

Hi Walter,

only a remark...   for not being the same thing like with the ominous 
purple

halite-crystals containing liquid water in Zag,
which are described in literature - but so far noone of the 
collectors

ever found one in any of their 175kgs of slices...  :-)

Those inclusions in the Martian shock glasses - you can really have them 
as

a collector too!!

The fresh-shergottite-series - NWA 2975/2986/4766 seq..
there the maskelynite is still so fresh, that it is translucent.
So it's possible without special equipment and special preparation to 
spot

these inclusions in the maskelynite with a simple microscope under low
magnification in cut surfaces.

And you know what? Here and there these maskelynite patches contain 
little

bubbles!

A while ago a collector loaded up a photo he made from such a bubble out 
of

that NWA-series in the German forum.

Fascinating isn't it?

So, dear collectors, I'm sure many of you have samples form that Martian,
let's hunt for bubbles!


Best!
Martin

-Ursprüngliche Nachricht-
Von: meteorite-list-boun...@meteoritecentral.com
[mailto:meteorite-list-boun...@meteoritecentral.com] Im Auftrag von 
Walter

Branch
Gesendet: Mittwoch, 9. Februar 2011 04:31
An: MeteorList
Betreff: [meteorite-list] EETA 79001 and the Martian Atmosphere

Hello Everyone,

I feel like an idiot.

I know that trapped atmospheric gases have been found in some martian
meteorites but for some unexplained reason, I had always thought that the
gases had been incorporated in the rock at the time of formation. I 
always
wondered how gases from the martian atmosphere could have been trapped in 
a
rock at the time it formed, particularly an igneous rock in an 
underground

magma chamber.

Well, thanks to William Cassidy, the man who founded ANSMET, I now 
realize
my assumption was wrong. Cassidy makes it clear that gasses became 
trapped
in martian rocks at the time of the impact which launched the rock from 
the
surface. The rather lengthy quote below is from Cassidy's book 
Meteorites,

Ice and Antarctica an excellent book (see more after the quote).

From pages 119-121

EETA 79001 was an important find for another reason. It contained proof 
that


SNC meteorites come from Mars. This meteorite had been highly shocked 
during


the impact that ejected it from the martian surface, and one of the shock
effects was to produce pods of glass that had been melted from the
constituent minerals of the meteorite by the transient heating generated 
by

shock pressures. The melts that were formed were partly injected along
cracks in the rock and partly retained as molten beads at the sites where
they formed. Cooling

[meteorite-list] EETA 79001 and the Martian Atmosphere

2011-02-08 Thread Walter Branch

Hello Everyone,

I feel like an idiot.

I know that trapped atmospheric gases have been found in some martian 
meteorites but for some unexplained reason, I had always thought that the 
gases had been incorporated in the rock at the time of formation. I always 
wondered how gases from the martian atmosphere could have been trapped in a 
rock at the time it formed, particularly an igneous rock in an underground 
magma chamber.


Well, thanks to William Cassidy, the man who founded ANSMET, I now realize 
my assumption was wrong. Cassidy makes it clear that gasses became trapped 
in martian rocks at the time of the impact which launched the rock from the 
surface. The rather lengthy quote below is from Cassidy's book Meteorites, 
Ice and Antarctica an excellent book (see more after the quote).



From pages 119-121


EETA 79001 was an important find for another reason. It contained proof that 
SNC meteorites come from Mars. This meteorite had been highly shocked during 
the impact that ejected it from the martian surface, and one of the shock 
effects was to produce pods of glass that had been melted from the 
constituent minerals of the meteorite by the transient heating generated by 
shock pressures. The melts that were formed were partly injected along 
cracks in the rock and partly retained as molten beads at the sites where 
they formed. Cooling occurred immediately behind the shock wave and the 
beads were chilled to glass before they could crystalize. Apparently the 
crater forming asteroid had built up a lense off compressed atmosphere in 
front of it during it's lengthy trajectory toward the surface of the planet. 
When it struck the surface it injected highly compressed air into the target 
rock, and some of this was trapped in the shock-melted inclusions. We know 
the composition of the martian atmosphere from measurements made by Viking 
Landers I and II. When some of the glass inclusions were picked out of EETA 
79001 and remelted, the gave up their dissolved gases. These gasses when 
analyzed and corrected for slight terrestrial contamination, contained 
nitrogen and carbon dioxide in the same abundances as the atmosphere of 
Mars; they also had isotopes of argon, neon, , krypton, and xenon in the 
same abundances as does the martian atmosphere. This neat bit of detective 
work by a number of workers, for the first time tied a SNC meteorite 
directly to the planet Mars and, through this meteorite, to all the other 
meteorites.


I love Cassidy's book. If you like meteorites in general, martian and lunar 
meteorites (like me) and are curious about the ANSMET program and you don't 
have a copy of this book, you are really missing out. The book is a gold 
mine of information regarding ANSMET. It is very readable, technical in some 
places, humorous in others and poignant in others. Some books I love holding 
and reading and this is one of those books. It is hardbound with glossy 
pages and nicely illustrated. I like the physical proportion of the book and 
I even like the dust jacket (I usually abhor dust jackets).


Anyway, many thanks to Dr. Cassidy for clearing that up with me and thanks 
for writing such a wonderful book.


-Walter Branch

__
Visit the Archives at http://www.meteoritecentral.com/mailing-list-archives.html
Meteorite-list mailing list
Meteorite-list@meteoritecentral.com
http://six.pairlist.net/mailman/listinfo/meteorite-list