Re: [meteorite-list] Rocks from Space Picture of the Day - June 15, 2008

2008-06-16 Thread Rob Matson
Hi Michael,

Awesome image of the large, recent Kainsaz find!  When I saw that
shape, I was sure I'd seen it before...

http://www.rocksfromspace.org/June_15_2008.html
http://images.wikia.com/starwars/images/1/1b/Sandcrawler.jpg

--Rob ;-)

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Re: [meteorite-list] Am I missing something here?

2008-06-16 Thread Jeff Grossman

Dear Martin and list,

I can't comment on the CO3 oxymoron, but I am the inventor of the 
type 3.05 classification, so I can comment on that.


As we have studied type 3 chondrites over the last 30 years, 
especially ordinary and CO chondrites, we have been gradually 
refining the 1967 Van Schmus and Wood classification scheme.  In 
1980, we realized that type 3 chondrites alone showed as great a 
range of metamorphic effects as type 4-6 did, so Sears and coworkers 
including me, proposed subdividing type 3 into types 3.0-3.9.  In 
2005, Grossman and Brearley (2005) described a similar wide range of 
metamorphic effects just between types 3.0 and 3.2 and subdivided 
this into 3.00-3.15 by steps of 0.05.  Since then, we have even begun 
to recognize different levels of metamorphic heating between types 
3.00 and 3.05, and so we find Acfer 094 at type 3.00, Semarkona at 
type 3.01, ALHA77307 at type 3.03 (e.g., Bonal et al. 2007; Kimura, 
Grossman and Weisberg, 2008, MAPS in press).


These differences are quite real and important.  In type 3.05 
ordinary chondrites, the olivine in chondrules has begun to decompose 
from its high-temperature state, the matrix chemistry is quite 
different, especially for sulfur, and the metal has greatly changed 
in structure and composition (all compared to the much, much rarer 
type 3.00-3.01 chondrites).  Although these numbers do not tell you 
the peak metamorphic temperature, they are very useful in describing 
the various transitions that occur during metamorphic heating.


The fact that there may be many possible combinations of chemical 
group and petrologic type is a good thing, although there certainly 
aren't 1500.  Basically, current usage is 3.00-3.04 (5 categories), 
3.05-3.15 (3 categories), 3.2-3.9 (8 catagories), 4-7 (4 categories) 
= 20 categories.  I suppose if you double this for classifiers who 
can't make up their minds, you get ~40 categories, times 3 chondrite 
groups plus 2 transitional groups = ~200 total combinations.


Jeff

At 11:24 PM 6/15/2008, Dark Matter wrote:

Hi All,

Twice in the past few days, I found myself staring at the screen in
confused disbelief. The two statements in sales ads:


a yet unclassified CO3

and

absolutely rare type L3.05 !

just seem to me to border on absurdity. How can a unclassified
specimen be identified by its classification?

And if we carry petrological grade to the hundredths, then
theoretically we could have over 1500 ordinary chondrite designations
not to mention all the transitional possibilities. I fail to see how
that level of hypothetical opinionated hair splitting could do any
good...except for ebay sales ads that is.

Just an evening though when I should be working on something else.

Cheers,

Martin
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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] Am I missing something here?

2008-06-16 Thread Alexander Seidel
Hi Jeff,

if this is state of the art of the classification scheme, and has been accepted 
by a majority of the meteoriticists, does this mean some important primitive 
meteorites finally need a refinement of their established classifications?

I am thinking of (e. g.) the Krymka meteorite, which to my knowledge is an 
LL3.1. Does this have to be refined to become either an LL3.05, or an LL3.10, 
or an LL3.15 in the end?

Just curious,
Alex
Berlin/Germany


 Original-Nachricht 
 Datum: Mon, 16 Jun 2008 07:36:53 -0400
 Von: Jeff Grossman [EMAIL PROTECTED]
 An: Dark Matter [EMAIL PROTECTED], Meteorite List 
 meteorite-list@meteoritecentral.com
 Betreff: Re: [meteorite-list] Am I missing something here?

 Dear Martin and list,
 
 I can't comment on the CO3 oxymoron, but I am the inventor of the 
 type 3.05 classification, so I can comment on that.
 
 As we have studied type 3 chondrites over the last 30 years, 
 especially ordinary and CO chondrites, we have been gradually 
 refining the 1967 Van Schmus and Wood classification scheme.  In 
 1980, we realized that type 3 chondrites alone showed as great a 
 range of metamorphic effects as type 4-6 did, so Sears and coworkers 
 including me, proposed subdividing type 3 into types 3.0-3.9.  In 
 2005, Grossman and Brearley (2005) described a similar wide range of 
 metamorphic effects just between types 3.0 and 3.2 and subdivided 
 this into 3.00-3.15 by steps of 0.05.  Since then, we have even begun 
 to recognize different levels of metamorphic heating between types 
 3.00 and 3.05, and so we find Acfer 094 at type 3.00, Semarkona at 
 type 3.01, ALHA77307 at type 3.03 (e.g., Bonal et al. 2007; Kimura, 
 Grossman and Weisberg, 2008, MAPS in press).
 
 These differences are quite real and important.  In type 3.05 
 ordinary chondrites, the olivine in chondrules has begun to decompose 
 from its high-temperature state, the matrix chemistry is quite 
 different, especially for sulfur, and the metal has greatly changed 
 in structure and composition (all compared to the much, much rarer 
 type 3.00-3.01 chondrites).  Although these numbers do not tell you 
 the peak metamorphic temperature, they are very useful in describing 
 the various transitions that occur during metamorphic heating.
 
 The fact that there may be many possible combinations of chemical 
 group and petrologic type is a good thing, although there certainly 
 aren't 1500.  Basically, current usage is 3.00-3.04 (5 categories), 
 3.05-3.15 (3 categories), 3.2-3.9 (8 catagories), 4-7 (4 categories) 
 = 20 categories.  I suppose if you double this for classifiers who 
 can't make up their minds, you get ~40 categories, times 3 chondrite 
 groups plus 2 transitional groups = ~200 total combinations.
 
 Jeff
 
 At 11:24 PM 6/15/2008, Dark Matter wrote:
 Hi All,
 
 Twice in the past few days, I found myself staring at the screen in
 confused disbelief. The two statements in sales ads:
 
 
 a yet unclassified CO3
 
 and
 
 absolutely rare type L3.05 !
 
 just seem to me to border on absurdity. How can a unclassified
 specimen be identified by its classification?
 
 And if we carry petrological grade to the hundredths, then
 theoretically we could have over 1500 ordinary chondrite designations
 not to mention all the transitional possibilities. I fail to see how
 that level of hypothetical opinionated hair splitting could do any
 good...except for ebay sales ads that is.
 
 Just an evening though when I should be working on something else.
 
 Cheers,
 
 Martin
 __
 http://www.meteoritecentral.com
 Meteorite-list mailing list
 Meteorite-list@meteoritecentral.com
 http://six.pairlist.net/mailman/listinfo/meteorite-list
 
 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] Am I missing something here?

2008-06-16 Thread info
Martin, others,

as for the unclassified CO3 that was indeed the wrong term. I was referring 
to a CO3 type chondrite whose classification has not yet reached official 
status. I sincerely apologize for causing confused disbelief. 

Svend

www.meteorite-recon.com

 


-
Jeff Grossman wrote:

Dear Martin and list,

I can't comment on the CO3 oxymoron, but I am the inventor of the 
type 3.05 classification, so I can comment on that.

As we have studied type 3 chondrites over the last 30 years, 
especially ordinary and CO chondrites, we have been gradually 
refining the 1967 Van Schmus and Wood classification scheme.  In 
1980, we realized that type 3 chondrites alone showed as great a 
range of metamorphic effects as type 4-6 did, so Sears and coworkers 
including me, proposed subdividing type 3 into types 3.0-3.9.  In 
2005, Grossman and Brearley (2005) described a similar wide range of 
metamorphic effects just between types 3.0 and 3.2 and subdivided 
this into 3.00-3.15 by steps of 0.05.  Since then, we have even begun 
to recognize different levels of metamorphic heating between types 
3.00 and 3.05, and so we find Acfer 094 at type 3.00, Semarkona at 
type 3.01, ALHA77307 at type 3.03 (e.g., Bonal et al. 2007; Kimura, 
Grossman and Weisberg, 2008, MAPS in press).

These differences are quite real and important.  In type 3.05 
ordinary chondrites, the olivine in chondrules has begun to decompose 
from its high-temperature state, the matrix chemistry is quite 
different, especially for sulfur, and the metal has greatly changed 
in structure and composition (all compared to the much, much rarer 
type 3.00-3.01 chondrites).  Although these numbers do not tell you 
the peak metamorphic temperature, they are very useful in describing 
the various transitions that occur during metamorphic heating.

The fact that there may be many possible combinations of chemical 
group and petrologic type is a good thing, although there certainly 
aren't 1500.  Basically, current usage is 3.00-3.04 (5 categories), 
3.05-3.15 (3 categories), 3.2-3.9 (8 catagories), 4-7 (4 categories) 
= 20 categories.  I suppose if you double this for classifiers who 
can't make up their minds, you get ~40 categories, times 3 chondrite 
groups plus 2 transitional groups = ~200 total combinations.

Jeff

At 11:24 PM 6/15/2008, Dark Matter wrote:
Hi All,

Twice in the past few days, I found myself staring at the screen in
confused disbelief. The two statements in sales ads:


a yet unclassified CO3

and

absolutely rare type L3.05 !

just seem to me to border on absurdity. How can a unclassified
specimen be identified by its classification?

And if we carry petrological grade to the hundredths, then
theoretically we could have over 1500 ordinary chondrite designations
not to mention all the transitional possibilities. I fail to see how
that level of hypothetical opinionated hair splitting could do any
good...except for ebay sales ads that is.

Just an evening though when I should be working on something else.

Cheers,

Martin
__
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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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-- 
www.niger-meteorite-recon.de
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Re: [meteorite-list] Am I missing something here?

2008-06-16 Thread Dark Matter
Hello Jeff and All,

Thank you very much for the thorough and thoughtful reply. I certainly
would not disagree with you on such matters.

Now I'm curious if refinement in classification will be made for
Krymka (like Alex):
http://www.meteorite.com/MT_links/2003/March/1krymka.jpg

Bishunpur:
http://www.meteorite-times.com/Back_Links/2005/December/bishunpur.jpg

and what about carbonaceous chondrites like Leoville, currently a
CV3.0 I believe:
http://www.meteorite-times.com/Back_Links/2004/December/leo_cai.jpg

And thanks to Svend for his clarification.

Martin
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Re: [meteorite-list] Am I missing something here?

2008-06-16 Thread Jeff Grossman
Yes.  All of the low-petrologic-type chondrites can be refined.  In 
Grossman and Brearley (2005) we reclassified Krymka as type 3.2 and 
Bishunpur as type 3.15.   Here is the entire set of ordinary 
chondrite petrologic types from that paper:


Semarkona -- 3.00
QUE 97008 -- 3.05
MET 00526 -- 3.05
EET 90161 -- 3.05
NWA 1756 -- 3.10
NWA 3127 -- 3.10
Roosevelt County 075 -- 3.10
MET 96503 -- 3.10
Adrar 003 -- 3.10
Bishunpur -- 3.15
Y-791324 -- 3.15
Y-791558 -- 3.15
Y-793596 -- 3.2
Krymka -- 3.2
GRO 95502 -- 3.2
GRO 95544 -- 3.2


jeff

At 08:11 AM 6/16/2008, Alexander Seidel wrote:

Hi Jeff,

if this is state of the art of the classification scheme, and has 
been accepted by a majority of the meteoriticists, does this mean 
some important primitive meteorites finally need a refinement of 
their established classifications?


I am thinking of (e. g.) the Krymka meteorite, which to my knowledge 
is an LL3.1. Does this have to be refined to become either an 
LL3.05, or an LL3.10, or an LL3.15 in the end?


Just curious,
Alex
Berlin/Germany


 Original-Nachricht 
 Datum: Mon, 16 Jun 2008 07:36:53 -0400
 Von: Jeff Grossman [EMAIL PROTECTED]
 An: Dark Matter [EMAIL PROTECTED], Meteorite List 
meteorite-list@meteoritecentral.com

 Betreff: Re: [meteorite-list] Am I missing something here?

 Dear Martin and list,

 I can't comment on the CO3 oxymoron, but I am the inventor of the
 type 3.05 classification, so I can comment on that.

 As we have studied type 3 chondrites over the last 30 years,
 especially ordinary and CO chondrites, we have been gradually
 refining the 1967 Van Schmus and Wood classification scheme.  In
 1980, we realized that type 3 chondrites alone showed as great a
 range of metamorphic effects as type 4-6 did, so Sears and coworkers
 including me, proposed subdividing type 3 into types 3.0-3.9.  In
 2005, Grossman and Brearley (2005) described a similar wide range of
 metamorphic effects just between types 3.0 and 3.2 and subdivided
 this into 3.00-3.15 by steps of 0.05.  Since then, we have even begun
 to recognize different levels of metamorphic heating between types
 3.00 and 3.05, and so we find Acfer 094 at type 3.00, Semarkona at
 type 3.01, ALHA77307 at type 3.03 (e.g., Bonal et al. 2007; Kimura,
 Grossman and Weisberg, 2008, MAPS in press).

 These differences are quite real and important.  In type 3.05
 ordinary chondrites, the olivine in chondrules has begun to decompose
 from its high-temperature state, the matrix chemistry is quite
 different, especially for sulfur, and the metal has greatly changed
 in structure and composition (all compared to the much, much rarer
 type 3.00-3.01 chondrites).  Although these numbers do not tell you
 the peak metamorphic temperature, they are very useful in describing
 the various transitions that occur during metamorphic heating.

 The fact that there may be many possible combinations of chemical
 group and petrologic type is a good thing, although there certainly
 aren't 1500.  Basically, current usage is 3.00-3.04 (5 categories),
 3.05-3.15 (3 categories), 3.2-3.9 (8 catagories), 4-7 (4 categories)
 = 20 categories.  I suppose if you double this for classifiers who
 can't make up their minds, you get ~40 categories, times 3 chondrite
 groups plus 2 transitional groups = ~200 total combinations.

 Jeff

 At 11:24 PM 6/15/2008, Dark Matter wrote:
 Hi All,
 
 Twice in the past few days, I found myself staring at the screen in
 confused disbelief. The two statements in sales ads:
 
 
 a yet unclassified CO3
 
 and
 
 absolutely rare type L3.05 !
 
 just seem to me to border on absurdity. How can a unclassified
 specimen be identified by its classification?
 
 And if we carry petrological grade to the hundredths, then
 theoretically we could have over 1500 ordinary chondrite designations
 not to mention all the transitional possibilities. I fail to see how
 that level of hypothetical opinionated hair splitting could do any
 good...except for ebay sales ads that is.
 
 Just an evening though when I should be working on something else.
 
 Cheers,
 
 Martin
 __
 http://www.meteoritecentral.com
 Meteorite-list mailing list
 Meteorite-list@meteoritecentral.com
 http://six.pairlist.net/mailman/listinfo/meteorite-list

 Dr. Jeffrey N. Grossman   phone: (703) 648-6184
 US Geological Survey  fax:   (703) 648-6383
 954 National Center
 Reston, VA 20192, USA


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


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] Am I missing something here?

2008-06-16 Thread Alexander Seidel
Thank you, Jeff, for your quick reply. Seems that some type collectors will now 
feel a need to expand their meteorite inventories with the new subclasses, 
which is not an easy, or even impossible, task with almost all of those 
mentioned meteorites out of reach for a private person. So let´s hope some more 
exotic low-petrologic-type chondrites will surface in NWA or other hot deserts, 
as time goes by...

Alex
Berlin/Germany

[whose Krymka had to step down a bit from the top of the ladder (sigh!) - 
yet remains a beauty!]
 

 Original-Nachricht 
 Datum: Mon, 16 Jun 2008 10:50:53 -0400
 Von: Jeff Grossman [EMAIL PROTECTED]
 An: Alexander Seidel [EMAIL PROTECTED], 
 meteorite-list@meteoritecentral.com, [EMAIL PROTECTED]
 Betreff: Re: [meteorite-list] Am I missing something here?

 Yes.  All of the low-petrologic-type chondrites can be refined.  In 
 Grossman and Brearley (2005) we reclassified Krymka as type 3.2 and 
 Bishunpur as type 3.15.   Here is the entire set of ordinary 
 chondrite petrologic types from that paper:
 
 Semarkona -- 3.00
 QUE 97008 -- 3.05
 MET 00526 -- 3.05
 EET 90161 -- 3.05
 NWA 1756 -- 3.10
 NWA 3127 -- 3.10
 Roosevelt County 075 -- 3.10
 MET 96503 -- 3.10
 Adrar 003 -- 3.10
 Bishunpur -- 3.15
 Y-791324 -- 3.15
 Y-791558 -- 3.15
 Y-793596 -- 3.2
 Krymka -- 3.2
 GRO 95502 -- 3.2
 GRO 95544 -- 3.2
 
 
 jeff
 
 At 08:11 AM 6/16/2008, Alexander Seidel wrote:
 Hi Jeff,
 
 if this is state of the art of the classification scheme, and has 
 been accepted by a majority of the meteoriticists, does this mean 
 some important primitive meteorites finally need a refinement of 
 their established classifications?
 
 I am thinking of (e. g.) the Krymka meteorite, which to my knowledge 
 is an LL3.1. Does this have to be refined to become either an 
 LL3.05, or an LL3.10, or an LL3.15 in the end?
 
 Just curious,
 Alex
 Berlin/Germany
 
 
  Original-Nachricht 
   Datum: Mon, 16 Jun 2008 07:36:53 -0400
   Von: Jeff Grossman [EMAIL PROTECTED]
   An: Dark Matter [EMAIL PROTECTED], Meteorite List 
  meteorite-list@meteoritecentral.com
   Betreff: Re: [meteorite-list] Am I missing something here?
 
   Dear Martin and list,
  
   I can't comment on the CO3 oxymoron, but I am the inventor of the
   type 3.05 classification, so I can comment on that.
  
   As we have studied type 3 chondrites over the last 30 years,
   especially ordinary and CO chondrites, we have been gradually
   refining the 1967 Van Schmus and Wood classification scheme.  In
   1980, we realized that type 3 chondrites alone showed as great a
   range of metamorphic effects as type 4-6 did, so Sears and coworkers
   including me, proposed subdividing type 3 into types 3.0-3.9.  In
   2005, Grossman and Brearley (2005) described a similar wide range of
   metamorphic effects just between types 3.0 and 3.2 and subdivided
   this into 3.00-3.15 by steps of 0.05.  Since then, we have even begun
   to recognize different levels of metamorphic heating between types
   3.00 and 3.05, and so we find Acfer 094 at type 3.00, Semarkona at
   type 3.01, ALHA77307 at type 3.03 (e.g., Bonal et al. 2007; Kimura,
   Grossman and Weisberg, 2008, MAPS in press).
  
   These differences are quite real and important.  In type 3.05
   ordinary chondrites, the olivine in chondrules has begun to decompose
   from its high-temperature state, the matrix chemistry is quite
   different, especially for sulfur, and the metal has greatly changed
   in structure and composition (all compared to the much, much rarer
   type 3.00-3.01 chondrites).  Although these numbers do not tell you
   the peak metamorphic temperature, they are very useful in describing
   the various transitions that occur during metamorphic heating.
  
   The fact that there may be many possible combinations of chemical
   group and petrologic type is a good thing, although there certainly
   aren't 1500.  Basically, current usage is 3.00-3.04 (5 categories),
   3.05-3.15 (3 categories), 3.2-3.9 (8 catagories), 4-7 (4 categories)
   = 20 categories.  I suppose if you double this for classifiers who
   can't make up their minds, you get ~40 categories, times 3 chondrite
   groups plus 2 transitional groups = ~200 total combinations.
  
   Jeff
  
   At 11:24 PM 6/15/2008, Dark Matter wrote:
   Hi All,
   
   Twice in the past few days, I found myself staring at the screen in
   confused disbelief. The two statements in sales ads:
   
   
   a yet unclassified CO3
   
   and
   
   absolutely rare type L3.05 !
   
   just seem to me to border on absurdity. How can a unclassified
   specimen be identified by its classification?
   
   And if we carry petrological grade to the hundredths, then
   theoretically we could have over 1500 ordinary chondrite designations
   not to mention all the transitional possibilities. I fail to see how
   that level of hypothetical opinionated hair splitting could do any
   good...except for ebay sales ads that is.
   
   

Re: [meteorite-list] Am I missing something here?

2008-06-16 Thread Zelimir Gabelica

Yes, thanks to Jeff for these clearings and examples for LL's.
Note that, in contrast to the Met Bull on line, in the new edition of 
Meteorites from A to Z, the LL petrological types as given by Jeff are 
correctly mantioned, except for Bishunpur, which remained LL3.1 (but 
LL1.15  in Met. Bull.).


Alex, 2 little sisters of your Krymka, a complete slice of 17.4 grams and 
another of 28.2 g will be exhibited next week-end in Ensisheim (theme: 
meteorites from Russia and Eastern Europe).


More news on Ensisheim (latest info) to follow later today.

Best to all,

Zelimir

A 17:34 16/06/2008 +0200, Alexander Seidel a écrit :
Thank you, Jeff, for your quick reply. Seems that some type collectors 
will now feel a need to expand their meteorite inventories with the new 
subclasses, which is not an easy, or even impossible, task with almost all 
of those mentioned meteorites out of reach for a private person. So let´s 
hope some more exotic low-petrologic-type chondrites will surface in NWA 
or other hot deserts, as time goes by...


Alex
Berlin/Germany

[whose Krymka had to step down a bit from the top of the ladder 
(sigh!) - yet remains a beauty!]



 Original-Nachricht 
 Datum: Mon, 16 Jun 2008 10:50:53 -0400
 Von: Jeff Grossman [EMAIL PROTECTED]
 An: Alexander Seidel [EMAIL PROTECTED], 
meteorite-list@meteoritecentral.com, [EMAIL PROTECTED]

 Betreff: Re: [meteorite-list] Am I missing something here?

 Yes.  All of the low-petrologic-type chondrites can be refined.  In
 Grossman and Brearley (2005) we reclassified Krymka as type 3.2 and
 Bishunpur as type 3.15.   Here is the entire set of ordinary
 chondrite petrologic types from that paper:

 Semarkona -- 3.00
 QUE 97008 -- 3.05
 MET 00526 -- 3.05
 EET 90161 -- 3.05
 NWA 1756 -- 3.10
 NWA 3127 -- 3.10
 Roosevelt County 075 -- 3.10
 MET 96503 -- 3.10
 Adrar 003 -- 3.10
 Bishunpur -- 3.15
 Y-791324 -- 3.15
 Y-791558 -- 3.15
 Y-793596 -- 3.2
 Krymka -- 3.2
 GRO 95502 -- 3.2
 GRO 95544 -- 3.2


 jeff

 At 08:11 AM 6/16/2008, Alexander Seidel wrote:
 Hi Jeff,
 
 if this is state of the art of the classification scheme, and has
 been accepted by a majority of the meteoriticists, does this mean
 some important primitive meteorites finally need a refinement of
 their established classifications?
 
 I am thinking of (e. g.) the Krymka meteorite, which to my knowledge
 is an LL3.1. Does this have to be refined to become either an
 LL3.05, or an LL3.10, or an LL3.15 in the end?
 
 Just curious,
 Alex
 Berlin/Germany
 


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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[meteorite-list] The Times archives

2008-06-16 Thread Pelé Pierre-Marie
Hello,

I just learned that the british newspaper Times had
put all of its archives online, for free.

You can browse and consult any single issue of this
newspaper from 1785 to 1985.

I typed meteorite in the search engine and found 551
results.

Maybe a good way to get information about well known
worldwide falls, british falls and potential new finds
to do ?

The link is http://archive.timesonline.co.uk

Pierre-Marie Pele
www.meteor-center.com
www.encyclopedia-of-meteorites.com


  
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Envoyez avec Yahoo! Mail. Une boite mail plus intelligente http://mail.yahoo.fr

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Re: [meteorite-list] The Times archives

2008-06-16 Thread Darren Garrison
On Mon, 16 Jun 2008 20:06:42 +0200 (CEST), you wrote:

I typed meteorite in the search engine and found 551
results.

aerolite gives 235 results:

http://archive.timesonline.co.uk/tol/keywordsearch.arc
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Re: [meteorite-list] Happy 10th Birthday Portales Valley

2008-06-16 Thread mckinney trammell
me  dave etched a totally bitchin', 70% metal,  pv completeslice , 
fusion-crusted yesterday- turned out beautiful!


--- On Sat, 6/14/08, Dark Matter [EMAIL PROTECTED] wrote:

 From: Dark Matter [EMAIL PROTECTED]
 Subject: Re: [meteorite-list] Happy 10th Birthday Portales Valley
 To: [EMAIL PROTECTED]
 Cc: Meteorite-list@meteoritecentral.com
 Date: Saturday, June 14, 2008, 9:13 PM
 Sorry, forgot the link:
 
 http://www.meteorite-times.com/Back_Links/2006/September/Micro_Visions.htm
 
 happy viewing.
 
 
 
 
 On Sat, Jun 14, 2008 at 7:12 PM, Dark Matter
 [EMAIL PROTECTED] wrote:
  Hi Bernd and All,
 
  For a close up view of PV, check out Tom's Micro
 Visions article on
  it. I suspect that piece might be the PV with the
 finest polish in the
  world.
 
  Thanks Tom!
 
  -Martin
 
 
 
  On Sat, Jun 14, 2008 at 9:55 PM, 
 [EMAIL PROTECTED] wrote:
  Mike Farmer writes:
 
  I found one stone, and bought many more for
 a total of more than 15 kilos.
 
  and: Happy Birthday to one of my favorite
 meteorites
 
 
  A very enthusiastic Mike Farmer sent me this mail
 on Wed, 22 Jul 1998:
 
  Bernd, I just returned from the UofA where
 most of the analysis is being done.
   They loved this piece. It is quite obvious that
 this chondrite was smashed in
   a huge shock event and metal flowed into the
 stone crushed pieces. I wish they
   were all this nice! I had to pay over $...*/ gram
 for this slice and I will try
   to get another since it is so incredible.
 
  * amount canceled by me because I don't know
 if Mike wants to keep this private
 
  Best wishes from the happy owner of  an 11.5-gram
 metal-poor slice (M. Farmer),
  a 3.9-gram metal-rich slice (M. Blood) and a PV
 thin section (M. Farmer),
 
  Bernd
 
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Re: [meteorite-list] The Times archives

2008-06-16 Thread Mark Grossman
This is a terrific development.

The Times normally sells its database to libraries, and it is certainly not
for free!  Many libraries in the NYC area even have a restriction that the
Times database must be used on site at the library to keep the cost down,
unlike other library databases maintained by the libraries that can be
accessed at home, so long as one has a library card.

I took a quick look, and it seems that the free part is only an introductory
offer.  Still, if the price is reasonable, it is a great resource, and sure
beats traveling into the City to use the database on site at a public
library.

Will be interesting to see how this develops.  Perhaps the Times realizes
there is more money to be made by selling the archives over the internet,
rather than focusing on library sales.

In any event, thanks so much for the information that this resource is now
available for free on line - at least for the time being!

Mark Grossman


- Original Message - 
From: Pelé Pierre-Marie [EMAIL PROTECTED]
To: MeteoriteList meteorite-list@meteoritecentral.com
Sent: Monday, June 16, 2008 2:06 PM
Subject: [meteorite-list] The Times archives


 Hello,

 I just learned that the british newspaper Times had
 put all of its archives online, for free.

 You can browse and consult any single issue of this
 newspaper from 1785 to 1985.

 I typed meteorite in the search engine and found 551
 results.

 Maybe a good way to get information about well known
 worldwide falls, british falls and potential new finds
 to do ?

 The link is http://archive.timesonline.co.uk

 Pierre-Marie Pele
 www.meteor-center.com
 www.encyclopedia-of-meteorites.com




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[meteorite-list] Hot new vacation spots

2008-06-16 Thread Darren Garrison
Anyone want to calculate the surface temps for these puppies?

http://esciencenews.com/articles/2008/06/16/a.trio.super.earths

A trio of super-Earths
Published: Monday, June 16, 2008 - 09:15 in Astronomy  Space 


Today, at an international conference, a team of European astronomers announced
a remarkable breakthrough in the field of extra-solar planets. Using the HARPS
instrument at the ESO La Silla Observatory, they have found a triple system of
super-Earths around the star HD 40307. Looking at their entire sample studied
with HARPS, the astronomers count a total of 45 candidate planets with a mass
below 30 Earth masses and an orbital period shorter than 50 days. This implies
that one solar-like star out of three harbours such planets. Does every single
star harbour planets and, if yes, how many? wonders planet hunter Michel Mayor
from Geneva Observatory. We may not yet know the answer but we are making huge
progress towards it.

Since the discovery in 1995 of a planet around the star 51 Pegasi by Mayor and
Didier Queloz, more than 270 exoplanets have been found, mostly around
solar-like stars. Most of these planets are giants, such as Jupiter or Saturn,
and current statistics show that about 1 out of 14 stars harbours this kind of
planet.

With the advent of much more precise instruments such as the HARPS spectrograph
on ESO's 3.6-m telescope at La Silla, we can now discover smaller planets, with
masses between 2 and 10 times the Earth's mass, says Stéphane Udry, one of
Mayor's colleagues. Such planets are called super-Earths, as they are more
massive than the Earth but less massive than Uranus and Neptune (about 15 Earth
masses).

The group of astronomers have now discovered a system of three super-Earths
around a rather normal star, which is slightly less massive than our Sun, and is
located 42 light-years away towards the southern Doradus and Pictor
constellations.

We have made very precise measurements of the velocity of the star HD 40307
over the last five years, which clearly reveal the presence of three planets,
says Mayor.

The planets, having 4.2, 6.7, and 9.4 times the mass of the Earth, orbit the
star with periods of 4.3, 9.6, and 20.4 days, respectively.

The perturbations induced by the planets are really tiny - the mass of the
smallest planets is one hundred thousand times smaller than that of the star -
and only the high sensitivity of HARPS made it possible to detect them, says
co-author François Bouchy, from the Institut d'Astrophysique de Paris, France.

Indeed, each planet induces a motion of the star of only a few metres per
second.

At the same conference, the team of astronomers announced the discovery of two
other planetary systems, also with the HARPS spectrograph. In one, a super-Earth
(7.5 Earth masses) orbits the star HD 181433 in 9.5 days. This star also hosts a
Jupiter-like planet with a period close to 3 years. The second system contains a
22 Earth-mass planet having a period of 4 days and a Saturn-like planet with a
3-year period as well.

Clearly these planets are only the tip of the iceberg, says Mayor. The
analysis of all the stars studied with HARPS shows that about one third of all
solar-like stars have either super-Earth or Neptune-like planets with orbital
periods shorter than 50 days.

A planet in a tight, short-period orbit is indeed easier to find than one in a
wide, long-period orbit.

It is most probable that there are many other planets present: not only
super-Earth and Neptune-like planets with longer periods, but also Earth-like
planets that we cannot detect yet. Add to it the Jupiter-like planets already
known, and you may well arrive at the conclusion that planets are ubiquitous,
concludes Udry.


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[meteorite-list] Crater in Portugal ?

2008-06-16 Thread Thomas Kurtz
Hello list,

in the Earth Impact Database I can not find this structure, which is about 20km 
in diameter and located in Morais Macedo de Cavaleiros, Portugal

Google satellite map :
http://images.google.de/imgres?imgurl=http://lh3.ggpht.com/_ojJ5jSqmKP4/R124tZfg-vI/BQw/Vh83Xqry1kg/La%2BMancha.JPGimgrefurl=http://picasaweb.google.com/lh/photo/Bl2frv3O6R3s9lNq047TtAh=600w=800sz=46hl=destart=25um=1tbnid=mkVaT3kxnskm4M:tbnh=107tbnw=143prev=/images%3Fq%3DEspana%2B%252B%2522la%2Bmancha%2522%26start%3D18%26ndsp%3D18%26um%3D1%26hl%3Dde%26sa%3DN

Does anybody know anything about the origin of this round structure ?

Thank you,

with best wishes from the Ries-crater in Germany.

Thomas Kurtz

PS.:

In the case anybody of you is planning to visit the famous RIES-Crater (27km) 
in this summer, just let me know. I´m living and working in this impact site 
since 2007.

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Re: [meteorite-list] Crater in Portugal ?

2008-06-16 Thread Thomas Kurtz
Sorry, the link is wrong.

Just google map for : Morais Macedo de Cavaleiros Portugaland zoom out.



 Original-Nachricht 
 Datum: Mon, 16 Jun 2008 22:48:51 +0200
 Von: Thomas Kurtz [EMAIL PROTECTED]
 An: meteorite-list@meteoritecentral.com
 Betreff: [meteorite-list] Crater in Portugal ?

 Hello list,
 
 in the Earth Impact Database I can not find this structure, which is about
 20km in diameter and located in Morais Macedo de Cavaleiros Portugal
 
 Google satellite map :
 http://images.google.de/imgres?imgurl=http://lh3.ggpht.com/_ojJ5jSqmKP4/R124tZfg-vI/BQw/Vh83Xqry1kg/La%2BMancha.JPGimgrefurl=http://picasaweb.google.com/lh/photo/Bl2frv3O6R3s9lNq047TtAh=600w=800sz=46hl=destart=25um=1tbnid=mkVaT3kxnskm4M:tbnh=107tbnw=143prev=/images%3Fq%3DEspana%2B%252B%2522la%2Bmancha%2522%26start%3D18%26ndsp%3D18%26um%3D1%26hl%3Dde%26sa%3DN
 
 Does anybody know anything about the origin of this round structure ?
 
 Thank you,
 
 with best wishes from the Ries-crater in Germany.
 
 Thomas Kurtz
 
 PS.:
 
 In the case anybody of you is planning to visit the famous RIES-Crater
 (27km) in this summer, just let me know. I´m living and working in this
 impact site since 2007.
 
 -- 
 GMX startet ShortView.de. Hier findest Du Leute mit Deinen Interessen!
 Jetzt dabei sein: http://www.shortview.de/[EMAIL PROTECTED]
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[meteorite-list] Ad - eBay auctions closing shortly

2008-06-16 Thread star-bits
Greetings all

I have afew auctions closing shortly including

tagish lakd currently around $400/gm
Mars shergottite individuals currently around $200/gm
polymict diogenite currently less than 25% of what it s sell for.
Oriented sikhote-alins
bassikounou
vigarano, carancas, allende, an LL3 and others.   See them all at

http://members.ebay.com/ws/eBayISAPI.dll?ViewUserPageuserid=katy2kary
--
Eric Olson
7682 Firethorn Dr
Fayetteville, NC 28311

http://www.star-bits.com
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[meteorite-list] Portales Valley

2008-06-16 Thread star-bits
 Portales Valley was my first hunt for a fresh fall.   Mike Farmer called 
to tell me about the fall.   I wasn't able to get away immediately, but I 
borrowed a bunch of cash and a couple days later met Mike and Jack and Devon 
Shrader in southern New Mexico and followed Mike back to the fall site.   I 
wound up sharing a hotel room with Mike and the first night there 2 locals 
showed up with a couple stones  looking for Mike.Mike graciously allowed me 
to buy one of the stones.   As I recall it was a very metal rich 212 gram stone 
purchased for $1500.   The next day Mike told me he had a buyer for the stone 
for $2500.   Since I was working with borrowed money I took the sale and over 
the years have regreted it many times.

  I never found a piece myself, but from descriptions of later finds I was 
within 50 meters of a number of pieces.   I met Skip Wilson and spent several 
hours talking with him at his house.   Mike and I got to look over the 
meteorites Skip had found over the years and through Skip, Mike and I were able 
to purchase and split what came to be known as Roosevelt County 102.   

Aside from being hot it was a very enjoyable time.   Can't wait for the next 
fall.
--
Eric Olson
7682 Firethorn Dr
Fayetteville, NC 28311

http://www.star-bits.com

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[meteorite-list] Genetic Building Blocks May Have Formed in Space (Murchison Meteorite)

2008-06-16 Thread Ron Baalke

http://space.newscientist.com/article/dn14142-genetic-building-blocks-may-have-formed-in-space.html


Genetic building blocks may have formed in space
Rachel Courtland
New Scientist
13 June 2008

Some fundamental building blocks of our genetic code might have come
from outer space, according to a controversial new meteorite study.

The study suggests that some organic compounds associated with genetic
material might have formed in a meteorite called Murchison before it
landed in Australia in 1969. The chemicals are two kinds of nucleobases,
ring-like carbon molecules that are essential for the creation of
nucleic acids like DNA and RNA.

The find might bolster claims that meteorites delivered some of the
chemicals needed to create life. It boosts the idea that the origin of
life on Earth may have had an important contribution from an
extraterrestrial object, says lead author Zita Martins, a chemist at
Imperial College London in the UK.

But it may be too early to conclude these nucleobases formed beyond the
Earth, says Sandra Pizzarello, a chemist at Arizona State University in
Tempe, US. The study raises a very interesting question that was raised
a very long time ago, but I don't think it solves it, she told New
Scientist.

No one knows how life got its start. Primitive Earth conditions might
not have been favourable
http://www.newscientist.com/article/mg12617132.600-science-chemical-clues-to-the-origin-of-life-.html
for the chemistry needed to create life's building blocks.
  
Meteorite impacts

Instead, researchers have argued that frequent bombardments by
meteorites
3.8 billion years ago - when life is suspected to have first emerged -
could have delivered the material to Earth, where it might have helped
further the development of life.

Studies of meteorites, as well as astronomical observations of
interstellar dust and gas, have turned up a number of organic compounds,
including sugars and phosphates.

But nucleobases are also needed to make a nucleic acid like DNA or RNA.
Such chemicals have been found in a number of meteorites, but no one was
sure whether they were extraterrestrial in origin or the result of
earthly contamination.

Noisy signal

To study the origins of these nucleobases, Martins and colleagues
studied the mass of organic chemicals isolated from the meteorite.

The team looked at two different isotopes of carbon in the chemicals,
which included the nucleobases uracil and xanthine. The lighter version,
carbon-12, is present on Earth in large amounts. Carbon-13 is more
common in sweeping clouds of cold, interstellar gas. Large amounts of
the stuff usually indicate the material did not form on Earth.

The ratio of carbon-13 to carbon-12 was unusually high in the two
nucleobases, leading the team to conclude the materials likely formed in
the meteorite itself rather than on Earth.

But Pizzarello says too many other chemicals were present in the samples
to clearly distinguish the carbon ratio. Analytically, it's not
convincing, Pizzarello told New Scientist.

Astrobiology - Learn more in our out-of-this-world special report
http://www.newscientistspace.com/channel/astronomy/astrobiology.

Journal reference: Earth and Planetary Science Letters
http://www.sciencedirect.com/science/journal/0012821X (vol 270, p 130)


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[meteorite-list] Stan turecki, proof of arrest for grand theft, burglery

2008-06-16 Thread Michael Farmer

I paid for a background check on Mr. Stan Turecki, and here is what I found, of 
course, tons of files, but the actual arrest and prison sentence are below.
He was in prison from Sept 1995 until November 1996, and he stole more than 
$100,000 in this case. 
People, we are dealing with a real piece of human crap here, I have got emails 
from people in Russia, France, and USA. He owes meteorite dealers and 
collectors well over $100,000. I am, compiling a list to present to the Port 
Richeypolice department. If this con-man owes you money, let me know, I am 
going to shut this guy down.
Michael Farmer



Criminal Profile

Subject Name:TURECKI, STANLEY FREDERICKDate:6/16/2008 5:29:21 PM

Nationwide criminal search for TURECKI, STANLEY FREDERICK

Subject:
Name:TURECKI, STANLEY FOffender Status:INACTIVE 
OFFENDERSex:MALERace:WHITEHeight:5'6Eye color:GREENSSN:XXX-XX-7317Date of 
Birth:08/03/1975Offenses:
Offense: 1BURG/UNNOCSTRUCT/CONVEYOffense State: FLOffense Date: 10/14/1994Case 
Number: 9504295Sentence: 1Sentence Begin Date:09/20/1995Actual 
Release:11/22/1996Admission Date:10/27/1995

Offense: 2BURG/UNNOCSTRUCT/CONVEYOffense State: FLOffense Date: 03/30/1995Case 
Number: 9504295

Offense: 3BURGLARY TOOLS-POSSESSOffense State: FLOffense Date: 10/14/1994Case 
Number: 9504295

Offense: 4GRAND THEFT O/$100,000 1STDEGOffense State: FLOffense Date: 
10/14/1994Case Number: 9504295

Offense: 5TRAFFIC IN STOLEN PROPERTYOffense State: FLOffense Date: 
10/14/1994Case Number: 9504295



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[meteorite-list] Morocco Trip

2008-06-16 Thread ensoramanda
Many thanks to all those on the list who have already helped by giving 
tips about places to see on my trip around Morocco at the beginning of 
July. Any more are always welcome. Looking forward to it.


Hope you all have a great time in Ensisheimdont think I can pull 
that in this year...will miss all the fun...was great last year...many 
thanks to Zelimir for that.


Regards,

Graham Ensor, UK
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[meteorite-list] Colorado DOW Habitat Stamp

2008-06-16 Thread Michael Murray
Since there is a big one scheduled to come down somewhere over  
Colorado in the very near future, I wanted to get this tidbit of info  
out now to all the meteorite hunters that would travel here in such  
an event.


My message has to do with the Division of Wildlife's Habitat Stamp.   
If you have purchased a Colorado hunting or fishing license this  
year, undoubtedly you were given council by the clerk selling you the  
license that you should also buy the Habitat Stamp for $5 which will  
allow you to access DOW property called State Wildlife Areas (SWA).


What is the Stamp about?  According to the DOW, All of the funds  
raised from the sale of these stamps will be used to benefit wildlife  
by acquiring or preserving habitat.


Okay, so I don't necessarily disagree with any of that and it is  
probably well known by outdoors sportsmen but  Here is something  
about this requirement to have the stamp that may not be so well  
known.  If you are NOT a hunter, or an angler but say a hiker, or  
camper, or bird watcher, or picnicker, or sightseer, or meteorite  
hunter, etc., and you are in the age group 19 to 64 years old, you  
also will need to have this stamp to access DOW property listed in  
their property directory as an SWA or State Trust Land leased by the  
DOW.   There are only a few exceptions to this rule.


SWAs are all over the place in Colorado.  Its not uncommon at all to  
head up a road into the hills around here and find a sign declaring  
you are about to enter State Wildlife Area.


The cost of the stamp to the non-hunter is $10.25 per person.  Okay  
so not so much.  Have a car filled with 5 or six people in the 19-64  
age group without the stamps and they all get cited, well then it  
could become an expensive access.  Might even cost your group equal  
to the cost of a tank of diesel for your Hummer and we all know the  
sting in that.


Okay, let the big one fall!

Mike in CO

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[meteorite-list] AD: Big Ebay Sale - 10+ Kilos Plus Special Auction

2008-06-16 Thread Eric Wichman

Hi All,

We're having a BIG sale all this week with hundreds of NWA meteorites up 
for auction. We'll be listing more auctions than ever this week and need 
to move these meteorites now. Some BIG fusion crusted pieces too!


Lots of meteorite starting at only $1.99 for 150+ grams. NWA 869, Canyon 
Diablo, Odessa, and 2 slices of NWA 2754 LL5, some NWA 4300, and 6 very 
nice pieces of NWA Mesosiderite to be listed in the next day or so. Also 
will be listing 2 very nice NWA chondrites with HUGE Protruding 
Chondrules, look for these this week. In the meantime be sure to bid on 
these auctions listed below as well.


SUPER WONDERFUL FANTABULOUSLY GORGEOUS THUMBPRINTED FUSION CRUSTED 
BEAUTY - Starting @ .99 cents

http://cgi.ebay.com/Special-3851g-Huge-NWA-XXX-CHONDRITE-METEORITE-AWESOME_W0QQitemZ250260289396

1982 Gram Large NWA XXX With Fusion Crust - Good solid piece, some 
weathering, Will Slice nicely.

http://cgi.ebay.com/1982g-HUGE-NWA-XXX-CHONDRITE-METEORITE-MOROCCO-U7-001_W0QQitemZ260250444603

1579.1 Gram Large NWA XXX with weathered crust. Nice Big Piece.
http://cgi.ebay.com/1579-1g-NWA-HUGE-XXX-CHONDRITE-METEORITE-MOROCCO_W0QQitemZ250257876571

359.8 Gram NWA XXX - Nice Thumbprints On Edges. Solid Piece Will Make 
Very Nice Polished Slices.

http://cgi.ebay.com/359-8g-NWA-XXX-CHONDRITE-METEORITE-MOROCCO-U3-070_W0QQitemZ260250165335

61.1 Gram Full Slice Of Odessa Iron - Sanded and Ready For Etch
http://cgi.ebay.com/61-1g-ODESSA-IRON-METEORITE-SLICE-CUT-SANDED-PIECE_W0QQitemZ250258567865

90.7 Gram Full Slice Of Odessa Iron - Sanded and Ready For Etch
http://cgi.ebay.com/90-7g-ODESSA-IRON-METEORITE-SLICE-CUT-SANDED-PIECE_W0QQitemZ260250832550

105.3 Gram NWA XXX WIth Cool Shape - Some Residual Crust - Displays Nicely
http://cgi.ebay.com/105-3g-NWA-XXX-CHONDRITE-METEORITE-MOROCCO-U3-071_W0QQitemZ260250164251

We've got over 120 auctions running right now in addition to our Ebay 
Store deals: http://stores.ebay.com/Little-Bits-Of-Earth


Keep an eye out for more this week.

Happy Bidding! Good Luck!

Regards,
Eric Wichman
MeteoritesUSA
MeteoriteWatch

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Re: [meteorite-list] Morocco Trip

2008-06-16 Thread Zelimir Gabelica

Thanks for your kind words Graham and for your appreciating our show
We will miss you this time.

Always feel free to come any time in future, you know that you are very 
welcome. And in 2009 it is the 10th anniversary of the show. We foresee a 
great vintage.


Good trip to Morocco. Some Morroccan dealers will be, as every year, in 
Ensisheim.
But, if you can make Ste Marie the week after, many of them will be also 
most probably there around.


At least Ali Hmani, who can give you interesting tips, has his curent tent 
in one of the main alleys of Ste Marie.


Oh yes, while you are there, don't forget to contact also some mineral 
dealers from Morocco. They are well represented at Ste Marie, easy to spot 
and they will all be happy and proud to give you tips for a trip around 
their country.


All my best wishes,

Zelimir





A 01:49 17/06/2008 +0100, ensoramanda a écrit :
Many thanks to all those on the list who have already helped by giving 
tips about places to see on my trip around Morocco at the beginning of 
July. Any more are always welcome. Looking forward to it.


Hope you all have a great time in Ensisheimdont think I can pull that 
in this year...will miss all the fun...was great last year...many thanks 
to Zelimir for that.


Regards,

Graham Ensor, UK
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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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