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NWA 11228   contributed by Jonathan Ospina   MetBul Link


Roll Overs:     #1   #2   #3   #4    


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View all entries for   Meteorite (1)   Jonathan Ospina (17)


6.369 grams.   Lunar (feldsp. breccia)

TKW 140 grams. Fall not observed. Found 20 March 2017, Morocco.

 


  Click to view larger photos     #1     #2     #3     #4


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MexicoDoug
 9/19/2019 10:56:32 AM
"analyzed by Jose Garcia and confirmed as 11228" Are you saying Jose Garcia has officially paired this darker stone to NWA 11228? Based on what, that is a relevant question!
John Divelbiss
 9/19/2019 10:44:34 AM
It is OK Jon. I understood you had it looked at by someone "to be sure" it was a lunar, and also that it was darker than most you've seen...you never mentioned FC. Ignore those comments is my recommendation. The meteorite police really don't exist...
Jonathan Ospina
 9/18/2019 10:00:41 PM
In my comment he mentioned: * is a *fragment* analyzed by Jose Garcia in the Canarian Museum / I never said that Jose Garcia was the one who analyzed the 11228 meteorite and reported it to MBD * with a very *dark surface*, more than normal / I never said: It is a surface with Fusion Crust
Jonathan Ospina
 9/18/2019 9:48:54 PM
Hello Anne Black, what I meant that this particular piece was analyzed by Jose Garcia and confirmed as 11228, I did not mean that Jose was the one who generated the report to MBD, and on the point I mentioned about its surface being darker I was not referring to Fusion Crust, I was referring to its dark hue unlike the others
Alfredo Petrov
 9/18/2019 2:24:38 PM
I wonder whether that rectangular protrusion is actually an anorthite crystal?
Anne Black
 9/18/2019 12:45:02 PM
Jonathan, according to the Met. Bulletin, it was classified by Carl Agee, of the University of New Mexico. And it is not fusion crust, it is desert varnish! Physical characteristics: Many irregular shaped fragments, dark sand-blasted exterior, no fusion crust. Petrography: (C. Agee, UNM) This meteorite is a fragmental breccia with pyroxene, plagioclase, and olivine grains set in fine grained groundmass. Scattered micro-gabbro fragments were also observed. Ubiquitous, fine grained, accessory Fe-metal and sulfide are present. Minor amount of shock melt was observed in the microprobe section. All pyroxene grains probed were pigeonite, no augite was detected.
Jonathan Ospina
 9/18/2019 11:41:56 AM
Thanks Ben Fisler and Bernd Pauli, It is a fragment analyzed by Jose Garcia in the Canarian Museum, and its shape is incredible, with a very dark surface, more than normal, so I bought it immediately :)
Bernd Pauli
 9/18/2019 11:10:08 AM
... and interesting shape!
Ben Fisler
 9/18/2019 10:32:58 AM
Jonathan, beautiful lunar. Thanks.
 

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