[meteorite-list] Glassface found the 33rd Mars Rock

From: Sharkkb8_at_aol.com <Sharkkb8_at_meteoritecentral.com>
Date: Thu Apr 22 10:31:25 2004
Message-ID: <1c0.156b618c.2d6a8853_at_aol.com>

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 mlblood_at_cox.net writes:
I don't get it, you guys.... not misleading unless you don't read.....I don'=
t=20
get it... =20
I don't get YOU, Michael ;-) - where here do you read that he's NOT=20
selling this stuff as Martian? (You sure you're not just re-reading John D=
.'s=20
retaliatory fake-Martian-auction spoof?!)


NWA Mars Basaltic Achondrite just got here !=20


"This stone was purchased in Rissani, Morocco, november 2002. Trapped melt=20
inclusions in olivine contain Al-pigeonite, Al-diopside, pleonaste and glass=
.=20
Large opx phenocrysts show preferred orientation; olivine phenocrysts are we=
akly=20
oriented and tend to occur in clusters. The stone has a 1=E2=80=932 mm weath=
ering=20
rind; interior is very fresh. The nomade that sold it to me said he saw it w=
hile=20
walking through the desert. Twelve unusual meteorites are almost certainly=20
pieces of Mars that were blasted off the red planet by meteoroid impact. The=
y=20
have been called SNC meteorites after the three type samples, Shergotty, Nak=
hla,=20
and Chassigny, or now simply martian meteorites. All twelve meteorites are=20
igneous rocks crystallized from lava in the crust of a parent body. They are=
,=20
however, distinct from typical igneous meteorites from asteroids in ways tha=
t=20
suggest that the SNC meteorites come from a much larger body, a planet. All=20=
but=20
one of these meteorites are very young (1.3 Ga or less) compared to ancient=20
ages for other igneous meteorites (about 4.5 Ga). They also have higher oxyg=
en=20
fugacities and contents of water and other volatiles, contain minerals with=20
ferric iron, and form a distinct trend in oxygen isotopic composition. The=20
conclusive evidence that SNC meteorites are from Mars is the analysis of gas=
es=20
trapped in glass inclusions in EETA79001, which chemically and isotopically=20=
match=20
gases measured in the unique martian atmosphere by the Viking lander spacecr=
aft=20
desert early morning. "

Gregory

J. Gregory Wilson
2118 Wilshire Blvd. #918
Santa Monica, CA 90403

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<DIV>
<DIV>
<DIV>&nbsp;<A title=3Dmailto:mlblood_at_cox.net href=3D"mailto:mlblood@cox.net"=
>mlblood_at_cox.net</A> writes:</DIV>
<BLOCKQUOTE style=3D"PADDING-LEFT: 5px; MARGIN-LEFT: 5px; BORDER-LEFT: blue=20=
2px solid"><FONT face=3DArial>I don't get it, you guys.... not misleading un=
less you don't read.....I don't get it...&nbsp; </FONT></BLOCKQUOTE></DIV>
<DIV>I don't get YOU, Michael&nbsp; ;-)&nbsp;&nbsp; &nbsp; -&nbsp; where her=
e do you read that he's NOT selling&nbsp;this stuff&nbsp;as Martian?&nbsp;&n=
bsp; (You sure you're not just re-reading John D.'s retaliatory fake-Martian=
-auction spoof?!)</DIV>
<DIV>&nbsp;</DIV>
<DIV>&nbsp;</DIV>
<DIV>
<TABLE cellSpacing=3D0 cellPadding=3D0 width=3D"100%" border=3D0>
<TBODY>
<TR bgColor=3D#d6dcfe>
<TD><IMG title=3D"" height=3D1 alt=3D"" src=3D"http://pics.ebaystatic.com/aw=
/pics/x.gif" width=3D6></TD>
<TD width=3D"100%"><FONT face=3DArial size=3D4><B>NWA Mars Basaltic Achondri=
te just got here !</B></FONT> </TD></TR></TBODY></TABLE></DIV>
<DIV>&nbsp;</DIV>
<DIV>"This stone was purchased in Rissani, Morocco, november 2002. Trapped m=
elt inclusions in olivine contain Al-pigeonite, Al-diopside, pleonaste and g=
lass. Large opx phenocrysts show preferred orientation; olivine phenocrysts=20=
are weakly oriented and tend to occur in clusters. The stone has a 1=E2=80=
=932 mm weathering rind; interior is very fresh. The nomade that sold it to=20=
me said he saw it while walking through the desert. Twelve unusual meteorite=
s are almost certainly pieces of Mars that were blasted off the red planet b=
y meteoroid impact. They have been called SNC meteorites after the three typ=
e samples, Shergotty, Nakhla, and Chassigny, or now simply martian meteorite=
s. All twelve meteorites are igneous rocks crystallized from lava in the cru=
st of a parent body. They are, however, distinct from typical igneous meteor=
ites from asteroids in ways that suggest that the SNC meteorites come from a=
 much larger body, a planet. All but one of these meteorites are very young=20=
(1.3 Ga or less) compared to ancient ages for other igneous meteorites (abou=
t 4.5 Ga). They also have higher oxygen fugacities and contents of water and=
 other volatiles, contain minerals with ferric iron, and form a distinct tre=
nd in oxygen isotopic composition. The conclusive evidence that SNC meteorit=
es are from Mars is the analysis of gases trapped in glass inclusions in EET=
A79001, which chemically and isotopically match gases measured in the unique=
 martian atmosphere by the Viking lander spacecraft desert early morning. "<=
!-- End Description --></DIV></DIV>
<DIV>&nbsp;</DIV>
<DIV><FONT lang=3D0 face=3DArial size=3D2 FAMILY=3D"SANSSERIF" PTSIZE=3D"10"=
></FONT><FONT lang=3D0 face=3DArial color=3D#ff0000 size=3D3 FAMILY=3D"SANSS=
ERIF" PTSIZE=3D"12"></FONT><FONT lang=3D0 face=3D"Comic Sans MS" color=3D#ff=
0000 size=3D3 FAMILY=3D"SCRIPT" PTSIZE=3D"12">Gregory</FONT><FONT lang=3D0 f=
ace=3DArial color=3D#000000 size=3D2 FAMILY=3D"SANSSERIF" PTSIZE=3D"10"><BR>=
<BR>J. Gregory Wilson<BR>2118 Wilshire Blvd. #918<BR>Santa Monica, CA 90403<=
/FONT></DIV></BODY></HTML>

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Received on Sun 22 Feb 2004 05:33:55 PM PST


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