Adam Hupe wrote:

> I am betting that NWA 998 has a different ejection date
> and crystallization age than the other five Nakhlites.
> The isotope data is proving to be very interesting and
> was announced at the 65th Meteoritical Society meeting.


... and pre-atmospheric sizes of martian meteorites:

a) The authors estimate the minimum masses of the martian
   meteoroids to have been in the range of 150�220 kg.

b) The 36Cl concentration in Los Angeles is consistent with
   a meteoroid radius of 20�40 cm.

c) The 10Be, 26Al, and 36Cl activities in QUE 94201 indicate a      
   pre-atmospheric radius of 25�40 cm.

d) For Shergotty, Bhandari et al. (1986) obtained from the 26Al      
   concentration an effective radius of ~12 cm of the meteoroid,
   about half the value of 23 cm calculated by Eugster et al.

e) Density of the shergottites, Nakhla, and Chassigny is about
   3.23, 3.37, and 3.72 g/cm3.

f) Model calculations of the upper limit of the radius of
   fragments ejected from Mars yield radii of <2 m.


Don�t these data ring a bell? The next step for meteoriticists
(and several people on our List) could be to compare the existing/
recovered masses - especially of documented falls, of course, like
Shergotty, Chassigny, Zagami, and Naklha (Watch out, the Nakhla Dog
is back in town :-) - to these minimum pre-atmospheric sizes and
thus masses. (Model) calculations involving the physics of the falls
(heating and ablation, velocity, deceleration, entry angle, strewn
field geometry, etc., etc.) might then give us a clue as to if
there is still more recoverable material out there. In the case of
Shergotty and Chassigny, most if any at all, may have weathered away
in the meantime, but Zagami and Nakhla ... Well, we all know that up
to 90 % of a meteorite�s mass is lost to ablation which would be close
to Zagami�s total recovered mass of about 18.1 kg (well within the 150 -
220 kg interval mentioned by Eugster et al. - 10% => 15-22 kg) but
remember the authors say they are minimum masses!

If only the discrepancy between the upper limit and
the lower limit of the radii wasn�t so huge :-(


Best martian
regards,

Bernd


Reference

EUGSTER O. et al. (2002) Ejection ages from 81Kr-83Kr
dating and pre-atmospheric sizes of martian meteorites
(MAPS 37-10, 2002, 1345-1360)

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