[meteorite-list] Mercurian Meteorites
From: Bernd Pauli HD <bernd.pauli_at_meteoritecentral.com>
Date: Thu Apr 22 09:50:29 2004 Message-ID: <3CC4345F.1CBF1FB9_at_lehrer1.rz.uni-karlsruhe.de> Martin Horejsi wrote: > I believe that Stanley Love did some work in this area. > Maybe someone out there has some references handy. and: > enstatite-rich achondrites were the best candidates > at the moment. In specific, the aubrites. Here's one: LOVE S.G. et al. (1995) Recognizing mercurian meteorites (MAPS 30-3, 1995, 269-278): "The groups in which a misclassified mercurian meteorite would be most likely to lurk are differentiated, low-FeO objects such as the lunar anorthosites and the aubrites. Future searches for mercurian meteorites should focus on similar objects." Excerpts from the March issue of MAPS: - the Sun is up to 11 x more intense than on Earth - the sunlit side of the planet heats up to over 400°C - specific gravity of 5.44 as compared to the Moon's 3.34 - Mercury has the highest metal/silicate ratio and the Moon the lowest - Rocks on Mercury are generally Fe-poor, and therefore light-colored - ~3 wt% FeO is the most reasonable value for the crust of Mercury - presence of a magnetic field (strength of ~1% of the Earth's field is just enough to indicate the existence of a core dynamo) - current models suggest that the evolution of a planetary dynamo requires the presence of a solid inner core and a liquid outer core - discovery of material of high radar reflectivity near the poles is interpreted as ice, possibly mantled by dust. >From the Editors, Mercury 2001 conference, Field Museum, Chicago, Illinois, 2001 October 4-5 [MAPS 37, 307-309 (2002)] Cheers, Bernd Received on Mon 22 Apr 2002 12:03:43 PM PDT |
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