[meteorite-list] Mercurian Meteorites (was: Rocks from Space Picture of the Day - June 16, 2010)
From: bernd.pauli at paulinet.de <bernd.pauli_at_meteoritecentral.com>
Date: 18 Jun 2010 16:47:09 UT Message-ID: <DIIE.0000000A00004CC5_at_paulinet.de> Greg S. inquired: "I heard that possible meteorites from Mercury should contain very little (or no) free iron. Is this true? I think the one pictured here and NWA 2999 do contain some free iron." Hello Greg and List, I thought this summary of the "Summary and Conclusions" part of Love's article might be of interest because it partly answers your question about Mercury's iron: Summary: - orbital evolution of Mercurian material to Earth-crossing orbits possible - efficiency probably < 1% of that computed for Mars - a ~ 10% chance that a mercurian rock could exist in current meteorite collections - may possess an unusual isotopic composition - rocks from Mercury probably low in volatiles - Mercury bulk composition moderately enriched in refractory oxides of Al, Ti, and Ca - FeO contents not more than ~ 5%, and possibly much lower - Mercurian regolith breccias: - rich in micrometeorite craters - rich in exogenic chondritic materials - rich in agglutinates - rich in impact vapor deposits - lower solar-wind content than similar lunar soils - implanted gas may be fractionated by interaction with Mercury's global magnetic field - a uniquely high solar-to-galactic cosmic-ray damage track ratio of surfac rocks - launch-induced shock damage may be comparable to or greater than in martian meteorites - no match of these predicted properties of mercurian rocks in current meteorite groups - misclassified mercurian meteorites most likely differentiated, low-FeO objects such as lunar anorthosites and aubrites Reference: LOVE S.G. et al. (1995) Recognizing mercurian meteorites (MAPS 30-3, 1995, 269-278). ......................................................................................... There are some scientists who favor enstatite chondrites but there's a problem with that: Mercury's mean density is about 5.4 g/cm^3, whereas enstatite chondrites have a density of about 3.4-3.7 g/cm^3. In 2002, H. Palme proposed that NWA 011 (and paired material like NWA 4587) might be a fragment of Mercury but the high FeO content of this meteorite would point toward a parent body with a small metallic iron core. Mercury, however, is believed to have a large iron core. Best wishes, Bernd Received on Fri 18 Jun 2010 12:47:09 PM PDT |
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