T293 Preparations for the New Era of Lunar Science: Laboratory Measurements and New Insights into the Moon
Wednesday, 8 October 2008
8:00 AM - 12:00 PM
High-Fe, Low-Al Basalts: Evidence of Extensive Mantle Processing on Earth, Moon, Mars, Vesta, Venus, and Io
Paper number: T293-13
Program: Technical Sessions
Time: 11:15 AM – 11:30 AM
Authors
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Michelle KirchoffSouthwest Research Institute, Boulder, CO
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Susanne P. SchwenzerLunar and Planetary Institute, Houston, TX
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Walter S. KieferLunar and Planetary Institute, Houston, TX
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Allan TreimanLunar and Planetary Institute, Houston, TX
Abstract
High-Fe, low-Al igneous compositions have been found on the Earth, Moon, Mars, Vesta, and possibly on Venus and Io. Therefore they are not unique to one planetary body, but seem to be widespread throughout terrestrial bodies in the solar system. This suggests that similar processes could be occurring to produce these compositions on different planetary bodies. The common factor required to produce such compositions on all the planetary bodies under consideration is an extensively processed mantle source region, through a magma ocean or repeated partial melting episodes. Magma ocean models (Hofmeister, 1983) have shown that Mg-, Fe-rich minerals sink thereby producing a Mg- Fe-rich residual mantle. If these minerals were re-melted during rehomogenization, or mantle overturn, then high -Mg, -Fe, low -Al basalts could be produced. Such a model has been suggested for Mars (Debaille et al., 2007; Elkins-Tanton et al., 2003), the moon (Elkins Tanton et al., 2002; Warren, 1985), Vesta (Righter and Drake, 1997), Io (Keszthelyi and McEwen, 1997), Venus (Elkins-Tanton et al., 2007), and the Earth (Hofmeister, 1983), but now may be extrapolated to any planet that has undergone extensive mantle processing. Therefore, finding such high-Fe, low-Al compositions on other terrestrial bodies gives an indication about the extent of mantle processing.