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Found during the 2004 U.S. Antarctic Search for
Meteorites season, LAP 04841 represents an addition to the
LaPaz lunar basalts suite, and brings the total mass
collected to 1.93 kg. Mineral modes and chemistries, as well
as trace-element patterns, provide evidence for pairing of
this meteorite to others in the suite. Analyses of chromite
grains provide a V/(Al+Cr) ratio of 1.33 ± 13,
translating to an fO2 one log unit below the IW buffer, in
accordance with previous fO2 estimates. Pyroxene and olivine
Mn/Fe values plot along the trend set for lunar basalts. The
presence of FeNi grains, troilite, and the anorthositic
composition of plagioclase are further evidence for the
lunar origin of this meteorite. Application of the
Zr-cooling speedometer, for ilmenite and ulvöspinel
pairs, give a cooling rate of 5.2°C/day. Study of the
impact-shock deformation of LAP 04841 reveals a considerable
range of impact stress may be encountered within a few
millimeters, suggesting complex controls on pressure
dissipation throughout the meteorite.
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