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Exposure histories of lunar meteorites: ALHA81005, MAC88104, MAC88105, and Y791197

Conference · · Geochimica et Cosmochimica Acta; (United States)
OSTI ID:5171790
;  [1]; ; ;  [2]; ; ;  [3];  [4]
  1. Univ. of California, San Diego, (United States)
  2. Univ. of Pennsylvania, Philadelphia (United States)
  3. Univ. of Rochester, NY (United States)
  4. Los Alamos National Lab., NM (United States)
The cosmogenic radionuclides {sup 41}Ca, {sup 36}Cl, {sup 26}Al, and {sup 10}Be in the Allan Hills 81005, MacAlpine Hills 88104, MacAlpine Hills 88105,and Yamato 791197 meteorites were measured by accelerator mass spectrometry (AMS). {sup 53}Mn in Allan Hills 81005 and Yamato 791197 was measured by activation. These four lunar meteorites experienced similar histories. They were ejected from near the surface of the Moon ranging in depth down to 400 g/cm{sup 2} and had very short transition times (less than 0.1 Ma) from the Moon to the Earth. A comparison of the cosmogenic nuclide concentrations in MacAlpine Hills 88104 and MacAlpine Hills 88105 clearly indicates that they are a pair from the same fall.
OSTI ID:
5171790
Report Number(s):
CONF-9003166--
Conference Information:
Journal Name: Geochimica et Cosmochimica Acta; (United States) Journal Volume: 55:11
Country of Publication:
United States
Language:
English