Other
Scientific paper
Jun 1986
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986gecoa..50.1023b&link_type=abstract
(Lunar and Planetary Institute, NASA, American Geophysical Union, et al., Lunar and Planetary Science Conference, 16th, Houston,
Other
8
Achondrites, Cosmic Rays, Meteoritic Composition, Particle Tracks, Radiation Effects, Ablation, Aluminum 26, Evolution (Development), Heavy Nuclei, Radioactivity, Shock Loads, Solar Heating, Thermoluminescence, Meteorites, Stony Meteorites, Achondrites, Shergotty, Samples, Meteorite, Shergottites, Fission Tracks, Radioactivity, Thermal History, Cosmic Rays, Antarctic Meteorites, Alh Meteorites, Alha77005, Eet Meteorites, Eeta79001, Thermoluminescence, Shock Effects, Comparisons, Procedure, Met Meteorites, L
Scientific paper
Heavy nuclei tracks, thermoluminescence (TL), and Al-26 activity have been analyzed in samples of Shergotty, ALHA 77005, and EETA 79001 achondrites with the purpose of tracing their thermal and cosmic ray exposure history. The track data indicate low (1 to 3 cm) ablation for all three shergottites, pointing to low geocentric velocities and small masses. Nuclear track, Al-26 activity, and other cosmogenic effects in the three shergottites are consistent with their single stage exposure in space as small objects. The TL data indicate a low equivalent dose (ED) of less than 30 krad at low glow curve temperature for all the shergottites. Solar heating at close perihelion distance (0.70 to 0.85 AU) might be primarily responsible for the low ED's, although shock-induced effects cannot be ruled out. The results of this study are compared with the dynamical models developed by Wetherill (1984) for the origin of shergottites.
Bhandari Narendra
Goswami Jitendra N.
Jha Rajveer
Sengupta Debasis
Shukla P. N.
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