We have examined the relationship between natural thermoluminescence (TL) and ~(26)Al in 120 Antarctic meteorites in order to explore the orbital history and terrestrial ages of these meteorites. Our results confirm the observations of Hasan et al. (1987) which were based on 23 meteorites. For most meteorites there was a positive correlation between natural TL and ~(26)Al, reflecting their similarity in decay rate under Antarctic conditions and thus in terrestrial age. For a small group with low TL and high ~(26)Al a small perihelion was proposed. Within this group, natural TL decreases with terrestrial age as determined by ~(36)Cl measurements, although the rate of TL decay is faster (half-life approximately 10ka) and the ages that can be determined are smaller (<200ka) than for most meteorites. The faster decay rate and lower natural TL levels are a reflection of recent exposure to higher radiation doses and higher temperatures, since this history would populate less stable TL traps with smaller electron densities. We sort the 120 meteorites by perihelion and terrestrial age. The normal perihelion group range up to approximately 1000ka and the small perihelion group range up to approximately 200ka. An intermediate perihelion group tends to have short terrestrial ages (20-60ka). There is acceptable agreement between most (34 out of 43) of our present terrestrial age estimates and those determined by isotopic means, the exceptions reflecting complex irradiation histories, long burial times in the Antarctic, or other issues.
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