Abstract
An analysis of the distribution of 3He and 4He in L and H chondrites has shown that the parent body of L chondrites underwent a catastrophic collision in space 340 ± 50 Ma ago. This age differs considerably from the collision age of 520 ± 60 Ma given previously (Heymann, 1967). The parent body of H chondrites may also have undergone local heating and degassing ∼200 Ma ago. Data for L chondrites argue in favour of Antarctic and non-Antarctic meteorites having originated from a common parent body.
Cite
CITATION STYLE
Alexeev, V. A. (1998). Parent bodies of L and H chondrites: Times of catastrophic events. Meteoritics and Planetary Science, 33(1), 145–152. https://doi.org/10.1111/j.1945-5100.1998.tb01616.x
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