We suggest that impacts by icy planetesimals during the first billion years of solar system history played a major role in the origin of planetary atmospheres. In the outer solar system, the effect of these planetesimals is evident in the super‐solar values of C/H and the variations of D/H in giant planet atmospheres. Laboratory experiments on the trapping of noble gases in ice forming at various temperatures provide an illuminating interpretation of noble gas abundances in the atmospheres of the inner planets, again implicating icy planetesimals. This model can be tested by searching for noble gases in comets, by investigating abundances and isotopic ratios in Jupiter’s atmosphere, and by further studies of the SNC meteorites and the atmospheres of the inner planets.
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25 July 1995
Volatiles in the Earth and solar system
Sep 1994
Pasadena, California (USA)
Research Article|
July 25 1995
Comets, impacts and atmospheres II. Isotopes and noble gases Available to Purchase
Tobias Owen;
Tobias Owen
University of Hawaii, Honolulu, Hawaii 96822
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Akiva Bar‐Nun
Akiva Bar‐Nun
Tel‐Aviv University, Tel‐Aviv, Israel
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Tobias Owen
Akiva Bar‐Nun
University of Hawaii, Honolulu, Hawaii 96822
AIP Conf. Proc. 341, 123–138 (1995)
Citation
Tobias Owen, Akiva Bar‐Nun; Comets, impacts and atmospheres II. Isotopes and noble gases. AIP Conf. Proc. 25 July 1995; 341 (1): 123–138. https://doi.org/10.1063/1.48736
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