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Noble Gases in Terrestrial Planets: Evidence for Cometary Impacts?

  • Tobias Owen
  • Akiva Bar-Nun
  • Idit Kleinfeld
Part of the Astrophysics and Space Science Library book series (ASSL, volume 167)

Abstract

The possible role of comets in bringing volatiles to the inner planets is investigated by means of laboratory studies of the ability of ice to trap gases at low temperatures. The pattern of the heavy noble gases formed in the atmosphere of Venus can be explained by the impact of a planetesimal composed of ices formed in the range of 20 to 30 K. The noble gas patterns on Mars and Earth are less explicable by cometary bombardment alone.

Keywords

Solar Wind Enrichment Factor Terrestrial Planet Solar Nebula Lunar Soil 
These keywords were added by machine and not by the authors. This process is experimental and the keywords may be updated as the learning algorithm improves.

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Copyright information

© Springer Science+Business Media Dordrecht 1991

Authors and Affiliations

  • Tobias Owen
    • 1
  • Akiva Bar-Nun
    • 2
  • Idit Kleinfeld
    • 2
  1. 1.Institute for AstronomyUniversity of HawaiiHonoluluUSA
  2. 2.Department of Geophysics and Planetary SciencesTel Aviv UniversityTel AvivIsrael

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