Venus Was Wet: A Measurement of the Ratio of Deuterium to Hydrogen

@article{Donahue1982VenusWW,
  title={Venus Was Wet: A Measurement of the Ratio of Deuterium to Hydrogen},
  author={T. Donahue and J. Hoffman and R. Hodges and A. J. Watson},
  journal={Science},
  year={1982},
  volume={216},
  pages={630 - 633}
}
  • T. Donahue, J. Hoffman, +1 author A. J. Watson
  • Published 1982
  • Medicine, Chemistry
  • Science
  • The deuterium-hydrogen abundance ratio in the Venus atmosphere was measured while the inlets to the Pioneer Venus large probe mass spectrometer were coated with sulfuric acid from Venus' clouds. The ratio is (1.6 � 0.2) x 10–2. The hundredfold enrichment of deuterium means that at least 0.3 percent of a terrestrial ocean was outgassed on Venus, but is consistent with a much greater production. 

    Topics from this paper.

    Atmospheric and water loss from early Venus
    102
    Composition of the atmosphere of Venus below the clouds
    43
    Solar System Deuterium/Hydrogen Ratio
    43
    The Surface and Atmosphere of Venus: Evolution and Present State
    2
    The origin of inner Solar System water
    20

    References

    Publications referenced by this paper.
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    Lohmann for useful comments
      show that the present escape modes on Venus would imply a lower limit of 800 g cm-2 of H20 on Venus 4.5 billion years ago. Escape of deuterium is negligible
      • 1982