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Interstellar cloud material: contribution to planetary atmospheres.

D M Butler, M J Newman, R J Talbot

    Science (New York, N.Y.)
    |August 11, 1978
    PubMed
    Summary
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    The solar system has passed through dense interstellar clouds, potentially adding significant amounts of isotopes like neon to planets. Earth

    Area of Science:

    • Planetary Science
    • Astrophysics
    • Astrochemistry

    Background:

    • Interstellar clouds are vast regions of gas and dust in space.
    • The composition of interstellar clouds can vary significantly.

    Purpose of the Study:

    • To investigate the potential impact of dense interstellar cloud encounters on planetary atmospheres.
    • To determine if these encounters can explain observed isotopic abundances.

    Main Methods:

    • Statistical analysis of interstellar cloud properties.
    • Modeling the accumulation of isotopes during cloud passage.

    Main Results:

    • The solar system has encountered at least a dozen dense interstellar clouds.
    • Neon accumulation is most pronounced, with potential to explain Earth's atmospheric neon.

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  • Predicted neon addition to Mars far exceeds its current abundance.
  • Conclusions:

    • Interstellar cloud encounters are a plausible mechanism for significant isotopic additions to planets.
    • This mechanism may be crucial for understanding the atmospheric evolution of terrestrial planets.