Stability of ammonia in the primitive terrestrial atmosphere

書誌事項

公開日
1982-04-20
権利情報
  • http://onlinelibrary.wiley.com/termsAndConditions#vor
DOI
  • 10.1029/jc087ic04p03091
公開者
American Geophysical Union (AGU)

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説明

<jats:p>A one‐dimensional photochemical model is used to calculate the rate at which ammonia would have been destroyed in the earth's atmosphere for assumed NH<jats:sub>3</jats:sub> mixing ratios of 10<jats:sup>−8</jats:sup> to 10<jats:sup>−4</jats:sup>. The calculated NH<jats:sub>3</jats:sub> destruction rates are then compared with possible abiotic and biotic sources for ammonia. Abiotic sources were probably sufficient to maintain the NH<jats:sub>3</jats:sub> mixing ratio of 10<jats:sup>−8</jats:sup> needed for life to have evolved but were too small to sustain the mixing ratios of 10<jats:sup>−5</jats:sup> or more necessary to produce significant greenhouse warming. The atmospheric ammonia concentration may have increased during the Archean as a result of biological activities but probably remained below the level required to generate measurable thermal effects.</jats:p>

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