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The relevance of the IUE results on young stars for Earth's paleoatmosphereUsing the latest IUE results for seven T Tauri stars, which are believed to represent the young Sun and a detailed photochemical chemical model of the paleoatmosphere, the vertical distribution of Oxygen and Ozone in the early atmosphere was calculated. The calculations indicate that the surface Oxygen mixing ratio is as much as six orders of magnitude larger than previously estimated, but appears low enough for the formation of amino acids via the Urey-Miller type of experiments. It is believed that the quantification of the oxygen level in the Earth's paleoatmosphere presented can reconcile the demands of both biological and geological considerations.
Document ID
19820023330
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Canuto, V. M.
(NASA Goddard Inst. for Space Studies New York, NY, United States)
Levine, J. S.
(NASA Langley Research Center Silver Spring, Md., United States)
Augustsson, T. R.
(NASA Langley Research Center)
Imhoff, C. L.
(Computer Sciences Corp.)
Giampap, M. S.
(Harvard-Smithsonian Center for Astrophysics)
Date Acquired
August 10, 2013
Publication Date
January 1, 1982
Publication Information
Publication: NASA. Goddard Space Flight Center Advan. in Ultraviolet Astron.
Subject Category
Astronomy
Accession Number
82N31206
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.

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