Abstract
VIKING 1 and 2 have collected various data on the amount and composition of the martian atmosphere. The isotopic ratios 15N/14N, 40Ar/36Ar and 129Xe/132Xe have been found to be distinctly different from the terrestrial values1–3. We propose here that the enrichment of 15N amounting to 62% (ref. 4) may be caused by nuclear reactions with intense cosmic rays in the early Solar System. The implications of the ratios 40Ar/36Ar and 129Xe/132Xe are different from that of 15N/14N, because although 40Ar and 129Xe have a long-lived radioactive parent nuclide, 15N does not. These two isotopic ratios may be the results of the initial endowment of the relevant elements, the degree of outgassing from the interior and recondensation or trapping in the surface region.
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YANAGITA, S., IMAMURA, M. Excess 15N in the martian atmosphere and cosmic rays in the early Solar System. Nature 274, 234–235 (1978). https://doi.org/10.1038/274234a0
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DOI: https://doi.org/10.1038/274234a0
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