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Observation of a mass independent oxygen isotopic composition in terrestrial stratospheric CO 2 , the link to ozone chemistry, and the possible occurrence in the Martian atmosphere
Author(s) -
Thiemens Mark H.,
Jackson Teresa L.,
Brenninkmeijer Carl A. M.
Publication year - 1995
Publication title -
geophysical research letters
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 2.007
H-Index - 273
eISSN - 1944-8007
pISSN - 0094-8276
DOI - 10.1029/94gl02996
Subject(s) - atmosphere (unit) , ozone , photodissociation , martian , atmosphere of mars , atmospheric sciences , environmental chemistry , astrobiology , meteorite , isotopes of oxygen , atmospheric chemistry , isotope , oxygen , environmental science , stratosphere , ozone layer , chemical composition , chemistry , mars exploration program , geology , photochemistry , meteorology , physics , organic chemistry , quantum mechanics , nuclear chemistry
Multi‐isotope (δ 17 O and δ 18 O) measurements of stratospheric CO 2 and 14 CO are reported. Samples were acquired from altitudes in excess of 11.5 km from Christchurch, New Zealand to the South Pole. A mass independent isotopic variation is observed in CO 2 , the magnitude of which correlates well with 14 CO concentration, indicating a stratospheric source of the effect. The component arises from isotopic exchange between the product of O 3 photolysis, O(¹D) and CO 2 thus providing a unique measure of ozone photolysis and turnover. A similar process may occur in the Martian atmosphere, as suggested by water isotopic measurements from SNC meteorites.

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