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The oxygen isotopic composition of the Sun inferred from captured solar wind.

Authors :
McKeegan KD
Kallio AP
Heber VS
Jarzebinski G
Mao PH
Coath CD
Kunihiro T
Wiens RC
Nordholt JE
Moses RW Jr
Reisenfeld DB
Jurewicz AJ
Burnett DS
Source :
Science (New York, N.Y.) [Science] 2011 Jun 24; Vol. 332 (6037), pp. 1528-32.
Publication Year :
2011

Abstract

All planetary materials sampled thus far vary in their relative abundance of the major isotope of oxygen, (16)O, such that it has not been possible to define a primordial solar system composition. We measured the oxygen isotopic composition of solar wind captured and returned to Earth by NASA's Genesis mission. Our results demonstrate that the Sun is highly enriched in (16)O relative to the Earth, Moon, Mars, and bulk meteorites. Because the solar photosphere preserves the average isotopic composition of the solar system for elements heavier than lithium, we conclude that essentially all rocky materials in the inner solar system were enriched in (17)O and (18)O, relative to (16)O, by ~7%, probably via non-mass-dependent chemistry before accretion of the first planetesimals.

Details

Language :
English
ISSN :
1095-9203
Volume :
332
Issue :
6037
Database :
MEDLINE
Journal :
Science (New York, N.Y.)
Publication Type :
Academic Journal
Accession number :
21700868
Full Text :
https://doi.org/10.1126/science.1204636