In:
Science, American Association for the Advancement of Science (AAAS), Vol. 317, No. 5835 ( 2007-07-13), p. 231-233
Abstract:
Oxygen isotopic composition of our solar system is believed to have resulted from mixing of two isotopically distinct nebular reservoirs, 16 O-rich and 17,18 O-rich relative to Earth. The nature and composition of the 17,18 O-rich reservoir are poorly constrained. We report an in situ discovery of a chemically and isotopically unique material distributed ubiquitously in fine-grained matrix of a primitive carbonaceous chondrite Acfer 094. This material formed by oxidation of Fe,Ni-metal and sulfides by water either in the solar nebula or on a planetesimal. Oxygen isotopic composition of this material indicates that the water was highly enriched in 17 O and 18 O (δ 17,18 O SMOW = +180‰ per mil), providing the first evidence for an extremely 17,18 O-rich reservoir in the early solar system.
Type of Medium:
Online Resource
ISSN:
0036-8075
,
1095-9203
DOI:
10.1126/science.1142021
Language:
English
Publisher:
American Association for the Advancement of Science (AAAS)
Publication Date:
2007
detail.hit.zdb_id:
128410-1
detail.hit.zdb_id:
2066996-3
detail.hit.zdb_id:
2060783-0
SSG:
11
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