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Richard W Carlson1, Maud Boyet, Mary Horan

  • 1Department of Terrestrial Magnetism, Carnegie Institution of Washington, 5241 Broad Branch Road, NW, Washington, DC 20015, USA. carlson@dtm.ciw.edu

Science (New York, N.Y.)
|May 26, 2007
PubMed
まとめ

隕石内のバリウム,ネオジミウム,サマリウムの同位体変動は,初期の太陽系への多様な恒星の貢献を明らかにします. この研究は,初期の惑星の分化プロセスが隕石のネオジミウム-142 (142Nd) レベルに影響を与えたことを確認しています.

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