Science (New York, N.Y.)
|July 29, 1988
PubMed
まとめ

数学的シミュレーションでは,3Dプレソラー星雲の崩壊が小惑星領域で高温 (1500 K) を発生させ,惑星形成における重要な論争を解決することが示されています. これは,初期の太陽星雲における固体の熱循環を説明するかもしれない.

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