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熱クロノメトリーによって明らかにされたH-コンドライト母小惑星の構造と熱史

Mario Trieloff1, Elmar K Jessberger, Ingrid Herrwerth

  • 1Mineralogisches Institut der Universität Heidelberg, Im Neuenheimer Feld 236, D-69120 Heidelberg, Germany. trieloff@min.uni-heidelberg.de

Nature
|April 4, 2003
PubMed
まとめ

Hコンドライトのような初期の太陽系惑星系は,アルミニウム-26の腐敗による内部加熱によって急速に形成された可能性が高い. これにより,数百万年にわたって冷却された層状の親体が形成され,中央地域はより高い温度を経験し,外層よりも冷却が遅い.

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