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Applying X-ray Imaging Crystal Spectroscopy for Use as a High Temperature Plasma Diagnostic
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結晶塵の分数から彗星の年齢を決定する

J A Nuth1, H G Hill, G Kletetschka

  • 1Astrochemistry Branch, NASA's Goddard Space Flight Centre, Greenbelt, Maryland 20771, USA. u1jan@lepvax.gsfc.nasa.gov

Nature
|August 5, 2000
PubMed
まとめ

彗星の形成は,初期の太陽系に関する手がかりを明らかにします. 若い恒星円盤の塵の熱処理は彗星の組成を説明し,彗星を年代測定する方法を提供し,惑星系進化の洞察を提供します.

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