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Updated: Jun 21, 2026

Laboratory Drop Towers for the Experimental Simulation of Dust-aggregate Collisions in the Early Solar System
09:44

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Published on: June 5, 2014

若い環恒星円盤における塵粒の成長の証拠

H B Throop1, J Bally, L W Esposito

  • 1Laboratory for Atmospheric and Planetary Sciences, University of Colorado, Boulder, CO 80309-0392, USA. throop@boulder.swri.edu

Science (New York, N.Y.)
|April 28, 2001
PubMed
まとめ

オリオン星雲の若い惑星円盤は,激しい放射線によって破壊されています. それにもかかわらず,惑星の形成が始まっている可能性があり,ディスクが消去される前に,塵粒子がより大きな粒子に成長することを示す証拠があります.

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