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Updated: Dec 6, 2025

Laboratory Drop Towers for the Experimental Simulation of Dust-aggregate Collisions in the Early Solar System
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初期 恒星 の 円盤 の 中 の 4 つの 環状 の 構造

Dominique M Segura-Cox1,2, Anika Schmiedeke3, Jaime E Pineda3

  • 1Center for Astrochemical Studies, Max Planck Institute for Extraterrestrial Physics, Garching, Germany. dom@mpe.mpg.de.

Nature
|October 8, 2020
PubMed
まとめ

惑星の形成は最古の原始恒星段階から始まるかもしれない. 観測により,若い円盤の環状構造が明らかになり,惑星の形成に不可欠な初期の塵粒の成長を示唆し,既存の理論に異議を唱える.

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