Chondrule Formation by the Jovian Sweeping Secular Resonance

Chondrules are silicate spheroids found in meteorites, and they serve as important fossil records of the early solar system. In order to form chondrules, chondrule precursors must be heated to temperatures much higher than the typical conditions in the current asteroid belt. One proposed mechanism f...

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Veröffentlicht in:	The Astrophysical journal 2019-10, Vol.883 (2), p.164
Hauptverfasser:	Gong, Munan, Zheng, Xiaochen, Lin, Douglas N. C., Silsbee, Kedron, Baruteau, Clement, Mao, Shude
Format:	Artikel
Sprache:	eng
Schlagworte:	Aluminum Asteroids Astrophysics Calcium Chondrule Computer simulation Depletion Earth and Planetary Astrophysics Eccentricity Heating Inclusions Jupiter Mathematical models Meteorites meteorites, meteors, meteoroids minor planets, asteroids: general Numerical simulations Orbital mechanics Physics Planet formation Planetary evolution Precursors Protoplanetary disks Rarefied gases Resonance shock waves Solar system Spheroids Sweeping
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