Terrestrial planet formation from a ring: Long-term simulations accounting for the giant planet instability-Reference-Cited by-同舟云学术

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Terrestrial planet formation from a ring: Long-term simulations accounting for the giant planet instability

Published:2024-07 Issue: Volume:417 Page:116109
ISSN:0019-1035
Container-title:Icarus
language:en
Short-container-title:Icarus

Author:

Woo J.M.Y.,Nesvorný D.,Scora J.,Morbidelli A.

Funder

Deutsche Forschungsgemeinschaft

European Research Council

ERC

Publisher

Elsevier BV

Reference101 articles.

1. The gas drag effect on the elliptic motion of a solid Body in the primordial solar nebula;Adachi;Prog. Theor. Phys.,1976

2. Hit-and-run planetary collisions;Asphaug;Nature,2006

3. Early formation of the moon 4.51 billion years ago;Barboni;Sci. Adv.,2017

4. Collisional stripping of Mercury’s mantle;Benz;Icarus,1988

5. Chronological evidence that the moon is either young or did not have a global magma ocean;Borg;Nature,2011

Cited by 2 articles. 订阅此论文施引文献订阅此论文施引文献，注册后可以免费订阅5篇论文的施引文献，订阅后可以查看论文全部施引文献

1. Composition, structure, and origin of the Moon;Reference Module in Earth Systems and Environmental Sciences;2024

2. Origin of the Earth;Reference Module in Earth Systems and Environmental Sciences;2024

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