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pro vyhledávání: '"collisional evolution"'
Akademický článek
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Autor:
Bottke, William, Vokrouhlicky, David, Marshall, Raphael, Nesvorny, David, Morbidelli, Alessandro, Deienno, Rogerio, Marchi, Simone, Dones, Luke, Levison, Harold
The tumultuous early era of outer solar system evolution culminated when Neptune migrated across the primordial Kuiper belt (PKB) and triggered a dynamical instability among the giant planets. This event led to the ejection of approximately 99.9\% of
Externí odkaz:
http://arxiv.org/abs/2307.07089
Autor:
Houge, Adrien, Krijt, Sebastiaan
Most protoplanetary discs are thought to undergo violent and frequent accretion outbursts, during which the accretion rate and central luminosity are elevated for several decades. This temporarily increases the disc temperature, leading to the sublim
Externí odkaz:
http://arxiv.org/abs/2303.11318
Conditions in the outer protoplanetary disk during Solar System formation were thought to be favorable for the formation of amorphous water ice (AWI),a glassy phase of water ice. However, subsequent collisional processing could have shock crystallize
Externí odkaz:
http://arxiv.org/abs/2212.03852
Autor:
Santiago, Raíssa, Caxito, Fabricio de Andrade, Pedrosa-Soares, Antonio, Neves, Mirna Aparecida, Dantas, Elton Luiz, Calegari, Salomão Silva, Lana, Cristiano
Publikováno v:
In Precambrian Research October 2023 397
Autor:
Szalay, J. R., Pokorny, P., Malaspina, D. M., Pusack, A., Bale, S. D., Battams, K., Gasque, L. C., Goetz, K., Kruger, H., McComas, D. J., Schwadron, N. A., Strub, P.
The zodiacal cloud is one of the largest structures in the solar system and strongly governed by meteoroid collisions near the Sun. Collisional erosion occurs throughout the zodiacal cloud, yet it is historically difficult to directly measure and has
Externí odkaz:
http://arxiv.org/abs/2104.08217
If the Solar system had a history of planet migration, the signature of that migration may be imprinted on the populations of asteroids and comets that were scattered in the planets' wake. Here, we consider the dynamical and collisional evolution of
Externí odkaz:
http://arxiv.org/abs/1903.03199
Autor:
Walsh, Kevin J., Levison, Harold F.
Publikováno v:
Icarus 329,1 (2019)
We present numerical simulations of terrestrial planet formation that examine the growth continuously from planetesimals to planets in the inner Solar System. Previous studies show that the growth will be inside-out, but it is still common practice t
Externí odkaz:
http://arxiv.org/abs/1908.00897
Akademický článek
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