Zobrazeno 1 - 10
of 86
pro vyhledávání: '"Nice 2 model"'
Autor:
Matthieu Gounelle, Tristan Guillot, Elena Lega, A. Crida, Seth A. Jacobson, Alessandro Morbidelli, Michiel Lambrechts, Bertram Bitsch, Anders Johansen
Publikováno v:
Icarus
Icarus, 2016, 267, pp.368-376. ⟨10.1016/j.icarus.2015.11.027⟩
Icarus, Elsevier, 2016, 267, pp.368-376. ⟨10.1016/j.icarus.2015.11.027⟩
Icarus, 2016, 267, pp.368-376. ⟨10.1016/j.icarus.2015.11.027⟩
Icarus, Elsevier, 2016, 267, pp.368-376. ⟨10.1016/j.icarus.2015.11.027⟩
The terrestrial planets and the asteroids dominant in the inner asteroid belt are water poor. However, in the protoplanetary disk the temperature should have decreased below water condensation level well before the disk was photoevaporated. Thus, the
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::9a42a6ac70c5b75944327ec777ec2e3c
Publikováno v:
Geophysical Research Letters. 42:256-263
We investigate the problem of satellite survival during a hypothetical late heavy bombardment in the outer solar system, as predicted by the Nice Model (Tsiganis, Gomes, Morbidelli, & Levison 2005, Nature 435). Using a Monte-Carlo approach we calcula
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::86ddcfebc0be1e4de7608ef51f0a2730
https://doi.org/10.1002/2014gl062133
https://doi.org/10.1002/2014gl062133
Autor:
Akio Makishima
In Chapter 2, formation of the solar system from a gas nebula is discussed. In geophysical models, our solar system is considered to have started from the gas cloud. Then it began to gather and rotate, forming the Sun as well as the planetary system.
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::ba74b9f92091ee3e3a09a5c7c6de1a56
https://doi.org/10.1016/b978-0-12-812058-3.00002-8
https://doi.org/10.1016/b978-0-12-812058-3.00002-8
Autor:
Andrea Bolle, Christian Circi
Publikováno v:
Communications in Nonlinear Science and Numerical Simulation. 19:1375-1390
The discovery of several extrasolar systems, each one characterized by its own planetary distribution around a central star, made the scientific interest addressed to the analysis of models permitting to predict, or at least estimate, the orbital fea
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::d0492064fd033d406a90378a77129004
https://doi.org/10.1016/j.cnsns.2013.09.018
https://doi.org/10.1016/j.cnsns.2013.09.018
Publikováno v:
Icarus. 232:13-21
We quantify the relative contribution of volatiles supplied from outer Solar System planetesimal reservoirs to large wet asteroids during the first few My after the beginning of the Solar System. To that end, we simulate the fate of planetesimals ori
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::aaf07d2aaa2a48b8b0980fb7daa80405
https://doi.org/10.1016/j.icarus.2013.12.011
https://doi.org/10.1016/j.icarus.2013.12.011
We study how close-in systems such as those detected by Kepler are affected by the dynamics of bodies in the outer system. We consider two scenarios: outer systems of giant planets potentially unstable to planet--planet scattering, and wide binaries
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::6cfcbe1ee90527d3c189cf5891e27907
http://arxiv.org/abs/1609.08058
http://arxiv.org/abs/1609.08058
Autor:
Mohamad Ali-Dib
We investigate the chemical composition of the solar system's giant planets atmospheres using a physical formation model with chemistry. The model incorporate disk evolution, pebbles and gas accretion, type I and II migration, simplified disk photoev
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::d6f8745f62cdd2d5330d27fb73f42127
Autor:
Alessandro Morbidelli
Publikováno v:
Comptes Rendus. Physique
Comptes Rendus. Physique, Académie des sciences (Paris), 2011, 12, pp.651-659
Comptes Rendus. Physique, Académie des sciences (Paris), 2011, 12, pp.651-659
Since the discovery of the first extra-solar planets, we are confronted with the puzzling diversity of planetary systems. Processes like planet radial migration in gas-disks and planetary orbital instabilities, often invoked to explain the exotic orb
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::ab589164a7cba587440f911a92d27bc1
https://doi.org/10.1016/j.crhy.2010.11.001
https://doi.org/10.1016/j.crhy.2010.11.001
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 407:1859-1865
We report on some simple experiments on the nature of chaos in our planetary system. We make the following interesting observations. First, we look at the system of Sun + four Jovian planets as an isolated five-body system interacting only via Newton
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::6cb950f110276fdae8d1931c14aee9ab
https://doi.org/10.1111/j.1365-2966.2010.17027.x
https://doi.org/10.1111/j.1365-2966.2010.17027.x
Publikováno v:
Icarus
We present results from a suite of N-body simulations that follow the accretion history of the terrestrial planets using a new parallel treecode that we have developed. We initially place 2000 equal size planetesimals between 0.5--4.0 AU and the coll
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::023739ba132774976ffc74deb2595951
https://doi.org/10.1016/j.icarus.2009.11.038
https://doi.org/10.1016/j.icarus.2009.11.038