Zobrazeno 1 - 10
of 224
pro vyhledávání: '"Jumping-Jupiter scenario"'
Publikováno v:
Celestial Mechanics and Dynamical Astronomy. 125:451-484
In a previous paper (Hou et al. in Celest Mech Dyn Astron 119:119–142, 2014a), the problem of dynamical symmetry between two Jupiter triangular libration points (TLPs) with Saturn’s perturbation in the present configuration of the two planets was
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::5b7957a72ae171acac882e2ed038ea9f
https://doi.org/10.1007/s10569-016-9692-1
https://doi.org/10.1007/s10569-016-9692-1
Publikováno v:
Monthly Notices of the Royal Astronomical Society
Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, 2016, 458 (3), pp.2962-2972. ⟨10.1093/mnras/stw431⟩
Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, 2016, 458 (3), pp.2962-2972. ⟨10.1093/mnras/stw431⟩
Jupiter's core is generally assumed to have formed beyond the snow line. Here we consider an alternative scenario, that Jupiter's core may have accumulated in the innermost parts of the protoplanetary disk. A growing body of research suggests that sm
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::b5e76bddbbb3fa075cd3e9211f3b8f5c
https://doi.org/10.1093/mnras/stw431
https://doi.org/10.1093/mnras/stw431
Autor:
P. S. Krasil’nikov, R. N. Amelin
Publikováno v:
Cosmic Research. 54:127-133
Saturn’s rotation relative to a center of mass is considered within an elliptic restricted three-body problem. It is assumed that Saturn is a solid under the action of gravity of the Sun and Jupiter. The motions of Saturn and Jupiter are considered
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::6bc12f00a286eaf6a4de6c55d0b9653b
https://doi.org/10.1134/s0010952516020027
https://doi.org/10.1134/s0010952516020027
Autor:
Nathan A. Kaib, John Chambers
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 455:3561-3569
Many features of the outer solar system are replicated in numerical simulations if the giant planets undergo an orbital instability that ejects one or more ice giants. During this instability, Jupiter and Saturn's orbits diverge, crossing their 2:1 m
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::ec5287b5428eb1d98c7b94c5f171e50f
https://doi.org/10.1093/mnras/stv2554
https://doi.org/10.1093/mnras/stv2554
Publikováno v:
Space Science Reviews. 197:191-269
Comets have three known reservoirs: the roughly spherical Oort Cloud (for long-period comets), the flattened Kuiper Belt (for ecliptic comets), and, surprisingly, the asteroid belt (for main-belt comets). Comets in the Oort Cloud were thought to have
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::82525c544d2e905370e1b2844073bac8
https://doi.org/10.1007/s11214-015-0223-2
https://doi.org/10.1007/s11214-015-0223-2
Autor:
Hugh F. Wilson
Publikováno v:
Icarus. 250:400-404
Recent work has suggested that gas giant planets such as Jupiter and Saturn may not consist of a small number of fully convective and chemically homogenous layers as has been conventionally assumed, but instead may be chemically inhomogeneous with co
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::6b766a6f52a484e1bd54f28618e6cda2
https://doi.org/10.1016/j.icarus.2014.11.031
https://doi.org/10.1016/j.icarus.2014.11.031
Autor:
N. Nettelmann
Publikováno v:
Contributions to Plasma Physics. 55:116-122
The H-He rich giant planets Jupiter and Saturn serve to test predictions on the high-pressure behavior of hydrogen and helium. Incorporating the process of H/He phase separation and He rain, or of core erosion, into planet structure and evolution mod
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::94bf4018bd45de6affc4e7c46854988d
https://doi.org/10.1002/ctpp.201400093
https://doi.org/10.1002/ctpp.201400093
Publikováno v:
Icarus
Icarus, Elsevier, 2018, 306, pp.319-327. ⟨10.1016/j.icarus.2017.10.018⟩
Icarus, Elsevier, 2018, 306, pp.319-327. ⟨10.1016/j.icarus.2017.10.018⟩
The origin of the orbital structure of the cold component of the Kuiper belt is still a hot subject of investigation. Several features of the solar system suggest that the giant planets underwent a phase of global dynamical instability, but the actua
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::d81b727aa6685c6ee2e616dd34e76c79
http://arxiv.org/abs/1710.05178
http://arxiv.org/abs/1710.05178
Autor:
Andre Izidoro, Sean N. Raymond
Publikováno v:
Icarus
Icarus, Elsevier, 2017, 297, pp.134-148. 〈10.1016/j.icarus.2017.06.030〉
Icarus, Elsevier, 2017, 297, pp.134-148. ⟨10.1016/j.icarus.2017.06.030⟩
Icarus, Elsevier, 2017, 297, pp.134-148. 〈10.1016/j.icarus.2017.06.030〉
Icarus, Elsevier, 2017, 297, pp.134-148. ⟨10.1016/j.icarus.2017.06.030⟩
There is a long-standing debate regarding the origin of the terrestrial planets' water as well as the hydrated C-type asteroids. Here we show that the inner Solar System's water is a simple byproduct of the giant planets' formation. Giant planet core
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::5c250a3c92faa89ecbb6b953960278d5
https://hal.archives-ouvertes.fr/hal-01558774
https://hal.archives-ouvertes.fr/hal-01558774
Publikováno v:
Web of Science
Repositório Institucional da UNESP
Universidade Estadual Paulista (UNESP)
instacron:UNESP
Repositório Institucional da UNESP
Universidade Estadual Paulista (UNESP)
instacron:UNESP
V-type asteroids are a taxonomic class whose surface is associated to a basaltic composition. The only known source of V-type asteroids in the Main Asteroid Belt is (4) Vesta, that is located in the inner part of the belt. However, many V-type astero
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::0e8e0fc8d1a47075fbec9629f824eef0