Zobrazeno 1 - 10
of 125
pro vyhledávání: '"Co-orbital resonance"'
Despite the existence of co-orbital bodies in the solar system, and the prediction of the formation of co-orbital planets by planetary system formation models, no co-orbital exoplanets (also called trojans) have been detected thus far. In this paper
Externí odkaz:
http://arxiv.org/abs/1901.07640
Autor:
Lemos, Pablo, Gallardo, Tabaré
Publikováno v:
Planetary and Space Science, Volume 161, p. 76-83, October 2018
In this work we pose the possibility that, at an early stage, the migration of a proto--giant planet caused by the presence of a gaseous circumstellar disk could explain the continuous feeding of small bodies into its orbit. Particularly, we study th
Externí odkaz:
http://arxiv.org/abs/1806.06005
Autor:
Oshima, Kenta1 (AUTHOR) k.oshima.nt@cc.it-hiroshima.ac.jp
Publikováno v:
Astrophysics & Space Science. Apr2022, Vol. 367 Issue 4, p1-14. 14p.
Autor:
Reiter, Stefanie1 stefanie.reiter@univie.ac.at, Lhotka, Christoph1,2 lhotka@mat.uniroma2.it
Publikováno v:
Proceedings of the International Astronomical Union. Oct2021, Vol. 15 Issue S364, p102-107. 6p.
Publikováno v:
In Icarus 1 September 2016 275:239-248
Autor:
Kenta Oshima
Publikováno v:
Astrophysics and Space Science. 367
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::29efa52ad45778ab172c2dac16e27a54
https://doi.org/10.1007/s10509-022-04071-4
https://doi.org/10.1007/s10509-022-04071-4
Autor:
Stefanie Reiter, Christoph Lhotka
Publikováno v:
Proceedings of the International Astronomical Union. 15:102-107
The interplanetary magnetic field may cause large amplitude changes in the orbital inclinations of charged dust particles. In order to study this effect in the case of dust grains moving in 1:1 mean motion resonance with planet Jupiter, a simplified
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::b5b3eb1821d4366db9cedcc1cf8c7a8a
https://doi.org/10.1017/s1743921322000758
https://doi.org/10.1017/s1743921322000758
Autor:
Pousse, Alexandre
Publikováno v:
Astrophysique [astro-ph]. Université Paris sciences et lettres, 2016. Français. ⟨NNT : 2016PSLEO006⟩
This work of thesis focuses on the study of the coorbital resonance. This domain of particular trajectories, where an asteroid and a planet gravitate around the Sun with the same period possesses a very rich dynamics connected to the famous Lagrange
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=dedup_wf_001::4a657ca650e095757f3be681830a9e50
https://theses.hal.science/tel-01457149
https://theses.hal.science/tel-01457149
Despite the existence of co-orbital bodies in the solar system, and the prediction of the formation of co-orbital planets by planetary system formation models, no co-orbital exoplanets (also called trojans) have been detected thus far. In this paper
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::fac29076c53781f327f39b51a2d1aecf
http://arxiv.org/abs/1901.07640
http://arxiv.org/abs/1901.07640
Despite the existence of co-orbital bodies in the solar system, and the prediction of the formation of co-orbital planets by planetary system formation models, no co-orbital exoplanets (also called trojans) have been detected thus far. In this paper
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::c89fa9f3d49abbd509c96b885c85625e