Mercury-T: Tidally evolving multi-planet systems code
hal.structure.identifier | Laboratoire d'Histoire des Sciences et de Philosophie - Archives Henri Poincaré [LHSP] | |
dc.contributor.author | BOLMONT, Emeline | |
hal.structure.identifier | ECLIPSE 2015 | |
dc.contributor.author | RAYMOND, Sean N. | |
hal.structure.identifier | Centre de Recherche Astrophysique de Lyon [CRAL] | |
hal.structure.identifier | Laboratoire de Météorologie Dynamique (UMR 8539) [LMD] | |
dc.contributor.author | LECONTE, J. | |
hal.structure.identifier | ECLIPSE 2015 | |
dc.contributor.author | HERSANT, F. | |
hal.structure.identifier | ConcurrencyFreaks | |
dc.contributor.author | CORREIA, Alexandre C. M., | |
dc.date.issued | 2015 | |
dc.description | 2015ascl.soft11020B - Astrophysics Source Code Library, record ascl:1511.020 | |
dc.description.abstractEn | Mercury-T calculates the evolution of semi-major axis, eccentricity, inclination, rotation period and obliquity of the planets as well as the rotation period evolution of the host body; it is based on the N-body code Mercury (Chambers 1999, ascl:1201.008). It is flexible, allowing computation of the tidal evolution of systems orbiting any non-evolving object (if its mass, radius, dissipation factor and rotation period are known), but also evolving brown dwarfs (BDs) of mass between 0.01 and 0.08 M⊙, an evolving M-dwarf of 0.1 M⊙, an evolving Sun-like star, and an evolving Jupiter. | |
dc.language.iso | en | |
dc.title.en | Mercury-T: Tidally evolving multi-planet systems code | |
dc.type | Autre document | |
dc.subject.hal | Planète et Univers [physics]/Astrophysique [astro-ph]/Planétologie et astrophysique de la terre [astro-ph.EP] | |
hal.identifier | hal-01239706 | |
hal.version | 1 | |
hal.popular | non | |
hal.origin.link | https://hal.archives-ouvertes.fr//hal-01239706v1 | |
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