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Mercury-T: Tidally evolving multi-planet systems code

hal.structure.identifierLaboratoire d'Histoire des Sciences et de Philosophie - Archives Henri Poincaré [LHSP]
dc.contributor.authorBOLMONT, Emeline
hal.structure.identifierECLIPSE 2015
dc.contributor.authorRAYMOND, Sean N.
hal.structure.identifierCentre de Recherche Astrophysique de Lyon [CRAL]
hal.structure.identifierLaboratoire de Météorologie Dynamique (UMR 8539) [LMD]
dc.contributor.authorLECONTE, J.
hal.structure.identifierECLIPSE 2015
dc.contributor.authorHERSANT, F.
hal.structure.identifierConcurrencyFreaks
dc.contributor.authorCORREIA, Alexandre C. M.,
dc.date.issued2015
dc.description2015ascl.soft11020B - Astrophysics Source Code Library, record ascl:1511.020
dc.description.abstractEnMercury-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.isoen
dc.title.enMercury-T: Tidally evolving multi-planet systems code
dc.typeAutre document
dc.subject.halPlanète et Univers [physics]/Astrophysique [astro-ph]/Planétologie et astrophysique de la terre [astro-ph.EP]
hal.identifierhal-01239706
hal.version1
hal.popularnon
hal.origin.linkhttps://hal.archives-ouvertes.fr//hal-01239706v1
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