Mercury-T: Tidally evolving multi-planet systems code
BOLMONT, Emeline
Laboratoire d'Histoire des Sciences et de Philosophie - Archives Henri Poincaré [LHSP]
Laboratoire d'Histoire des Sciences et de Philosophie - Archives Henri Poincaré [LHSP]
LECONTE, J.
Centre de Recherche Astrophysique de Lyon [CRAL]
Laboratoire de Météorologie Dynamique (UMR 8539) [LMD]
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Centre de Recherche Astrophysique de Lyon [CRAL]
Laboratoire de Météorologie Dynamique (UMR 8539) [LMD]
BOLMONT, Emeline
Laboratoire d'Histoire des Sciences et de Philosophie - Archives Henri Poincaré [LHSP]
Laboratoire d'Histoire des Sciences et de Philosophie - Archives Henri Poincaré [LHSP]
LECONTE, J.
Centre de Recherche Astrophysique de Lyon [CRAL]
Laboratoire de Météorologie Dynamique (UMR 8539) [LMD]
< Reduce
Centre de Recherche Astrophysique de Lyon [CRAL]
Laboratoire de Météorologie Dynamique (UMR 8539) [LMD]
Language
en
Autre document
This item was published in
2015
English Abstract
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 ...Read more >
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.Read less <
Origin
Hal imported