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[ascl:1511.020] Mercury-T: Tidally evolving multi-planet systems code

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.

Code site:
http://emelinebolmont.gandi.ws/research-interests
Described in:
https://ui.adsabs.harvard.edu/abs/2015A%26A...583A.116B
Bibcode:
2015ascl.soft11020B

Views: 4574

ascl:1511.020
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