ASCL.net

Astrophysics Source Code Library

Making codes discoverable since 1999

ASCL Code Record

[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
Appears in:
http://adsabs.harvard.edu/abs/2015A%26A...583A.116B
Bibcode:
2015ascl.soft11020B

ascl:1511.020
Add this shield to your page
Copy the above HTML to add this shield to your code's website.
Views: 1091