A Computational Tool to Interpret the Bulk Composition of Solid Exoplanets based on Mass and Radius Measurements

Details A Computational Tool to Interpret the Bulk Composition of Solid Exoplanets based on Mass and Radius Measurements A Computational Tool to Interpret the Bulk Composition of Solid Exoplanets based on Mass and Radius Measurements

2008-08-13

arxiv.org/abs/0808.1916v1

Astronomy and Astrophysics

Astrophysics

PASP, in press. 20 pages including 5 figures. Try the MATLAB code and send us comments

Scientific paper

The prospects for finding transiting exoplanets in the range of a few to 20
Earth masses is growing rapidly with both ground-based and spaced-based
efforts. We describe a publicly available computer code to compute and quantify
the compositional ambiguities for differentiated solid exoplanets with a
measured mass and radius, including the mass and radius uncertainties.

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