arXiv · 0808.1916
A Computational Tool to Interpret the Bulk Composition of Solid Exoplanets based on Mass and Radius Measurements
Abstract
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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Li Zeng, Sara Seager. 2008-08-13. A Computational Tool to Interpret the Bulk Composition of Solid Exoplanets based on Mass and Radius Measurements. https://doi.org/10.1086/591807
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