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{c}
{tag=Work by Sara Seager}
{title2=2007; doi:10.1086/521346}

Authored theoretical paper, Astrophysical Journal 669, 1279–1297. The gas-free solid-planet models distinguish broad composition families while illustrating limitations of inference from <mass> and <radius> alone.

https://arxiv.org/abs/0707.2895

Mass-radius relationships for solid exoplanets by Sara Seager and others

Past exam of the short options paper shared by Prelims and Parts A and B of the physics course of the University of Oxford / 2015 / S30 / 3 / 2 / Solution

Mass-radius relationships for solid exoplanets by Sara Seager and others (2007; doi:10.1086/521346)

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Mass-radius relationships for solid exoplanets by Sara Seager and others (2007; doi:10.1086/521346)

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