Mass-radius relationships for solid exoplanets by Sara Seager and others Created 2026-10-24 Updated 2026-11-05
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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.
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On the Unique Solution of Planet and Star Parameters from an Extrasolar Planet Transit Light Curve by Sara Seager and Gabriela Mallén-Ornelas Created 2026-10-20 Updated 2026-11-05
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By Sara Seager and Gabriela Mallén-Ornelas. Section3.1,equations1–4 specify depth, contact durations and the circular-orbit scale. The2002 manuscript was published in The Astrophysical Journal585,1038–1055(2003).
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Theoretical Transmission Spectra During Extrasolar Giant Planet Transits by Sara Seager and Dimitar Sasselov Created 2026-10-20 Updated 2026-11-05
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By Sara Seager and Dimitar Sasselov. The2000 study calculates transmission absorption through an atmospheric annulus and discusses how weak contrast and clouds affect sensitivity. The Astrophysical Journal537,916–921.
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