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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