An Introduction to Modern Astrophysics · Problem 7.18

The Classification of Stellar Spectra — Carroll & Ostlie

Physics — Astrophysics · twostars-ogle-tr-56b

Problem

Using the data given in the text, and assuming that the orbital inclination is 90∘90^\circ, use TwoStars (Appendix K) to generate data that model the light curve of OGLE-TR-56b. You may assume that the radius of the planet is approximately the radius of Jupiter (7×1077 \times 10^7 m) and its temperature is roughly 1000 K. Take the temperature of the star to be 3000 K. You may also assume that the planet's orbit is perfectly circular.

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