From the light and velocity curves of an eclipsing spectroscopic binary star system, it isdetermined that the orbital period is 6.31 yr and the maximum radial velocities of stars A and Bare 5.4 km/s and 22.4 km/s, respectively. Furthermore, the time period between first contactand minimum light (tp-ta) is 0.58 d and the length of the primary minimum (tc-tb) is 0.64 d. Fromthis information, assuming circular orbits, find:a) the ratio of stellar masses.b) the sum of masses (i ~ 90°).c) the individual masses.d) the individual radii.

Given, The radial velocity of stars A and B, vA=5.4km/svB=22.4km/s a. The ratio of stellar masses,…

Answered: From the light and velocity curves of…

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