AstroSpeedrunSearch
2010

A binary seen face on

Round
Theory
Points
10
Level
Bronze
Taught in
Section 8.2

Adapted from IOAA 2010 (Beijing), theory problem S4. We have restated it in our own words and kept the original data. The solution was last checked on 21 October 2026.

A binary star is 10 pc away. The largest angular separation of its two stars is 7.0″ and the smallest 1.0″. The period is 100 years and the orbit is face on, at right angles to the line of sight. The orbit of one star round the centre of mass has an angular semi-major axis of α1=3.0″. Estimate the mass of each star, in solar masses.

AnswerStar 1, with the larger orbit, has 1.6 solar masses and star 2 has 4.8 solar masses.

This problem also appears among the olympiad problems of Section 8.2, Visual binaries and the masses of stars, which teaches the ideas it uses. Equation and figure numbers refer to the course.