AstroSpeedrunSearch
2015

Neutron star or black hole?

Round
Theory
Points
Not given
Level
Silver
Taught in
Section 8.3

Adapted from IOAA 2015 (Magelang), theory problem L2. We have restated it in our own words and kept the original data. The solution was last checked on 21 October 2026.

Two stars A and B, of masses mA and mB, are a distance d apart and move on circular orbits round their centre of mass, in the xy plane with the centre of mass at the origin.

(a) Find the speed and the angular speed of star A. [30%]

(b) An observer far away in the yz plane looks at the stars along a direction at an angle θ to the z axis. The velocity of A along the line of sight is Kcos⁡(ωt+ε), with K and ε positive. Express K3/(ωG) in terms of mA, mB and θ. [30%]

(c) Star A has a mass of 30 solar masses. Star B gives out X-rays and is a neutron star if its mass is less than 2 solar masses, or a black hole if it is more. The observer measures K3/(ωG)=M⊙/250. The angle θ is not known. For which values of θ is B a black hole? [40%]

Answer(a) vA=mBG/((mA+mB)d) and ω=G(mA+mB)/d3. (b) K3/(ωG)=mB3sin3⁡θ/(mA+mB)2. (c) B is a black hole if sin⁡θ is less than 0.8, that is for θ less than 53.1° or more than 126.9°.

This problem also appears among the olympiad problems of Section 8.3, Spectroscopic binaries and the mass function, which teaches the ideas it uses. Equation and figure numbers refer to the course.