2013
Splitting the light of a binary
- Round
- Theory
- Points
- 10
- Level
- Bronze
- Taught in
- Section 4.2
Adapted from IOAA 2013 (Volos), theory problem S8. We have restated it in our own words and kept the original data. The solution was last checked on 20 October 2026.
A binary star cannot be split in a telescope and is seen from Earth as one star of magnitude 5.00. One of its stars is twice as bright as the other. What are the magnitudes of the two stars?
Write the fluxes of the two stars as and . What is their sum, in terms of the flux of a star of magnitude 5.00?
- Let the fainter star give flux
and the brighter . Together they give , the flux of a star of magnitude 5.00. - The fainter star gives a third of that flux, so by (4.2) it is fainter by
magnitudes, and . - The brighter star gives two thirds of the total, so it is fainter than the pair by
magnitudes, and . - As a check, the two differ by
magnitudes, as a ratio of 2 requires.
AnswerThe brighter star has magnitude 5.44 and the fainter 6.19.
This problem also appears among the olympiad problems of Section 4.2, The magnitude scale, which teaches the ideas it uses. Equation and figure numbers refer to the course.