SUMMARY
The combined apparent magnitude of two close stars with individual magnitudes of V = 5.1 and V = 4.6 is calculated using the luminosity-magnitude relation rather than direct addition. The correct apparent magnitude is determined to be approximately 4.07. The discussion also includes a related problem involving a binary star system with a total apparent magnitude of 15.00, where one star is twice as bright as the other, leading to a derived apparent magnitude of 15.44 for the brighter star. The participants clarify the use of the formula m = -2.5*log(L/4*pi*d^2) and its simplifications for solving these types of problems.
PREREQUISITES
- Understanding of apparent magnitude and luminosity concepts
- Familiarity with logarithmic functions and their properties
- Knowledge of the formula m = -2.5*log(L/4*pi*d^2)
- Basic grasp of binary star systems and their brightness relationships
NEXT STEPS
- Study the derivation and application of the luminosity-magnitude relation
- Learn how to calculate distances to stars using the distance modulus formula D = 10 ^ (m-M)/5 x 10
- Explore examples of binary star systems and their apparent magnitudes
- Review logarithmic properties and their applications in astrophysics
USEFUL FOR
Astronomy students, astrophysics enthusiasts, and anyone studying stellar properties and binary star systems will benefit from this discussion.