SUMMARY
The discussion centers on calculating the velocities and angles of two remnants from a star that breaks apart, emitting light at frequencies of 7.135 x 1014 Hz and 4.282 x 1014 Hz, while the original star emitted light at 6.690 x 1014 Hz. The participants utilized the relativistic Doppler shift equations, specifically v' = v γ [1 - β cos θ] and v' = v √((1 + β)/(1 - β)), to derive the speed of the remnants as 0.235c and β as 0.47. They encountered challenges in determining the angles between the remnants and the line of sight, leading to discussions about the relationship between speed and angle, ultimately concluding that the data provided may contain inconsistencies that prevent a valid solution.
PREREQUISITES
- Understanding of relativistic Doppler shift equations
- Familiarity with the concept of frequency and wavelength relationships
- Knowledge of conservation of momentum in physics
- Basic understanding of trigonometric identities and their application in physics
NEXT STEPS
- Study the derivation and application of the relativistic Doppler shift equations
- Explore the relationship between frequency, wavelength, and speed of light
- Investigate conservation of momentum in relativistic contexts
- Review trigonometric identities relevant to physics problems
USEFUL FOR
Students and educators in physics, particularly those focusing on relativistic mechanics, astrophysics, and anyone involved in solving complex problems related to Doppler effects and momentum conservation.