Problem 7. Assume that a star can be approximated as a black body, using Stefan's Boltzmann Law 1. Show that the luminosity obeys L x R²T4 (0.5) 2. Calculate the wavelength at which the radiation from the Sun peaks. For the Sun: Mo = 2 × 10³3 gram, Lo = 3.9 x 1033 erg/sec and Ro = 7 x 10¹⁰ cm.
Problem 7. Assume that a star can be approximated as a black body, using Stefan's Boltzmann Law 1. Show that the luminosity obeys L x R²T4 (0.5) 2. Calculate the wavelength at which the radiation from the Sun peaks. For the Sun: Mo = 2 × 10³3 gram, Lo = 3.9 x 1033 erg/sec and Ro = 7 x 10¹⁰ cm.
Related questions
Question
H5.

Transcribed Image Text:Problem 7. Assume that a star can be approximated as a black body, using Stefan's Boltzmann Law
1. Show that the luminosity obeys
L x R²T4
(0.5)
2. Calculate the wavelength at which the radiation from the Sun peaks. For the Sun: Mo = 2 × 1033 gram,
Lo = 3.9 x 1033 erg/sec and Ro = 7 × 10¹⁰ cm.
Expert Solution

This question has been solved!
Explore an expertly crafted, step-by-step solution for a thorough understanding of key concepts.
Step by step
Solved in 3 steps
