Select average representative temperatures for 1) the average Earth surface, 2) the Sun, 3) a typical cloud, and 4) typical snow and calculate: a) The rate of electromagnetic energy emission for each surface in Wm-2, assuming all surfaces are blackbodies. b) The wavelength of maximum radiation in mum and determine the portion of the spectrum in which it occur
Stellar evolution
We may see thousands of stars in the dark sky. Our universe consists of billions of stars. Stars may appear tiny to us but they are huge balls of gasses. Sun is a star of average size. Some stars are even a thousand times larger than the sun. The stars do not exist forever they have a certain lifetime. The life span of the sun is about 10 billion years. The star undergoes various changes during its lifetime, this process is called stellar evolution. The structure of the sun-like star is shown below.
Red Shift
It is an astronomical phenomenon. In this phenomenon, increase in wavelength with corresponding decrease in photon energy and frequency of radiation of light. It is the displacement of spectrum of any kind of astronomical object to the longer wavelengths (red) side.
Select average representative temperatures for 1) the average Earth surface, 2) the Sun, 3) a typical cloud, and 4) typical snow and calculate:
a) The rate of
b) The wavelength of maximum
Step by step
Solved in 4 steps with 3 images
