A star on the main sequence has a surface temperature of 10,000 K. Use the H-R diagram to determine it’s luminosity (approximately) and then calculate it’s mass and age (you may use solar units). If it were a red giant, could we do this?
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.
1. A star on the main sequence has a surface temperature of
10,000 K. Use the H-R diagram to determine it’s luminosity
(approximately) and then calculate it’s mass and age (you may
use solar units). If it were a red giant, could we do this?
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