Let G denote the universal gravitational constant and let M and m denote masses a distance r apart. (a) According to Newton’s Law of Universal Gravitation, M and m attract each other with a force of magnitude _____ . (b) If r is the radius vector from M to m, then the force of attraction that mass M exerts on mass m is ______ .
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.
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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.
Let G denote the universal gravitational constant and let M and m denote masses a distance r apart.
(a) According to Newton’s Law of Universal Gravitation, M and m attract each other with a force of magnitude _____ .
(b) If r is the radius vector from M to m, then the force of attraction that mass M exerts on mass m is ______ .
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