Applying Gauss's Law for Gravitation. Using Gauss's law for gravitation ∮g⃗ ⋅dA⃗ =−4(pi)GMenclosed where Menclosed is the total mass enclosed within the closed surface, show that the following statements are true: (a) For any spherically symmetric mass distribution with total mass M, the acceleration due to gravity outside the distribution is the same as though all the mass were concentrated at the center. (b) At any point inside a spherically symmetric shell of mass, the acceleration due to gravity is zero. (c) If we drill a hole through a spherically symmetric planet to its center, and if the density were uniform, we would find that the magnitude of g⃗ is directly proportional to the distance r from the center.
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.
Applying Gauss's Law for Gravitation. Using Gauss's law for gravitation ∮g⃗ ⋅dA⃗ =−4(pi)GMenclosed where Menclosed is the total mass enclosed within the closed surface, show that the following statements are true: (a) For any spherically symmetric mass distribution with total mass M, the acceleration due to gravity outside the distribution is the same as though all the mass were concentrated at the center. (b) At any point inside a spherically symmetric shell of mass, the acceleration due to gravity is zero. (c) If we drill a hole through a spherically symmetric planet to its center, and if the density were uniform, we would find that the magnitude of g⃗ is directly proportional to the distance r from the center.
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