Hey Future astrophysicists!!!
Here are some questions for you!!
1. Explain Angular Momentum Problem!
2. What is meant by Bidirectional scattering distribution function???
3. what is Darwin –Radau equation??
Answers
Answer:
1. Angular momentum is defined, mathematically, as L=Iω, or L=rxp. Which is the moment of inertia times the angular velocity, or the radius of the object crossed with the linear momentum. In a closed system, angular momentum is conserved in all directions after a collision.
2.The bidirectional scattering distribution function (BSDF) radiometrically characterizes the scatter of optical radiation from a surface as a function of the angular positions of the incident and scattered beams.
Explanation:
3. astrophysics, the Darwin–Radau equation (named after Rodolphe Radau and Charles Galton Darwin) gives an approximate relation between the moment of inertia factor of a planetary body and its rotational speed and shape. The moment of inertia factor is directly related to the largest principal moment of inertia, C.
1) The property of any rotating object given by moment of inertia times angular velocity.
2)It is used to evaluate the scattering properties of chemically vapor-deposited (CVD) zinc selenide (ZnSe).
3)It gives an approximate relation between the moment of inertia factor of a planetary body and its rotational speed and shape.
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