Class: Electrmagnetics As mentioned in class, the methods used in electrostatics can also be applied to Newtonian gravitation. Consider a spherical star of mass M and radius R. For simplicity, let’s assume that the density of the star can be approximated as p = c1(1 - (r/R)), ? ≤ ? (where r is less than or equal to R) where c1 is a constant. a. Determine the gravitational field produced by this star everywhere in terms of the mass M and radius R. b. Use your answer from (a) to determine the gravitational self-energy in terms of mass M and radius R.
Class: Electrmagnetics As mentioned in class, the methods used in electrostatics can also be applied to Newtonian gravitation. Consider a spherical star of mass M and radius R. For simplicity, let’s assume that the density of the star can be approximated as p = c1(1 - (r/R)), ? ≤ ? (where r is less than or equal to R) where c1 is a constant. a. Determine the gravitational field produced by this star everywhere in terms of the mass M and radius R. b. Use your answer from (a) to determine the gravitational self-energy in terms of mass M and radius R.
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Class: Electrmagnetics
As mentioned in class, the methods used in electrostatics can also be applied to Newtonian
gravitation. Consider a spherical star of mass M and radius R. For simplicity, let’s assume
that the density of the star can be approximated as
p = c1(1 - (r/R)), ? ≤ ? (where r is less than or equal to R)
where c1 is a constant.
a. Determine the gravitational field produced by this star everywhere in
terms of the mass M and radius R.
b. Use your answer from (a) to determine the gravitational self-energy in
terms of mass M and radius R.
Transcribed Image Text:As mentioned in class, the methods used in electrostatics can also be applied to Newtonian
gravitation. Consider a spherical star of mass M and radius R. For simplicity, let's assume
that the density of the star can be approximated as
p = c₂ (1-7),
r≤R
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