Gravitational potential
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Define gravitational potential (ϕ) at a point in a gravitational field.
Gravitational potential (ϕ) at a point is the work done per unit mass in bringing a small test mass from infinity to that point. It's a scalar quantity and is always negative.
State the formula for gravitational potential (ϕ) due to a point mass M at a distance r.
The gravitational potential (ϕ) is given by: ϕ = –GM / r, where G is the gravitational constant and r is the distance from the center of mass M. Note the negative sign; it indicates that work needs to be done *against* the gravitational field to increase potential.
Explain why gravitational potential is always a negative value.
Gravitational potential is negative because the gravitational force is attractive. Work is done *by* the field as a mass moves from infinity towards another mass. Since potential is defined as work done *against* the field, it is negative at all finite distances.
How does gravitational potential change as you move further away from a point mass?
As the distance (r) from a point mass increases, the gravitational potential (ϕ) becomes less negative (i.e., increases). At infinity, the gravitational potential is defined to be zero.
State the formula for gravitational potential energy (EP) of two point masses, M and m, separated by a distance r.
The gravitational potential energy (EP) is given by: EP = –GMm / r, where G is the gravitational constant. This represents the work done to separate the masses to infinity.
Describe the relationship between gravitational potential energy and gravitational potential.
Gravitational potential energy (EP) is the product of the gravitational potential (ϕ) at a point and the mass (m) placed at that point: EP = mϕ. Therefore, if you know the potential at a location, you can easily determine the potential energy of any mass placed there.
A 10kg mass is placed 5m away from a 1000kg mass. What is the gravitational potential energy of the 10kg mass?
E_p = -GMm/r = -(6.67 x 10^-11)(1000)(10)/5 = -1.33 x 10^-7 J. Remember to use appropriate units.
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