9 Gravitational Field Flashcards
Newton’s Law of Gravitation
The force of attraction between any two point masses is directly proportional to the product of their masses and inversely proportional to the square of their separation
F = Gm(1)m(2)/r^2
Gravitation constant, G
G = 6.67*10^-11 N m^2 kg^-2
Kepler’s Third Law
Gravitational force provides for centripetal force
F(g) = F(resultant)
Solving:
T^2 directly proportional to r^3
Binary star
m(A) r(A) = m(B) r(B)
Geostationary orbit
- Only one such orbit around Earth (above the equator and a fixed distance 4.2*10^7 m
- Orbital period is 24h
- Plane of orbit coincides with the equatorial plane
- Satellite orbits west to east
Gravitational field
A region in space where a mass experiences a gravitational force acting on it
Gravitational field strength, g
The gravitational force per unit mass acting on a small mass placed at that point
g = F/m
g = GM/r^2
Gravitational potential energy
Work done by an external agent in bringing the mass from infinity to that point without any change in kinetic energy
GPE= -GMm/r
Why is gravitational potential energy negative?
- Work done is taken with infinity as reference, hence gravitational potential energy at infinity is zero
- Due to attractive nature of gravity, the force by external agent is directed away from the mass producing the gravitational attraction
- Force by external agent is opposite is direction to the displacement of the mass, m
negative sign does not indicate direction, only means that the potential energy at a point closer to the fixed mass is lesser compared to the potential energy at infinity which is defined as 0
Gravitational potential, Φ
Work done per unit mass by an external agent in bringing a mass from infinity to that point
Φ = GPE/m = -GM/r
Escape velocity
Minimum kinetic energy required is equal to the gain in gravitational potential energy in reaching infinity
1/2 mv^2 = GMm/r
v = √(2GM/r)