21 Gravitational Fields Flashcards

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1
Q

what is the strength of a gravitational field, g?

A

the force per unit mass on a small test mass placed in the field

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2
Q

what is the formula for g?

A

g = F/m

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3
Q

what else is g?

A

the acceleration of a freely falling object

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4
Q

what is a radial field?

A

a field in which the field lines are straight and converge or diverge as if from a single point

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5
Q

what is a uniform field?

A

a region where the field strength is the same in magnitude and direction at every point in the field

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6
Q

what is the gravitational potential energy?

A

the energy of an object due to its position

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7
Q

what is gravitational potential, V?

A

the work done per unit mass to move a small object from infinity to that point

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8
Q

what is the formula for V?

A

V = W/m

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9
Q

what is an equipotential?

A

a surface with a constant gravitational potential

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10
Q

what is a potential gradient?

A

the change in the potential per metre at a point

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11
Q

what is the formula for change of potential?

A

potential gradient = ΔV/Δr (Δr = small distance

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12
Q

what is gravitational field strength equal to?

A

negative of the potential gradient
g = -ΔV/Δr

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13
Q

what is Kepler’s 3rd law?

A

r³ ∝ T³
r = average radius of orbit
T = time period for orbit

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14
Q

what is Newton’s law of gravitation?

A

the gravitational force F between two point masses m₁ and m₂ at a distance r apart is given by:
F = Gm₁m₂ / r²

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15
Q

what is G?

A

the universal constant of gravitation

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16
Q

what is a formula for g using Newton’s law of gravitation?

A

g = GM / r²

17
Q

how does g vary with distance from the centre of a spherical planet?

A

follows the inverse square law

18
Q

what is escape velocity?

A

the minimum velocity an object must be given to escape from the planet when projected vertically from the surface

19
Q

how do you derive the escape velocity formula?

A
  • substitute V = -GM/r into W = mV
  • equate Eₖ = 1/2(mv²) to W = mV
  • Rearrange to make v the subject
20
Q

what is a formula for gravitational potential?

A

V = - GM/r

21
Q

How can you prove Kepler’s third law by using Newton’s law of gravitation?

A
  • g = GM/r² and g = v²/r (centripetal acceleration)
  • equate these and v² = GM/r
  • v = 2𝜋r / T
  • so, (2𝜋r)² / T² = GM / r
  • rearrange, r³/T² = GM/4𝜋²
22
Q

what are geostationary satellites?

A

orbits the earth directly above the equator and has a time period of exactly 24 hours.
This means it remains in a fixed position above the equator

23
Q

what is the total energy of a satellite?

A

E = gravitational potential energy + kinetic energy