Gravitational Fields Flashcards

Newton's law of gravitation, gravitational field strength, gravitational potential, satellites, energy of satellites, geostationary satellites.

1
Q

State Newton’s law of gravitation.

A

Two point masses attract each other with a force that is proportional to the product of the masses and inversely proportional to the square of their separation.

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2
Q

Formula for Newton’s law of gravitation.

A

Check notes.

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3
Q

What is a gravitational field?

A

Region of space where a mass experiences a force.

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4
Q

Define gravitational field strength.

A

Force per unit mass acting on a mass placed at that point.

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5
Q

Formulae for gravitational field strength.

A

Check notes.

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6
Q

Derive the equation for the gravitational field strength of a point mass

A

Check notes.

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7
Q

On the surface of the Earth, gravitational field strength is also called ________.

A

the acceleration of free fall.

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8
Q

For an object in a circular orbit around a planet, what provides the centripetal force?

A

Gravitational force.

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9
Q

Show that T squared is proportional to R cubed, where T is the period of orbit of Earth and R is the radius of orbit.

A

Check notes.

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10
Q

What are the features of a geostationary satellite?

A

(a) its period of rotation is 24 hours (it orbits the Earth once every 24 hours)
(b) the satellite rotates from west to east
(c) its orbit is directly above the Equator

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11
Q

A ‘feeling’ of weightlessness occurs when __________ .

A

the only force acting on the body is gravitational force.

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12
Q

Define gravitational potential.

A

Work done per unit mass in moving a mass from infinity to the point.

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13
Q

Define gravitational potential energy.

A

Work done in moving a mass from infinity to the point.

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14
Q

Gravitational potential energy is always negative. Explain why.

A

The gravitational force between two masses is always attractive. Hence, to move a mass m from infinity towards another mass M, work is done by the gravitational force, ie. work done by the external force is negative, and the gravitational potential energy Ep decreases. Therefore, masses closer than infinity has negative amount of Ep (relative to ∞ ).

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15
Q

Recall the formula for gravitational potential energy.

A

Check notes.
Ep = ϕ x m
ΔEp = Δ ϕ x m

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16
Q

State the relationship between gravitational field strength and gravitational potential.

A

The gravitational field strength is equal to the negative of potential gradient.

17
Q

The gravitational field strength is equal to the negative of potential gradient.
What does the minus sign indicate?

A

The minus sign indicates that g is in the direction of decreasing potential.

18
Q

An object is orbiting round the Earth with speed v. How do we find an expression for v?

A

Centripetal force is provided by gravitational force.

Check notes for the rest of the working.

19
Q

Deduce the equation for kinetic energy of a satellite.

A

Centripetal force is provided by gravitational force.

Check notes.

20
Q

Deduce the equation for total energy of a satellite.

A

The total energy of the satellite is the sum of kinetic energy and potential energy of satellite.
Check notes for working.

21
Q

What is meant by the escape speed of a mass?

A

The escape speed is the minimum speed needed to project a mass m from the surface of a planet to infinity.

22
Q

How do you find the escape speed of a mass?

A

loss in kinetic energy = gain in potential energy
Ek on surface – Ek at infinity
= Ep at infinity – Ep on surface
Check notes for working.