Gravitational Fields F01-05 Flashcards

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1
Q

Describe Newton’s law
of gravitation?

A

The force of attraction that is directly proportional to the product of the two masses, and inversely proportional to the distance between the two centres squared.

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2
Q

Define ‘gravitational field strength’

A

The force per unit mass felt by a small test object at any point within that field.

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3
Q

Is field strength a scalar or a vector?

A

Vector.

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4
Q

Units of field strength?

A

N kg^-1

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5
Q

Define ‘gravitational potential’

A

The work done PER UNIT MASS to bring an object from infinity to that point.

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6
Q

Is potential a scalar or vector?

A

Scalar.

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7
Q

Units of potential?

A

J kg^-1

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8
Q

Draw the field lines in a radial field.

A

Circular centre with arrows all going towards to the centre of the circle.

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9
Q

Draw the equipotentials in a radial field

A

A dotted circle around the circle centre in a circle shape.

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10
Q

Draw the field lines in a uniform field.

A

Parallel lines pointing towards the ground/downwards.

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11
Q

Draw the equipotentials in a uniform field.

A

Dotted lines perpendicular to the direction of the force field.

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12
Q

How do the field lines indicate field strength?

A

The closer the lines are together the stronger the field is.

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13
Q

What is the angle between equipotentials and field lines?

A

Perpendicular to the direction of the field lines so 90 degrees.

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14
Q

What is the graph of the field strength against distance?

A

A typical y = 1/x graph

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15
Q

What is the graph of the potential against distance?

A

r shaped curve starting in the bottom right quadrant away from the y axis, at the radius of sphere, ending at the surface of the next object or the total distance.

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16
Q

How can we find the work done moving between points from a g vs r graph?

A

Work done is the area under the graph

17
Q

How can we find the field strength from a V vs r graph?

A

Finding the gradient = -(V/r)

18
Q

Show that T² ∝R³ (Kepler’s law)?

A

F = Gm1m2/r^2
F = mv^2/r
GMm/r^2 = mv^2/r
From above derive… v = (GM/r)^1/2
v = 2pir/T
T = 2pir/v
T = 2pir/(GM/r)^1/2
T = (4pi^2r^3/GM)^1/2
Therefore T^2 = 4pi^2r^3/GM
Therefore T² ∝R³

19
Q

Describe Newton’s law
of gravitation formula?

A

F = (Gm1m2)/(r^2)

20
Q

What is the value of the gravitational potential at infinity?

A

As r tends to infinity, 0.

21
Q

What are equipotential lines?

A

Definition: Join points of equal potential.
Orientation: at 90 degrees to the direction of the field lines.
Spacing: are closer in stronger in stronger fields.

22
Q

Is there work done along equipotential lines?

A

No work done is moving along an equipotential lines.

23
Q

What is a geostationary/geosynchronous satellite?

A

Time period is 24 hours.
Stays above the same point on the earth.
Cannot see the poles, (only up to 70 degrees above the equator).

24
Q

What is a Low orbit (Polar) satellite?

A

Over the poles.
This way a satellite can cover the whole earth as the earth rotates.
Short time period, around 90 minutes.

25
Q

How to calculate the total GFS?

A

g(T) = g(1) - g(2)
g(1) > g(2)

26
Q

How to calculate the total Gravitational Potential?

A

V(T) = V(1) + V(2)

27
Q

What is the equation relating work done, mass and gravitational potential?

A

W = mV
W = m(V(orbit) - V(surface))

28
Q

What are the uses for geostationary/geosynchronous satellite?

A

Communications

29
Q

What are the uses for Low orbit (Polar) satellite?

A

Military
Scientific
Weather
GPS

30
Q

What are the energy considerations for an object in orbit?

A

Total energy = KE + GPE (negative)
If total < 0, then stays in orbit.
If total > 0, then will escape orbit.
(KE > GPE)