Gravitiational Fields Flashcards

1
Q

What is a gravitational force

A

A force of attraction that acts between objects with mass

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2
Q

Define Newton’s Law of Gravitation

A

The gravitational force between 2 masses is directly proportional to the product of the masses and inversely proportional to the square of the distance between them

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3
Q

What is a uniform gravitational field

A

A field that exerts the same gravitational force on a mass anywhere in the field

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4
Q

What is a radial field

A

A field in which the force exerted depends on an objects position in the field. Decreases as the distance from the centre increases

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5
Q

Define Gravitational Field Strength

A

The force per unit mass exerted by a gravitational field on an object.

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6
Q

How does Gravitational field strength vary in a uniform and radial field

A

Uniform - Always the same Radial - Varies with distance

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7
Q

Define Gravitational potential at a point

A

The work done per unit mass when moving an object from infinity to that point.

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8
Q

Why is Gravitational potential always negative

A

Gravitational potential at infinity is zero, and as an object moves from infinity to a point, energy is released as the gravitational potential energy is reduced

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9
Q

Define Gravitational Potential Difference

A

The energy needed to move a unit mass between to points

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10
Q

What is an equipotential surface

A

Surfaces which are created through joining points of equal potential together, therefore the potential on an equipotential surface is constant everywhere.

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11
Q

What is the relationship between gravitational potential and distance between the centre of masses

A
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12
Q

What is the gradient of a V-r graph

A

Gravitational field strength x -1

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13
Q

What is the area under a g-r graph

A

Gravitational potential difference

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14
Q

What is Keplers 3rd Law and the equation

A

T<strong>2</strong> is proportional to r3

T2 = r3 x 4π2/GM

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15
Q

Describe the context that Keplers 3rd law should be used

A

An object orbiting a body

M = Mass of the body being orbited

r = Dist. between the object and the centre of the body being orbitted

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16
Q

What is the derivation for Keplers 3rd Law

A

When an object orbits a mass in circular motion, the gravitational force acts as the centripetal (resultant) force

mv2/r = GMm/r2 , mv2 = GMm/r , v2=GM/r

Since v=d/t, let d be the circumference = 2πr

v=2πr/T , v2=4π2r2/T2

Equate the 2 equations

2r2/T2=GM/r

T2=4π2r3/GM

17
Q

What is the total energy of a satellite in orbit

A

Sum of Kinetic Energy and Potential Energy

18
Q

How do the energy stores in an orbiting satellite change

A

Total energy is constant

i.e If it orbits at a lower height, Potential energy falls, so Kinetic energy increases to keep total energy constant

19
Q

What is escape velocity

A

The minimum velocity an object must travel at in order to escape the gravitational field at the surface of a mass, when it is projected vertically from the surface

When Ek=Ep

As Ep is the energy required for an object to leave a field, so when its Ek is high enough, it has enough energy to transfer.

20
Q

How to calculate escape velocity

A

When Ek=Ep

v = (2GM/r)½

M= Mass of larger mass

21
Q

What is a synchronous orbit

A

Where the orbital period is equal to the rotational period of the object it’s orbitting

22
Q

What is a geostationary Satellite

What can they be used for

A

A satellite that follows a geosynchronous orbit

Always stays above the same point as they orbit directly above the equator

Used in TV/telephone signals as its position never changes

23
Q

What is a low orbit satellite, what are they used for

A

A satellite with a much lower and faster orbit

Can orbit the entire earth

Used for military, weather, scientific purposes

24
Q

What is the relationship between Gravitational Field Strength and Potential Gradient

A

Gravitational Field Strength = -Potential Gradient

As potential gradient is how much energy a 1kg mass would transfer to move 1m further. This is the work done against the attractive gravitational force, which is facing the opposite direction.

That attractive gravitational force for the 1kg mass is just the gravitational field strength