Chapter 7: Gravitational Field Flashcards

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1
Q

State Newton’s Law of Gravitation

A

Two point masses attract each other with a force that is directly proportional to the product of their masses and inversely proportional to the square of the distance between them

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2
Q

What is a gravitational field?

A

It is a region of space where a mass experiences a force due to the presence of another mass

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3
Q

Define gravitational field strength

A

It is the gravitational force per unit mass acting on a test mass at that point

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4
Q

What is a geostationary orbit?

A

It is a circular orbit around the Earth that appears stationary to observers on Earth’s surface

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5
Q

What are the features of geostationary satellites?

A
  1. Located at the same height above Earth’s surface, directly above the equator
  2. All geostationary satellites have the same linear speed v
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6
Q

What is a polar orbit?

A

Satellites orbit about a plane containing the North and South poles, and the centre of the Earth

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7
Q

Define gravitational potential at a point

A

It is the work done per unit mass needed by an external agent to bring a test mass from infinity to that point (without a change in KE)

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8
Q

Why is gravitational potential always negative

A
  • The gravitational potential at infinity is zero
  • Gravitational pull is attractive in nature
  • The external force must be equal in magnitude and opposite in direction to gravitational pull such that there is not change in KE
  • Since the direction of external force is opposite to the displacement of the mass (positive), gravitational potential is negative
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9
Q

Define gravitational potential energy

A

It is the work done by an external agent in bringing a test mass from infinity to that point (without a change in KE)

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10
Q

Graphically, what is gravitational force equal to?

A

It is equal to the negative gravitational potential energy gradient (-dU/dt)

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11
Q

Graphically, what is gravitational field strength equal to?

A

It is equal to the negative gravitational potential gradient

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12
Q

Define escape speed

A

It is the speed required for a body to escape a gravitational field

v = sqrt(2GM/R) = sqrt(2gR)

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13
Q

How is orbital period related to orbital radius?

A

T^2

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