D1 Gravitational Fields Flashcards

1
Q

What is a gravitational field?

A

A region of space surrounding a body in which another body experiences a gravitational force due to their masses.

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2
Q

Gravitational force formula

A

F = GMm/r2

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3
Q

How are the field lines directed in a gravitational field near the Earth’s surface?

A

Parallel and equally spaced.

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4
Q

How are field lines directed over large distances from the Earth’s surface

A

Radially towards the earth’s centre
Weakens with distance

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5
Q

What does Newton’s law of gravitation state?

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 their separation.

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6
Q

What is the nature of the forces described by Newton’s universal law of gravitation?

A

Always attractive.

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7
Q

What is gravitational field strength (g)?

A

The gravitational force exerted per unit mass on a small mass placed at that point.

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8
Q

Gravitational field strength formula

A

g = F/m = GM/r2

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9
Q

In a gravitational field, what is the relationship of gravitational field strength (g) inside the Earth?

A

g is directly proportional to distance r from the center.

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10
Q

What is Kepler’s First Law?

A

Planetary orbits are elliptical with a star (the Sun) at a focus.

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11
Q

What does Kepler’s Second Law state?

A

The radius vector from the star (the Sun) to the orbiting body sweeps equal areas in equal times.

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12
Q

What is Kepler’s Third Law

A

GMm/r2 = mRw2 (okay actually it’s the relationship between period and radius but I want to remember this so)

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13
Q

What is the gravitational potential energy (Ep) of a point mass in a gravitational field?

A

The work done by an external agent in bringing the point mass from infinity to that point.

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14
Q

What does the negative sign in gravitational potential energy (Ep) indicate?

A

It means that Ep is always negative and has values less than zero.

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15
Q

What is escape velocity?

A

The minimum speed an object must have at the start to just escape from the gravitational influence of a body.

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16
Q

Formula for escape velocity

A

v esc = √(2GM/r)

17
Q

Fill in the blank: The gravitational force acting on each of two masses is ______ and ______.

A

equal and opposite (By Newton’s 3rd Law)

18
Q

By Kepler’s Third Law, what is the relationship between T and R

T (period of rotation); R (radius of orbit)

A

T squared is directly proportional to R cubed

19
Q

What is the significance of the neutral point in the interaction of two gravitational fields?

A

Gravitational field strength (g) is zero (but not potential)
Gravitational force due to each of two masses on a small mass placed at that point is equal to

20
Q

Fill in the blank: Neutral point is always closer to the _ mass

21
Q

What happens to gravitational potential energy as a point mass is moved toward infinity?

A

Ep approaches zero.

22
Q

Gravitational potential energy formula

A

Ep = -G(Mm/r).

23
Q

Gravitational potential formula

A

Vg = -Gm/r

24
Q

What is the total energy of a body in an orbit?

A

Total mechanical energy = KE + PE

25
What is gravitational potential?
Gravitational potential, Vg, at a point is the **work done per unit mass** by an external agent in bringing a small test mass **from infinity** to that point. ## Footnote This definition emphasizes the relationship between gravitational fields and energy.
26
True or False: Gravitational potential is a vector quantity.
False ## Footnote Gravitational potential is a scalar quantity.
27
What happens to gravitational potential as one moves further from a mass?
g becomes less negative and approaches 0 ## Footnote At infinity, gravitational potential is conventionally taken to be zero.
28
What does the gradient of a Ep - distance graph represent?
Gravitational force, F
29
What does the gradient of a Vg - r graph represent?
Gravitational field strength, g
30
What is the significance of equipotential curves?
Equipotential curves indicate points in a gravitational field where the potential is constant. ## Footnote They are useful in visualizing gravitational forces and energy distribution.
31
What happens to the total mechanical energy of a satellite when it changes orbital radius?
Radius increase - increase energy Radius decrease - decrease energy
32
How to calculate work done to move a mass in a gravitational field?
W = m∆Vg ## Footnote This relates to the concept of energy conservation in gravitational fields.
33
Orbital velocity formula
v orbital = √(GM/r)
34
Orbital KE formula
GMm/2r