Gravitational Fields Flashcards

1
Q

Define Gravitational Field

A

A region where an object that has mass, experiences a force

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2
Q

State newton’s law of gravitation and state equation it comes from

A

Attractive forces between two point masses is directly proportional to the product of their masses and inversely proportional to the square of their seperation
F=GMm/r^2

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3
Q

Define Gravitational Field strength and state the equation it comes from

A

Force acting on a body per unit mass
G=F/m

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4
Q

Equations for potential energy for uniform and radial field and define potential energy

A

Uniform, Ep=mgh
Radial = (Gm1m2)/r
Work done in moving object with mass from infinity to that point in the field

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5
Q

Define absolute Gravitational potential energy

A

Work done per unit mass in moving a body from infinity to that point in Gravitational Field
V=GM/r
Work done = m x V

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6
Q

Derive two equations to show Kepler’s 3rd Law

A
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7
Q

Derive two equations for equation of orbital velocity

A
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8
Q

Derive two equations to get equation for escape velocity

A
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9
Q

Derive two equations for total orbital energy

A
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10
Q

State times for Low earth orbit (LEO), Medium earth orbit (MEO), High earth orbit (HEO)

A

LEO : less than 2 hours
MEO : More than 2 hours and less than 24 hours
HEO : greater than 24 hours

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11
Q

Similarity and difference between geostationary and geoschrynous orbits, state advantage of geostationary

A

Similarity : time period of 24 hours
Differnce : geostationary orbits above same point Earth’s equator
Geoschrynous orbit do not stay above same points of Earth’s surface
Advantage : easier to track

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12
Q

State uses of geostationary orbits
State a little explanation

A

Monitoring weather : whole earth may be scanned
GPS : several satellites needed to fix position on earth
Communications : limited by intermittent contact

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13
Q

Problem of putting more satellites in orbit

A

Satellites orbit in closer proximity
Greater risk of collisions

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14
Q

What is meant by satellites in polar orbits
State uses

A

Satelite passes over north and south poles
Making them ideal for espionage (spying on other countries)

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15
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16
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17
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18
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19
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20
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21
Q
A

A

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22
Q
A

Speed = distance / time
Distance = 2.04 x 10^7
Can’t use Kepler’s third law as that gives the orbital of the earth, so your radius would just be equal to radius of earth

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23
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24
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25
Q
A

D

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26
Q
A

A

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27
Q
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28
Q

which one has different units to the other 3
a) gravitational potential
b) gravitational field strength
c) force per unit mass
d) gravitational potetnial gradient

29
Q

State what is meant by terminal velocity

A

Minimum speed at the Earth’s surface that will allow an object to leave

30
Q

State two reasons why a rocket does not need the escape velocity to leave the Earth’s surface

A
  • they aren’t given all their Kinetic energy at the Earth’s surface as energy is continually added in the flight
  • less energy needed to achieve orbit than to escape from Earth’s gravitational field
31
Q

Explain why all potential energy values are negative

A

Zero potential at infinity
Energy input needed to move to infinity
Work done by Field moving object from infinity

33
Q

Explain how change in potential energy relates to kinetic energy when satellites orbit alters

A

Loss of gpe is twice gain in kenetic energy

34
Q

Skip first part calculating force

35
Q

Explain why astronauts in an orbiting space vehicle experience the sensation of weightlessness

A

Both astronaut and vehicle are traveling at the same orbital speed
They have the same centripetal acceleration / they are in freefall
No normal reaction between astronaut and vehicle

36
Q

Explain what is meant by Gravitational potential in at a point in Gravitational Field

A

Work done against the field per unit mass
When moved from infinity to the point

37
Q

-63 equals gravitational potential at the surface of the earth

38
Q

State two features of a geo-sychronous orbit

A

Period is 24 hours
Remains in fixed position relative to surface of earth
Same angular speed as earth
Equatorial orbit

39
Q
A

Signal would be to weak at a large distance
Signal spreads out more further it travels making detection and transmission and less effective

41
Q

If you have been asked to calculate the gravitational force between two objects and they say calculate the force when the seperation changes, what must you remember to do and not do

44
Q

State what is represented by Gravitational field lines

A

Direction and magnitude of force on mass placed in the force field

45
Q
A

Lines are closer together so field is stronger
Material forming the Earth at K has a higher density than the surrounding material

46
Q

Only 6.3

A

Ball will speed up / accelerates when moving towards K because potential at K is lower

47
Q

In a gravitational field should lines point away or towards object

A

Towards object, if a ay then it is not a gravitational field

48
Q

Only 6.6

A

Should be at right angles and sop and bottom should be symmetrical

52
Q

The Moonís orbit around the Earth may be assumed to be circular. Explain why no work is done
by the gravitational force that acts on the Moon to keep it in orbit around the Earth.

A

work = force × distance moved in direction of force
(in circular motion) force is perpendicular to displacement
no movement in direction of force hence no work

53
Q

Define Gravitational potential difference

A

The energy needed to move a unit mass between two points in a Gravitational Field

54
Q

What is an equipotential surface

A

A surface in which the potential is constant at every point

55
Q

How are equipotential surfaces found

A

Through joining points off equal potential together to map out a surface