3.7.2 Gravitational Fields Flashcards

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1
Q

what is gravity

A

a universal attractive force acting between all matter

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2
Q

what does the gravitational force depend on

A

the mass of the two objects and the distance between them

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3
Q

what is gravitational force (equation)

A

F = G m1 m2 / r2

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4
Q

what is gravitational fields represented by

A

field lines

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5
Q

what is gravitational field strength, g , the same as

A

acceleration due to gravity

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6
Q

what is gravitational field strength

A

gravitational force on the object / mass of the object

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7
Q

what is gravitational potential energy

A

GPE = the energy an object has when lifted off the ground

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8
Q

what is the GPE outside the earth’s surface

A

the energy an object possesses due to its position in a gravitational field

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9
Q

what is gravitational potential at a point

A

the gravitational potential energy per unit mass at that point

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10
Q

what is gravitational potential

A

the work done per unit mass in bringing a test mass from infinity to a defined point

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11
Q

what is the zero value of gravitational potentials

A

an infinite distance away from the mass generating that field

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12
Q

what happens if an object moves along an equipotential surface

A

the potential has not changed and no work has been done on the object

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13
Q

why is gravitational potential shown with a negative sign

A

the gravitational potential is trying to do the opposite of what gravity wants

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14
Q

what is an orbital period

A

the time taken for an object to do one full orbit

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15
Q

what is the orbital radius

A

the average distance between the centre of the body and the centre of the object, for a circle this is constant, but changes for an elliptical orbit.

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16
Q

what is the relationship between orbital period and radius (Kepler’s third law)

A

T^2 ∝ r^3

17
Q

what happens in a circular orbit

A

in a circular orbit around a planet, the satellite is always on the same equipotential and so the total energy of an orbiting satellite is constant

18
Q

what is escape velocity

A

the velocity needed for an object to escape a planets gravitational pull

19
Q

what happens (to energy) when an object is removed from a planets gravitational pull

A

it loses KE equal to the GPE it gains

20
Q

what is the orbital period of a geosynchronous orbit

A

one day

21
Q

what are geostationary orbits

A

appear stationary above the equator

22
Q

what are the requirements for a geostationary orbit

A

circle earth above the equator
zero eccentricity (zero deviance form orbit)
zero inclination (zero change in angle between the planes)
west-east
same rate as earth

23
Q

what are the uses of geostationary orbits

A

meteorological
communication

24
Q

why are geostationary orbits used for satellites

A

satellites view the earth from the same perspective and can provide global coverage

25
Q

what are polar orbits

A

a low earth orbit that pass above or near the earths poles and has a high inclination angle

26
Q

what are the requirements for a polar orbit

A

low altitudes (200-1000km)
north-south
orbit time about 100 mins
inclination about 90 degrees to equator
speed about 7.5 km/s

27
Q

what are the uses of polar orbits

A

earth observation

28
Q

why are polar orbit satellites used

A

satellites can view entire earth’s surface multiples times a day
allows scientific research to study earth’s atmosphere, oceans and land cover
natural disasters can be monitored and the collection of long term data