Gravitational Fields Flashcards

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1
Q

what is a gravitational field?

A

a gravitational field is the region around a body in which other bodies will feel a force due to the mass of the body

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2
Q

what do gravitational field lines show?

A

the shape and direction of the field line at a point is the direction in which a small mass would move when placed at that point

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3
Q

what is gravitational field strength?

A

the gravitational field strength at any point in a gravitational field is the force acting per unit mass at that point, g = F / m (units are NKg^-1)

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4
Q

how do gravitational field lines act around a spherical mass?

A

they act radially inwards, towards the centre because spherical objects can be modelled as a point mass at its centre

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5
Q

what are gravitational field caused by?

A

they occur because objects have mass, the more mass that body has, the more that it will attract the smaller masses around it

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6
Q

what happens to the field lines of Earth as you get closer and closer to the surface of the Earth?

A

the gravitational field lines become uniform and straight, the lines converge to become almost parallel, the radial field becomes apparent the further we move away from the Earth and observe it from space

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7
Q

state Newton’s law of gravitation?

A

Newton’s law of gravitation states that the gravitational force of attraction between two point masses is directly proportional to the product of their masses and inversely proportional to the square of their separation

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8
Q

what is the equation for Newton’s law of gravitation?

A

F = - GMm / r^2
where M and m are the masses of the two bodies and r is the separation of their centres
(the minus shows it is an attractive force as bound)

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9
Q

what is G?

A

the universal gravitational constant, 6.67 x 10^-11

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10
Q

what law does Newton’s law of gravitation follow in terms of force? (think of intensity)

A

follows an inverse square law, forces gets smaller with distance because the strength changes

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11
Q

a spherical mass is often assumed to be what?

A

a point mass with all its mass concentrated at the centre

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12
Q

what is the other equation for gravitational field strength for a point mass and how can you get to it?

A

first g = F / m
F = - GMm / r^2, equate Fs
leading to g = - GMm / mr^2, cancel little m
leading to g = - GM / r^2

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13
Q

what is gravitational field strength equal to on earth?

A

g = 9.81 ms^-2 (acceleration due to freefall)

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14
Q

what are Kepler’s free laws of planetary motion?

A
  1. planets travel around the sun in elliptical orbits
  2. a line joining the Sun to a planet will sweep out equal areas in equal times
  3. the time period of the orbit squared is proportional to the mean radius of the orbit cubed, or T^2 ∝ r^3
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15
Q

what are Kepler’s free laws of planetary motion?

A
  1. planets travel around the sun in elliptical orbits
  2. a line joining the Sun to a planet will sweep out equal areas in equal times
  3. the time period of the orbit squared is proportional to the mean radius of the orbit cubed, or T^2 ∝ r^3
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16
Q

what is Kepler’s third law?

A

kepler’s third law states that the square of the period of a planet orbiting the Sun is proportional to the mean radius of its orbit cubed (his law also applies to other planetary stems, to the orbits of moons around planets and to binary stars)

17
Q

what is a geostationary orbit?

A

a geostationary orbit is an orbit of the Earth made by a satellite that has the same time period and orbital direction as the rotation of the Earth (i.e 24 hours) and is in the equatorial plane

18
Q

what are geostationary satellites used for?

A

geostationary satellites are used for communication. eg. TV and mobile phones

19
Q

what are polar orbiting satellites

A

polar orbiting satellites orbit over the poles from North to South, such that the Earth rotates West to East under them to provide a complete image of the Earth

20
Q

what are polar orbiting satellites used for

A

polar orbiting satelites are used for mapping and reconnaissance

21
Q

what are low earth orbits

A

low earth orbits take less than 2 hours to orbit the earth. eg. ISS

22
Q

what is the equation that relates time period to mean radius (kepler’s third law)?

A

T^2 = (4π^2 / GM ) x r^3. derived from F=(mv^2)/r=GMm/(r^2)

23
Q

what is gravitational potential?

A

work done per unit mass to move an object from infinity to the given point./ always negative as bound in field

24
Q

what is gravitational potential energy?

A

energy needed to get from distance r to infinity. always negative as bound

25
Q

what is escape velocity?

A

the velocity needed for an object to escape the gravitational field of a body

26
Q

what is the radius of a black hole?

A

the Schwarzschild radius - the minimum radius that allows a proton (velocity=c) to escape a body of mass M