Orbits of planets and satellites Flashcards

1
Q

Kepler’s third law

A

the square of the orbital period (T) is directly proportional to the cube
of the radius (r)

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2
Q

what happens when an object orbits a mass?

A

it experiences a gravitational force towards the centre of the
mass, and as the object is moving in a circle, this gravitational force acts as the centripetal
force

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3
Q

What is the total energy of an orbiting satellite made up of?

A
  • its kinetic and potential energy, and is
    constant.
  • For example, if the height of a satellite is decreased, its gravitational potential energy will
    decrease, however it will travel at a higher speed meaning kinetic energy increases, therefore total
    energy is always kept constant.
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4
Q

equation of Total energy of a satellite v

A

Total energy of a satellite = kinetic energy + potential energy

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5
Q

escape velocity

A

is the minimum velocity it must travel at, in order to escape
the gravitational field at the surface of a mass. This is the velocity at which the object’s kinetic
energy is equal to the magnitude of its gravitational potential energy.

  • Ek = Ep, Ep is GMm/r
  • rearrange to get V which is escape velocity
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6
Q

synchronous orbit

A
  • one where the orbital period of the satellite is equal to the rotational
    period of the object that it is orbiting,
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7
Q

Geostationary satellites

A

follow a specific geosynchronous orbit, meaning their orbital period is 24
hours and they always stay above the same point on the Earth, because they orbit directly
above the equator.

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8
Q

Why are geostationary satellites useful

A

for sending TV and telephone
signals because it is always above the same point on the Earth so you don’t have to alter the
plane of an aerial or transmitter.

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9
Q

how to find orbital radius?

A

you use this equation : T^2 = 4π^2/GM x r^3

  • rearrange for r to get the orbital radius
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10
Q

Low-orbit satellites

A
  • have significantly lower orbits in comparison to geostationary satellites,
    therefore they travel much faster meaning their orbital periods are much smaller.
  • Because of this, these satellites require
    less powerful transmitters and can potentially orbit across the entire
    Earth’s surface. ( this is why they are useful)
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11
Q

what are low-orbit satellites useful for ?

A
  • monitoring the weather
  • making scientific
  • observations about places which are unreachable and military applications.
  • They can also be
    used for communications but because they travel so quickly, many satellites must work together to
    allow constant coverage for a certain region.
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12
Q

Kepler third law deriviation

A

1) set equal the Centripetal force equation to the Gravitational force equation
2) Rearrange the equation to make v^2 the subject.
3)use v = 2πr/T and square the equation to get v^2 = 4π^2 r ^2 / T^2
4) set num 3 equation to num 2 equation
5)Rearrange to make T² the subject
6) As 4π2/GM is a constant, this shows that T^2 ∝ r^3

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13
Q

Compare the PE and KE of a lower orbit to a higher one

A

A lower orbit (smaller m ) has less potential energy and more kinetic energy than a higher orbit ( bigger r )

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