18 : Gravitational fields Flashcards

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1
Q

What is gravity

A

Gravity is the universal attractive fore which acts between all matter

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2
Q

What is G

A

The universal gravitational constant

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3
Q

What can field lines tell you

A

The direction and strength of the field depending 9n the density of the field lines

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4
Q

What is g

A
  • his the force per unit area in a uniform gravitational field
  • in a radial field the magnitude of g is the proportionality constant at that between force and mass
  • g = GM/r^2
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5
Q

Newtons law of gravitation

A

States that two point masses attract each other with a force that is directly proportional to the product of their masses and inversely proportional too the square of the distance between them

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6
Q

Keplers first law

A

The orbit of a plant is an ellipse with the sun at one of the foci- the eccentricity f the ellipse is very low so the notion can be modelled as circular

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7
Q

Keplers second law

A

A line segment joining a planet and the sun sweeps out equal areas during intervals of equal time
- the speed of the planet isn’t constant as it moves faster closer to the sun

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8
Q

Keplers third law

A

The square of the orbital period T is proportional to the cube of the average distance r from the sun
- this can be proved with forces acting on planet - centripetal force is required to keep planet in orbit and this force is provided by gravitational field of the sun

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9
Q

Derive equation to show T^2 is proportional to r^3

A
  • Keplers third law = mv^2/r = GMm/r
  • rearrange to get v^2 = GM/r
  • velocity in circular motion is 2πr/T
  • substitute in and rearrange to get T^2 as subject
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10
Q

What are satellites

A

Are objects that orbit other, large objects these include natural satellites such as moons and articulated satellites that humans have sent into space

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11
Q

Uses of satellites

A

Communications, scientific research and global positioning systems

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12
Q

What are Geostationary satellites

A

Have an orbital period that is exactly a day so day appear stationary above the earth
- orbit 36000km above the equator

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13
Q

Uses of geostationary satellites

A

Communications and surveying as the provide continuous coverage

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14
Q

Gravitational potential

A

The potential energy per kilogram, at any point in the field
- 0 potential is defined at infinity as at a point close to a mass the potential energy is negative as its an attractive force

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15
Q

What is Gravitational potential difference

A

The difference in gravitational potentials of two points in a gravitational field

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16
Q

What is gravitational potential energy at a point in the field

A

The work done per unit mass is moving object from infinity to that point in the field

17
Q

What is escape velocity

A

The minimum velocity an object requires in order to escape the gravitational field of an object when projected vertically form its surface
- formula derived from equating kinetic energy and gravitational potential energy required to reach infinity
- 1/2 mv^2 = GMm/r