Physics 5.4 Gravitational fields Flashcards

1
Q

Define gravitational fields and what do gravitational field lines show?

A

-Gravitational fields: a vector quantity, it is the region around a body in which other bodies will feel a force due to the mass of the body
-Gravitational field lines show the shape of the field and direction

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2
Q

What is gravitational field strength?

A

-Gravitational field strength at any point is the force per unit mass at that point. Units are Nkg^-1

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3
Q

Why does the gravitational field strength of the earth vary at the surface?

A

-Matter is not evenly distributed across the earth, for example water is less dense than rock, so gravitational force can vary slightly

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4
Q

What is the value of the gravitational field strength of the earth at its surface?

A

9.81 NKg^-1

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5
Q

Define Newtons 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 separation

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6
Q

What is the equation for Newtons law of gravitation?

A

-Where M and m are the masses of the bodies
-R is the separation of their centres
-G is the universal gravitational constant

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7
Q

What is the value of the universal gravitational constant?

A
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8
Q

Describe the gravitational field lines of a spherically symmetric mass?

A

-The gravitational field lines act radially towards the centre

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9
Q

What is the equation for gravitational force of a spherical or point object?

A

Where G is universal gravitational constant, M is mass of body and r is the radius of the mass

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10
Q

What is an equation for the gravitational field strength of the earth as height(h) above the earths surface increases

A

G-universal gravitational constant
R-radius of earth
H- height above earths surface
M-mass of earth

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11
Q

What are the definitions of Keplers third law and geostationary orbirt?

A

-Keplers third law: states that the square of the time period of a planet orbiting a sun is proportional to the mean radius of its orbit cubed
-Geostationary orbit: a sattelite that has the same time period and orbital rotation as the earth (24hours) so is in equatorial plane

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12
Q

What are keplers three laws describing 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 (explained in picture)
  3. The time period of the orbit squared is proportional to the mean radius of the orbit cubed
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13
Q

What is the equations for Keplers third law?

A

T-time period
R-mean radius of orbit
G-universal gravitational constant
M-mass of larger mass

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14
Q

What is an example of what geostationary satellites are used for?

A

-Monitiring air traffic, weather and changes in environment

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15
Q

Define gravitational potential and escape velocity?

A

-Gravitational potential: at a point in a gravitational field, is defined as the work done in moving unit mass from infinity to that point. Unit is Jkg^-1
-Escape velocity: from a point in a gravitational field, is the minimum launch velocity required to move the object from that point to infinity

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16
Q

What is the equation for escape velocity?

A

V-escape velocity
G-universal gravitational constant
M-mass of body
r-radius