Year 2- Gravitational Fields Flashcards

1
Q

what do all objects with a mass exert

A

a gravitational force on each other

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2
Q

what is the gravitational force a mass experiences near the surface of a planet or moon

A

weight

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3
Q

what is the equation for weight

A

W = mg

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4
Q

what is the gravitational force proportional to when 2 masses are involved

A

directly proportional to the product of the 2 masses, and inversely proportional to the distance between the two centres squared

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5
Q

how can we assume an object can act like a point mass

A

if it is spherical and has uniform density

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6
Q

define point mass

A

the object acts like all the mass is concentrated in the centre

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7
Q

when dealing with masses in a gravitational field, what is assumed

A

all the masses are point masses

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8
Q

what are all masses surrounded by

A

a gravitational field

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9
Q

where will all masses feel a force

A

in the gravitational field

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10
Q

what is gravitational field strength

A

the gravitational force per unit mass a mass will experience in a field

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11
Q

what is the source of a gravitational field called

A

a source mass

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12
Q

how can we test the field due to a source mass

A

using a test mass

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13
Q

what is a test mass

A

a small enough mass that won’t effect the field

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14
Q

is gravitational field strength vector or scalar

A

vector, with the direction towards the source mass

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15
Q

define gravitational field strength in terms of the equation

A

gravitational field strength is directly proportional to the mass of the source mass, and indirectly proportional to the distance between the centre of the test mass and source mass squared

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16
Q

how can the gravitational field strength be represented

A

-with vectors pointing in the direction of the field, with different lengths of the vectors representing different field strengths
-with field lines pointing in the direction of the field, and the distance between the field lines representing different field strengths

17
Q

what is the shape of field lines around a spherical mass

18
Q

what does a radial field represent in terms of gravitational field strength

A

it decreases as you get further from the centre point mass

19
Q

how can we represent the gravitational field close to the surface and what does it mean

A

as a uniform field, therefore g is a constant

20
Q

how do you differentiate between what equation to use for the force

A

w=mg for when the mass is close to a planet
f=gmm/r^2 for when the distance is a lot greater (where g would not be a contstant)

21
Q

how can you find the point between two masses where their each individual fields cancel out

22
Q

how can you find the direction/ force of a point in 2 gravitational fields

A

find the resultant force vector

23
Q

what does the graph of g against r look for a point mass

A

a decreasing curve

24
Q

what does the graph of g against r look for a planet

A

a positive linear line up to the surface of the planet, that rapidly changes to a decreasing curve

25
Q

when a mass is in a uniform gravitational field, how can you calculate the change in potential energy

26
Q

what is the gravitational potential energy closer than infinity in a radial field

A

less than 0

27
Q

define gravitational potential energy

A

the work done to move a test mass from infinity to a given point in the field

28
Q

when is Ep=GMm/R used and when is Ep=mgh used

A

Ep=GMm/R is used to find absolute values in a radial field
Ep=mgh is used to calculate changes in a uniform field

29
Q

what is the total potential energies of a test mass in 2 gravitational fields

A

the sum of the gravitational potential energies due to the individual gravitational fields, it is never 0

30
Q

what is the work done to move a test mass from one point to another

A

the change in gravitational potential energy between the two points

31
Q

is the work done positive or negative when a test mass is moved away from the source mass

32
Q

what is the gravitational field for an object to escape the field into deep space

A

0/ negligible

33
Q

how much kinetic energy does an object need to escape the field

A

an amount equal to the magnitude of the gravitational potential energy

34
Q

what equation can be used to solve for the escape velocity

A

o.5mv^2=GMm/R

35
Q

what is escape velocity

A

velocity an object needs to escape a gravitational field