Gravitational fields Flashcards

1
Q

what is a force field

A

an area that experiences a non-contact force

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2
Q

what is a gravitational field

A

an area where an object with mass experiences an attractive force

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3
Q

what are field lines

A

Represent a field visually, they tell you the direction of the force acting at that point in the field. dense lines indicate a stronger field.

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4
Q

what is a radial field

A

it means all the lines meet at the centre of mass, implying the field is weaker the further way from the centre. earth has a radial gravitational field.

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5
Q

what is a uniform field

A

where all the field line are parallel, implying field strength is constant. this is considered to be the case at an objects surface

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6
Q

how is field strength and distance to the centre related

A

its an inverse square law

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7
Q

what is newtons law of gravity

A

allows you to calculate force in a gravitational field.
-its proportional to the product of the masses
-its inversely proportional to the square of the distance
-its always attractive

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8
Q

what is gravitational field strength

A

the force on an object per unit mass

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9
Q

how does gravitational field strength relate to distance graphically

A

1/x^2
from 9.81 on the graph
doesnt reach 0

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10
Q

what is gravitational potential

A

the energy required (work done) to move a 1kg mass from infinity to a point in the field

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11
Q

what are equipotential lines

A

when putting values of V on a map they look like contour lines, which are at right angles to the gravitational field lines

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12
Q

why is gravitational potential negative

A

because at infinity, GPE=0 and g=0. so as you fall further from infinity you gain g, and therefore GPE. so moving toward it means you have negative GPE as its a vector.

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13
Q

what does gravitational potential against distance look line on a graph

A

-1/x
starts at -62.5
doesn’t reach 0

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14
Q

what does the gradient mean on a gravitational potential against distance graph.

A

gravity
a tangent will need to be drawn

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15
Q

what is gravitational potential difference

A

if you want to move an object close of further from earth then you need to move between equipotential lines
earth=62.5MJ ISS=60.6MJ diff= 1.9MJ
for every 1kg you want to move it will take 1.9MJ

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16
Q

why does a satellite do no work

A

it moves along an equipotential line, so the gravitational potential different is 0

17
Q

what is the equation for gravitational potential energy

18
Q

how to do you calculate gravitational difference from a field strength against distance graph

A

area underneath it

19
Q

what is a low earth orbit

A

between 200-2000km
around 2 hour time period
used for weather satellites
can be at an angle to the equator.

20
Q

what is a geostationary orbit

A

at 35000km
exactly 24 hour time period, will remain at the same point above earth
in line with the equator
used for communication

21
Q

what are polar orbits

A

when an orbit is at 90 degrees to the equator.
every time it fishies an orbit it will be over a new part of earth making it idea, for scanning it.
however you need a lot of satellite dishes with moveable heads to track it.

22
Q

what is a synchronous orbit

A

when the orbiting object has the same period equal to the body its orbiting

23
Q

what is a geosynchronous orbit

A

an orbit with the same time period as earth (24 hours)

24
Q

why is orbital speed different for different objects

A

a closer satellite to an object must go faster due to a much stronger gravitational force. so it will need a much higher horizontal velocity

25
what is orbit
bets explained using newtons cannon, cannon fired at the top of mountain will follow a curved path (projectile). but earth is curved, so all objects are in free fall toward earth, so firing an object fast enough the ground will fall away as fast as the object.
26
what are the energy changes in a circular orbit
speed is constant altitude is constant so total energy is Ek+GPE
27
what are the energy changes in an elliptical orbit
the total energy is still the sum of the kinetic and gravitational energy, and remains constant at closest approach GPE will be lowest so Ek will be highest to conserve energy. and vice versa
28
what 4 equations need to be derived
Keplers 3rd law- centripetal force=gravitational force escape velocity- Ek=gravitational potential orbital velocity- centripetal force=gravitational force kinetic energy of an orbit-Ek-(sub)orbital velocity
29
what is escape velocity
how fast an object needs to be going to escape the gravitational pull of a mass