gravitational fields Flashcards

You may prefer our related Brainscape-certified flashcards:
1
Q

what is gravity

A

universal attractive force that acts between all matter

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
2
Q

what are field lines due to

A

objects having mass

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
3
Q

what do gravitational field lines represent

A

the direction of a field and the strength of the field depending on the density of field lines

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
4
Q

what is gravitational field strength

A

force per unit mass

g = f/m

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
5
Q

where is the mass concentrated

A

in the centre

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
6
Q

what happens to field lines close to the surface of the earth

A

they are uniform, equally spaced and almost parallel

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
7
Q

equation for gravitational force

A

g = -GmM/r^2

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
8
Q

what is g

A

g is the force per unit area in a uniform gravitational field

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
9
Q

how to derive g = GM/r^2

A

use
F = -GMm/r^2, g = f/m

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
10
Q

newtons law of gravitation

A

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

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
11
Q

keplers first law

A

orbit of a planet is an ellipse with the sun at one focus

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
12
Q

keplers second law

A

line segment joining a planet and the sun sweeps out equal areas during intervals of equal time

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
13
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 by considering the forces acting on the planet

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
14
Q

derive keplers third law

A

use GMm/r^2 and mv^2/r

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
15
Q

what are geostationary orbit

A
  • orbital period of 24 hours, same direction of rotation as earth
  • equatorial orbit
  • remain fixed in sky to observer
How well did you know this?
1
Not at all
2
3
4
5
Perfectly
16
Q

gravitational potential

A

the potential energy per kilogram at any point in the field, 0 potential is defined at infinity so at a point close to a mass the potential of an object would be negative

17
Q

gravitational potential difference

A

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

18
Q

what kind of law is newtons law of gravitation

A

inverse square law

19
Q

what is meant by an inverse square law

A

one quantity is inversely proportional to the square of the other

20
Q

what tis the gravitational potential energy at a point in the field

A

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

21
Q

escape velocity

A

the min velocity an object requires in order to escape the gravitational field of an. object when projected vertically from its surface

22
Q
A