Gravitational and Electric Fields Flashcards
What type of field is a gravitational field?
A gravitational field is a force field
What is a force field?
- A force field is a region where an object will experience a non-contact force
- Force fields cause interactions between objects or particles or in the case of gravity, between masses
What type of quantity is a force field?
A vector quantity
What happens when an object is put in the gravitational field of another object?
Any object with mass will experience an attractive force if you put it in the gravitational field of another object
How can you represent the force field around an object?
Force fields can be represented as vectors showing the direction of the force they would exert on an object placed in that field. Gravitational field lines are arrows showing the direction of the force that masses would feel in a gravitational field
How can you tell the direction of the force in a force field diagram?
The direction that the arrows are pointing in shows the direction of the force
What would happen if you put a small mass anywhere in the Earth’s gravitational field?
If you put a small mass anywhere in the Earth’s gravitational field it will always be attracted towards the Earth
What type of field is the Earth’s gravitational field?
The Earth’s gravitational field is radial - the lines of force meet at the centre of the Earth
Explain in terms of field lines the effect on the force felt by a mass in the Earth’s gravitational field if it were moved further away?
If the mass is moved further away from the Earth where the lines of force are further apart the force it experiences decreases
Why does the gravitational field of a small mass in the Earth’s gravitational field not affect the Earth?
The gravitational field of the mass does not affect the Earth as the Earth is much more massive
How is an uniform field represented on a field line diagram?
The field lines are parallel and equally spaced
Define a gravitational force field
A region in which an object with mass experiences weight
State the equation given by Newton’s Law of Gravitation and each variable
F = Gm1m2/r^2
- G is the gravitational constant
- m1 and m2 are the respective masses of the objects involved
- r is the distance between the centres of the two masses in metres
- F is the magnitude of the gravitational force between masses m1 and m2
State Newton’s Law of Gravitation
The gravitational force of attraction between two masses is inversely proportional to the distance between their centre of masses squared and is directly proportional to the product of the two masses
What would happen to the force between two objects in a gravitational field if the distance r between two masses increases?
As Newton’s law of gravitation is an inverse square law, F ∝ 1/r^2
If the distance r between the masses increases the force F will decrease
What would happen to the force between two objects in a gravitational field if the distance between them doubles?
If the distance between two objects in a gravitational field doubles then the force will be one quarter of the original force
What does the gradient of a force-mass graph tell us?
The gravitational field strength
Define gravitational field strength
The gravitational field strength at a point in a gravitational field is the force acting per unit mass at that point
What is the formula for calculating the gravitational field strength of a uniform field?
g = F/m
- F is the force experienced by a mass when its placed in a gravitational field
- Units are N/kg
What is the gravitational field strength at a point equal to?
The gravitational field strength at a point is equal to the acceleration due to gravity at the point
What type of quantity is gravitational field strength?
A vector quantity
What is the formula for calculating the gravitational field strength in a radial field and what are the variables?
- g = GM/r^2
- G is the gravitational constant
- M is a point mass (kg)
- r is the radius of the mass (m)
What type of objects have a radial field?
Spherical objects
What type of relationship does gravitational field strength and distance have?
They have an inverse square law relationship meaning that as r increases, g decreases
Draw a graph of g against r to show the inverse square law relationship between them
- See page 121 in the revision guide*
See page 7 in g fields pack
Define gravitational potential
The gravitational potential at a point is defined as the work done in bringing unit mass from infinity to that point in the gravitational field
What is the formula for calculating gravitational potential in a radial field and its variables?
V = -GM/r
- V is gravitational potential
- M is the mass of the object causing the gravitational field
- r is the distance from the centre of the object
What is the gravitational potential at an infinite distance from an object?
0
Why are GPE and gravitational potential always negative?
GPE and gravitational potential are always negative because gravity causes an attractive force and you have to do work against the gravitational field to move an object out of it
What is the formula used to calculate gravitational field strength from gravitational potential?
g = - ΔV/Δr
What is the gradient of a graph of gravitational potential against distance?
The gravitational field strength
What is the area under a graph of gravitational field strength against distance?
The change in gravitational potential
Define escape velocity
The minimum speed an unpowered object needs in order the leave the gravitational field of a planet (or star)
Derive the formula for escape velocity
See page 122 in the revision guide
1- 1/2mv^2 - GMm/r = 0
2- 1/2mv^2 = GMm/r
3 - 1/2v^2 = GM/r
4 - v^2 = 2GM/r
5 - v = √2GM/r
Define gravitational potential difference
Gravitational potential difference is the energy needed to move a unit mass
(Difference in gravitational potential between two points, not traditional pd)
What is the formula used to calculate the work done when moving an object in a gravitational field?
ΔW = mΔV
- ΔW is the work done in J
- ΔV is the gravitational potential difference
- m is the mass of the object
What are gravitational equipotentials?
Gravitational equipotentials are lines in 2D and surfaces in 3D that join all of the points with the same potential. They show all points of equal potential in a field
What happens as you travel along an equipotential in terms of energy transfer?
As you travel along an equipotential, no work is done moving along an equipotential. This means that for the journey ΔV = 0
What is the relationship between equipotentials and field lines?
Equipotentials and field lines are perpendicular
What are the differences when calculating the work done in both uniform and non-uniform fields?
- In a uniform field the gravitational field strength is constant so we can calculate work done using GPE = mgh
- In a non-uniform field the gravitational field strength is not constant so we have the calculate the work done using ΔW=mΔV
Show the relationship between the period and the radius of an orbit to be T^2∝r^3
1- The force acting on an object in circular motion is given by F=mv^2/r
2- The force of attraction due to gravity between two objects with masses is given by F=GMm/r^2
3- Make the two equations equal and rearrange to find the speed of a satellite in a gravitational field to get v = √GM/r
4- The time taken for a satellite to make one orbit is called the orbital period, T
5- Speed = distance/time and the distance for a circular orbit is 2πr so v = 2πr/T
6 - Rearrange for T to get T = 2πr/v
7- Sub the expression for v we found earlier into T = 2πr/v
8 - Rearrange to get T^2 in terms of r^3 where the constant of proportionality is 4π^2/GM
Explain how a satellite will move around a planet/star at a constant speed but will be constantly accelerating
- A satellite will move around a planet/star at a constant speed but will be constantly accelerating because the centripetal force on the satellite is at right angles to the velocity
- Therefore, there is no component of the force in the direction of the velocity to increase or decrease the size of it
- The force does no work on the satellite and so there is no change in the kinetic energy of the satellite
- The satellite is always accelerating towards the centre of mass of the star/planet which it is orbiting
Show how the relationship T^2∝r^3 can be applied to questions
Ta^2/ra^3=Tb^2/rb^3 where a and b are two different orbiting objects
Describe the conservation of energy for an orbiting object which moves to another orbit from the one it started with
If a satellite is in a circular orbit and moves to another circular orbit then the sum of potential and kinetic energy will not be the same
Explain the conservation of energy for an orbiting satellite in both a circular orbit and an elliptical orbit
- An orbiting satellite has kinetic and potential energy, its total energy (KE + GPE) is always constant
- In a circular orbit a satellite’s speed and distance above the mass its orbiting are constant. This means that its kinetic energy and potential energy are also both constant
- In an elliptical orbit a satellite will speed up as its height decreases and slow down down as its height increases. This means that its kinetic energy increases as its potential energy decreases and vice versa so the total energy remains constant
How often do Geostationary satellites orbit the Earth?
Geostationary satellites orbit the Earth once in 24 hours. Their orbits take exactly one day