Fields Flashcards
(148 cards)
What is a field?
A region in which a body experiences a non-contact force.
A field arises from the interaction of mass, of static
charge, and between moving charges.
What is gravity?
A universal attractive force acting between all matter.
What is Newton’s Law of attraction?
Every particle attracts every other particle in the universe with a force which is directly proportional to the product of their masses and inversely proportional to the square of the distance between them.
What is the equation for force between point masses?
F = Gm(1)m(2)/r²
G is the ‘universal gravitational constant’
Every massive object in the universe attracts every other massive object. The force is always attractive.
What is a gravitational field?
The Earth applies a force to everything within its gravitational field.
The field due to a body is the region of space surrounding it where other bodies will feel a force due to it.
Gravitational fields have infinite reach.
What is a radial field?
The field lines become more spread out as the distance from a spherical object increases, increasing the diminishing strength of the field.
The force per unit mass varies inversely with distance squared.
NB: The field is 3D.
The gravitational field is radial in the region surrounding the Earth i.e. for satellites.
What is a uniform field?
The field lines are parallel and equidistant, indicating that the field is constant.
The gravitational field is uniform close to the Earth’s surface i.e. for cars, balls, planes, etc.
What are the rules about field lines?
- They don’t start and stop in empty space. They end on a mass and extend back all the way to infinity.
- They never cross.
What is gravitational field strength?
Your pull on the earth = the earth’s pull on you. But your gravitational field is far weaker.
The field strength at a point in a body’s field is the gravitational force exerted on an object placed at that point, per kg of the object’s mass.
i.e. the no of newtons of attractive force acting per kg of the object’s mass
g = F/m
The gravitational field strength at a point in a field does not depend on the mass placed there - it is a property of the field.
Therefore, two objects of different mass placed at the same point in the field will experience the same field strength, but a different force.
What is the difference between a and g?
They have the same symbol but a different unit.
What is the gravitational field strength in a radial field?
g = F/m but F = GMm/r²
therefore, g = GM/r²
What is gravitational potential?
The gravitational potential at a point in a gravitational field is the work done in moving a unit mass from infinity to that point.
OR
The gravitational potential at a point in a field is the energy per unit mass.
V = Ep/m
It has a 0 value at infinity.
NB: The answer for V is the same for everyone at the same point in the field.
What is gravitational potential difference?
If a mass is moved from one position to another, there is a change in gravitational potential.
Therefore, there is also a change in gravitational potential energy.
This is the work done in moving a mass.
ΔEp = mΔV
The actual value is always higher as frictional forces have to be overcome i.e. drag force within the Earth’s atmosphere.
What is an equipotential surface?
All points on an equipotential surface have the same gravitational potential.
The lines are always perpendicular to the gravitational field.
Due to this, the gravitational potential difference is zero when moving along the surface, so no work is done when moving along an equipotential surface.
What is gravitational potential energy?
The energy an object possesses because of its position in a gravitational field.
In a uniform field, Ep = mgh
In a radial field, Ep = - GMm/r = GM(E)m(1/r(2) - 1/r(1))
The energy doesn’t vary as rapidly.
What is gravitational potential in different fields?
In uniform:
V = Ep/m but Ep = mgh therefore V = gh
In radial:
V = Ep/m but Ep = -GMm/r therefore V = -GM/r
Why is gravitational potential negative?
Positive work must be done against gravity (by an external force) to move an object away from the Earth. The object gains potential energy if moved away from the Earth.
But it has zero potential energy at infinity.
Hence it must have negative potential energy when closer to Earth than infinity.
What two graphs can be drawn?
g against r
V against r
How is g related to V?
V = -GM/r
but g = GM/r²
therefore g = -ΔV/Δr
This is the gradient of the V-r graph.
How can a g-r graph be used?
Area: ΔV
Area x Mass: Work Done
How can a mg-r graph be used?
Area: Gravitational Potential Energy
What are Kepler’s Laws?
- The orbit of every planet is an elipse with the Sun at one focus.
- A line joining the planet to the Sun sweeps out equal areas in equal times.
- The time for one orbit, T and the average distance from the planet to the Sun, r are related by T² ∝ r³.
What was Newton’s proof?
Assuming the orbit of a planet is circular, there must be a RF towards the center of the circle i.e. a centripetal force.
This is provided by the gravitational attractive force of the Sun.
F = mv²/r and F = GMm/r²
therefore, mv²/r = GMm/r² so v²r = GM
but v = 2πr/T so 4π²r³/T² = GM
therefore, T²/r³ = 4π²/GM (everything is constant)
Why are equipotential surfaces useful for satellites?
A satellite orbiting the Earth along an equipotential line does 0 work as ΔV = 0 and the force is always at 90°. Therefore, Ek isn’t lost, else the satellite would fall towards the Earth.