Gravitational fields Flashcards
(39 cards)
What is the strength of a gravitational field, g?
The force per unit mass of a small test mass placed in the field (test mass is small such that it doesn’t significantly affect the gravitational field)
= F/m
Also the acceleration of a freely falling object - one that only experiences gravitational force
Radial vs uniform field
Radial - Line towards the centre of the body, g decreases with increasing distance
Uniform - magnitude of g is the same in magnitude and direction throughout the field - equally spaced and parallel
(Earth viewed from outer space vs viewed from surface)
Gravitational potential energy W
Energy of an object due to its position in a gravitational field - position for 0 gpe is at infinity - object so far away that the gravitational force on it is negligible
Gravitational potential (at a point) V
GPE per unit mass of a small test mass - work done per unit mass to move an object from infinity to that point
What is an equipotential
A surface of constant potential - no work is done moving along an equipotential
Equipotentials for equal increases in potential are spaced further apart for a planet
Over a small region, equipotentials are horizontal (parallel to ground), as a gravitational field over a small region is uniform
Potential gradient
Change in V/R for potential v over small distance r
also g=-V/R
Show that potential gradient = -g
To move a test mass m a distance r in the opposite direction to the gravitational force on it - its GPE must increase by an equal and opposite force F acting over a distance r, and by an amount of energy = Fr
change in V = Fr/m – F=mV/r – as gravitational force is in opposite direction - Fgrav = -mV/r
rearrange to give g = -V/R
g acts in the opposite direction to the potential gradient
Potential gradient contour analogy
Potential gradients are like contours on a map
Closer equipotentials - greater potential gradient and stronger field (closer contours steeper terrain), where equipotentials show equal spacing for equal changes of potential - potential gradient is constant (and g)
Potential gradient is at right angles to equipotential lines - so direction of gravitational force is always perpendicular to equipotentials
Rules for gravitational force between 2 objects
Always attractive
Inversely proportional to the square of distance between objects
Proportional to mass of objects
Gravitational field strength using law of gravitation
F=GMm/r^2 (M»m)
g = F/m = GM/r^2
Magnitude of attractive forces for spherical masses
Force of attraction on a test mass m from a distance R from the centre is the same as if all of the mass of M was concentrated at the centre
Relationship between g and r
g=g(s)R^2/r^2 where gs is g at the surface, and R is the radius of the body
inverse square relationship
g inside a planet
Inside a planet, only the mass in the sphere of radius r contributes to g, and remainder pf mass outside gives no resultant force. So as r becomes smaller, the mass of M that contributes to g is also smaller
derive eq then
Gravitational potential near a spherical planet
-GM/r
deriving escape velocity for a planet mass M and radius R
1/2mv^2 > GMm/r
V^2 > 2GM/R or V^2 > 2GR as gR^2 = GM
What is a geostationary orbit
One that is directly above the equator and has a time period of 24hrs
What is a synchronous orbit
One with the same time period as the orbiting body
(geostationary specifically over equator)
Significance of g=-V/R
g is in opposite direction of gradient.
r increases as you move away from the source of the gravitational field, but the force is in the opposite direction, ie towards the source of the gravitational field.
What is a hypothesis
a scientific hypothesis is a suggestion,
prediction or untested idea.
geosynchronous orbits vs low polar orbit
- It orbits over the Equator.
- It maintains a fixed position in relation to the
surface of the Earth. - It has a period of 24 hours (the same as the
Earth’s period of rotation on its axis). - The geosynchronous satellite enables
uninterrupted communication between a
transmitter and a receiver whereas the
other satellite does not. - Unlike the other satellite, the
geosynchronous satellite does not require the
use of a steerable dish.
A satellite in low polar orbit has a fairly
short time period, scanning the Earth
several times during the day.
An astronaut floats in a spacecraft in circular orbit around the earth, are they weightless
- the force of gravity on the astronaut is still
mg, where g is the local value of the field
strength within the spacecraft; - this force provides the centripetal force to
keep the astronaut in orbit; - the astronaut is in free fall, as is the
spacecraft; - the astronaut appears weightless because
he or she is not supported
Weight from sensation of support
What is a force field?
A region in which an object experiences a non contact force, arising from the interaction between mass, static charges and between moving charges
Definition of free fall
Only acted upon by gravity