What is gravity?
Gravity is a universal attractive force that acts between all of matter.
What are gravitational fields?
Regions in which a body would experience a non-contact force
What do the gravitational field lines represent?
They show the direction of a force on a mass placed in the field (always towards the object).
The strength of the field is represented by the density of the field lines (more dense means stronger).
What is Newton’s law of gravitation?
F = Gm1m2 / r2
where
F is gravitational force (N)
G is the gravitational constant (6.67 x 10-11 Nm2kg-2 - BU: m3kg-1s-2)
m1 is the mass of the first object (kg)
m2 is the mass of the second object (kg)
r is the distance between the objects (m)
How to calculate gravitational field strength?
g = F/m = GM / r2
where
g is the gravitational field strength (N/kg)
G is constant of gravitation
M is the mass of the larger object (e.g. planet)
r is the radius of the large object
What is gravitational potential?
The work done in bringing a 1kg mass from infinity to a point.
Therefore, the gravitational potential at infinity is 0 and gravitational potential is negative.
What are equipotential surfaces?
The gravitational potential is constant along an equipotential surface.
Field lines are perpendicular to equipotentials.
Closer that the lines are, the stronger the gravitational acceleration.
No work is done moving along an equipotential surface.
What is the area under the graph of gravitational force and distance between objects?
The work done.
What does the area under the gravitational field strength and distance between objects represent?
The change in gravitational potential.
g = - ΔV/Δr
How to calculate the kinetic energy of a satellite?
KE = 1/2 GMm/r
where
KE is the kinetic energy (J)
G is the constant of gravitation
M is larger mass
m is the smaller mass
r is the distance between the objects
How to find the orbital period and speed of planets and satellites?
V = 2πr / T = √GM/r
Where
r is the radius of orbit (m)
T is the time period of orbit (s)
V is the orbital speed (rad/s)
G is the constant of gravitation
M is the mass of the planet which is being orbitted
How to prove that T^2 is proportional to r^3 in orbit (where T is the orbit time period and r is the distance between satellite and planet)?
1) Set gravitational force as equal to centripetal force:
GMm / r2 = m⍵2r
2) Rearrange with ⍵ = 2π/T:
GM / r3 = 4π2 / T2
3) Since everything else is constant, T squared and r cubed are proportional.
How to find the total energy of an orbiting satellite?
ET = 1/2 mv2 - GMm/r
If total energy is 0J, then the satellite has escaped the orbit. Therefore, we can calculate escape velocity using:
vescape = √2GM/r
What is a geostationary orbit?
A satellite which has a geostationary orbit, it has a 24 hours, equatorial orbit moving from west to east.
What are the uses of geostationary orbits?
How to work out the height of a geostationary orbit?
r = 3√T2GM/4π2
What are the properties of the graph of log(T) against log(R)?
log(T) = (3/2)log(r) + (1/2)(log(4π2/GM)
What is Newton’s law of gravitation in words?
The gravitational force between two objects is proportional to the product of their masses and inversely proportional to the square of their separation.
What is Coulomb’s Law in words?
The electrostatic force between two point charges is directly proportional to the product of the charges and inversely proportional to the square of their separation.
What is the equation for electrostatic force between two charges?
F = Q1Q2 / 4πε0r2
where
Q1 is charge of one object
Q1 is the charge of the other object
ε0 is the permittivity of free space
r is the distance between the centres of the charges
What do negative and positive forces mean for electrostatic forces?
Negative is attraction, positive is repulsion
What are the approximations used in Coulomb’s law?
What are the rules for electric field lines?
What is electric field strength?
The force per unit charge experience by a small positive charge placed at that point in the electric field
E = F/Q