Graviaty basics
Escape velocity
Black holes
Measuring g
Graviational potential
100

The value of g is strongest at which part of the Earth?

poles

100

This happens to a ball thrown upwards if it doesn’t reach escape velocity.

Falls back

100

John Michell and Pierre Laplace speculated that stars with this property could trap light

very high mass / escape velocity equal to light speed

100

This instrument is used to measure tiny variations in gg

gravimeter

100

The gravitational field is called this because energy is not dissipated

conservative field

200

Earth’s shape is not perfectly spherical due to this reason

Rotation

200

The formula for escape velocity is this: 

v = square root 2GM/r

200

The radius at which an object becomes a black hole is called this

Schwarzschild radius

200

Variations in g caused by moving magma can be used to predict this natural hazard

Volcanic eruption

200

The work done by gravity around a closed loop is equal to this

Zero

300

Variations in gg can be used to prospect for these valuable resources

Minerals and oils

300

At infinity, gravitational potential energy has this value

0

300

According to Einstein, nothing can travel faster than this

speed of light

300

A gravimeter can detect changes as small as this fraction of g

one ten-millionth

300

Gravitational potential depends only on this, not the path taken

position (or location in the field)