Gravitational and Electric Fields (Unit 4) Flashcards
Newton’s Law of Gravity
an attractive force between two point masses
proportional to the product of their masses and inversely proportional to their separation squared
Concept of a force field
the region in which a body experiences a force
Representation of gravitational field lines (radial and uniform fields)
See sheet
Equipotential
Line joining points of equal potential
No work is done moving an object along an equipotential
Gravitational field strength, g
the force acting per unit mass
Gravitational field strength units
N kg-1 VECTOR
Gravitational potential, V, (at a point)
work done per unit mass to move a small mass from infinity to that point.
Units of gravitational potential
J kg-1 SCALAR
Gravitational potential, V, at infinity
zero
Gravitational potential difference, V, between two points
work done per unit mass to move a small mass from one point to the other.
Graphical variation of magnitude of g with r
See sheet
Graphical variation of V with r
See sheet
Area under graph of gravitational field strength against r
work done moving a unit mass between the two points
Gradient of graph of gravitational potential against r
gradient = -g (gravitational field strength); g= -(deltaV/delta r)
Derivation of Kepler’s Law
- Gravitational force = centripetal force
- GMm/r2 = mv2/r or GMm/r2 = mr(omega)2
- substitute for v (v = (2pi x r)/T) or omega( omega = (2pi)/T)
- re-arrange to get T2 = ((4pi2)/GM) x r3