Luminosity
The total radiant output power of a star
White dwarf
A very dense star formed from the core of a red giant, in which no fusion occurs
Doppler effect
Observed frequency is different to source frequency when source moves relative to observer.
Hubble’s law
Recessional speed / velocity of galaxy is proportional to its distance (from us)
Kepler 1
The orbit of a planet is an ellipse with the Sun at one of the two foci
Kepler 2
A line segment connecting a planet to the SUn sweeps out equal areas during equal intervals of time
Kepler 3
The square of the orbital period T is directly proportional to the cube of the average distance r to the sun
SHM
Oscillating motion for which the acceleration of the object is directly proportional to its displacement and in direction of the point of equilibrium
Gravitational potential
The work done per unit mass to bring an object from infinity to a point in the gravitational field
Ultimate tensile strength
The maximum stress that a material can withstand before it breaks
Newton 1
A body will remain at rest or at constant velocity unless acted upon by a resultant force
Newton 2
Resultant force is directly proportional to the rate of change of momentum
Newton 3
When two objects interact, each exerts an equal but opposite force on the other during the interaction
Latent heat
The energy required to change unit mass of a substance from ___ to ___ while at constant temperature
homogeneous
Uniform in terms of distribution of matter