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15 Terms

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Luminosity

The total radiant output power of a star

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White dwarf

A very dense star formed from the core of a red giant, in which no fusion occurs

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Doppler effect

Observed frequency is different to source frequency when source moves relative to observer.

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Hubble’s law

Recessional speed / velocity of galaxy is proportional to its distance (from us)

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Kepler 1

The orbit of a planet is an ellipse with the Sun at one of the two foci

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Kepler 2

A line segment connecting a planet to the SUn sweeps out equal areas during equal intervals of time

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Kepler 3

The square of the orbital period T is directly proportional to the cube of the average distance r to the sun

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SHM

Oscillating motion for which the acceleration of the object is directly proportional to its displacement and in direction of the point of equilibrium

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Gravitational potential

The work done per unit mass to bring an object from infinity to a point in the gravitational field

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Ultimate tensile strength

The maximum stress that a material can withstand before it breaks

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Newton 1

A body will remain at rest or at constant velocity unless acted upon by a resultant force

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Newton 2

Resultant force is directly proportional to the rate of change of momentum

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Newton 3

When two objects interact, each exerts an equal but opposite force on the other during the interaction

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Latent heat

The energy required to change unit mass of a substance from ___ to ___ while at constant temperature

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homogeneous

Uniform in terms of distribution of matter