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1
Q

Velocity

A

The rate of change of displacement

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2
Q

Acceleration

A

The rate of change of velocity

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3
Q

Work done

A

A measure of the energy transferred during a process

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4
Q

Law of consrvation of energy

A

Energy can neither be created or destroyed, just changes from one form to another.

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5
Q

Momentum

A

The product of an object’s mass times it velocity

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6
Q

Law of conservation of momentum

A

In the absence of external forces the total momentum before a collision is equal to the total momentum after a collision

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7
Q

Elastic collision

A

An elastic collision is one in which kinetic energy is conserved.

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8
Q

Inelastic collision

A

An inelastic collision is one in which kinetic energy is lost

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9
Q

Newton’s first Law

A

An object will remain at rest or continue at constant speed in a straight line unless acted on by an unbalanced force

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10
Q

Newton’s second law

A

The acceleration of an object is proportional to the unbalanced force acting on it and inversely proportional to its mass. (a = F/m)

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11
Q

Newton’s third law

A

If a body A exerts a force on body B then body B exerts an equal and opposite force on body A.

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12
Q

Newton

A

One Newton is the force required to give an object of mass 1kg an acceleration of 1ms-2.

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13
Q

Impulse

A

Impulse is the average force on an object multiplied by the time of contact (Ft)
Impulse is also equal to the change in momentum of the object.

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14
Q

Universal law of gravitation

A

The force of attraction between two objects is directly proportional to the product of their masses and inversely proportional to the square of the distance between them. F = Gmm/r2

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15
Q

Gravitational field strength

A

Gravitational field strength is the force (or weight) per unit mass experienced at a point in a gravitational field. (g = F/m)

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16
Q

Time dilation

A

The time between events measured by a stationary observer will be greater than that measured by an observer moving with the events.

17
Q

Length contraction

A

The length between events measured by a stationary observer will be less than that measured by an observer moving with the events.

18
Q

Doppler effect

A

The frequency of radiation observed depends on the velocity of the source relative to the observer.

19
Q

Redshift

A

Redshift is the term given to the change in frequency of light emitted by stars, as observed from earth, due to the stars moving away from us. The spectra of these stars is shifted towards the red end of the spectrum.

20
Q

Hubbles Law

A

For distant objects, the further away from Earth the object is, the faster it is moving away from Earth. v = Hod where v = recessional velocity and Ho = Hubbles constant.

21
Q

Dark Matter

A

Type of matter proposed to make up for the missing mass in the Universe.

22
Q

Dark energy

A

Type of energy proposed to make up for the missing energy in the Universe.
This is to account for the fact that the rate of expansion of the Universe is increasing.

23
Q

Cosmic Microwave Background (Radiation)

A

Observed background radiation present everywhere in the Universe. It provides evidence to support the Big Bang theory

24
Q

Anti-matter

A

Each matter particle has an antimatter particle equivalent with an opposite charge but identical mass.

25
Q

Baryon

A

A particle made up of 3 quarks

26
Q

Meson

A

A particle made up of 2 quarks

27
Q

Boson

A

Force mediating particle

28
Q

Fermion

A

Matter particle

29
Q

Hadron

A

a particle made up of quarks