Astrophysics Flashcards

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1
Q

Astronomical Unit

A

The distance from the Earth to the Sun. It is equivalent to 1.5x1011 m.

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2
Q

Light Year

A

The distance that light travels in one year. It is equivalent to 9.46x1015 m.

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3
Q

Gravitational Field Strength

A

The gravitational force per unit mass.

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4
Q

Gravitational Field

A

A region around a mass where another mass will experience a gravitational
force

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5
Q

Conservative Field

A

A field in which the work done by a force (e.g. the force of gravity) on a particle
that moves through any round trip in the field is zero i.e. energy is conserved

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6
Q

Newton’s Law of Universal Gravitation

A

Every object in the universe with a mass attracts every other object with a
mass. It gives a measure of the gravitational force of attraction between any
two objects and is an inverse square law.

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7
Q

Gravitational Potential

A

At a point in a gravitational field, it is the work done by external forces in
moving unit mass from infinity to that point.

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8
Q

Gravitational Potential Energy

A

Work done in moving mass from infinity to a point in the gravitational field

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9
Q

Escape velocity

A

The minimum velocity required by a mass, m, to just escape from a planet’s
gravitational field and reach infinity with zero velocity or zero kinetic energy.

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10
Q

Inertial frame of reference

A

A frame of reference in which an observer is not accelerating with respect to
another. That is, an observer will move at a constant speed with respect to
another.

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11
Q

Non-Inertial frame of reference

A

A frame of reference in which an observer is accelerating with respect to
another. That is, an observer will not move at a constant speed with respect to
another

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12
Q

Equivalence Principle

A

Gravity pulling in one direction is equivalent to acceleration in the other.
That is, there is no way to distinguish between the effects on an observer of a
uniform gravitational field and of a constant acceleration.

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13
Q

Spacetime

A

The combination of space and time.

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14
Q

Gravitational Time Dilation

A

Where the force of gravity is weaker, time passes more quickly

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15
Q

Gravitational Lensing

A

If an object has sufficient mass it can cause light which is travelling in a straight
line to bend.

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16
Q

World line/ geodesic

A

A curve in spacetime joining the positions of a particle throughout its existence.
It defines the position of an object in 3 dimensions (x, y and z) as well as the
fourth dimension of time (t).

17
Q

Geodesic path

A

The shortest distance between two points in spacetime

18
Q

Black hole

A

A region in space where the pull of gravity is so great that nothing, not even
light, can escape its pull.
It is also the last stage in the life cycle of a very high mass star.

19
Q

Event horizon

A

The radius of a black hole below which nothing, not even light, can escape from
its gravitational pull.
From the perspective of a distant observer, time appears to be frozen at this
point.

20
Q

Singularity

A

The centre point of a black hole

21
Q

Schwarzschild radius

A

The distance from the centre of a black hole to its event horizon.

22
Q

Stefan-Boltzmann Law

A

Gives a measure of the total energy being emitted at all wavelengths by a black
body.

23
Q

Black body

A

A body that absorbs all the electromagnetic radiation incident on it and also
emits all wavelengths of electromagnetic radiation.

24
Q

Luminosity

A

A measure of how bright a star actually is (i.e. the total power it emits), not
how bright it appears to us on Earth.
It is dependent on the star’s radius and surface temperature.

25
Q

Apparent brightness

A

A measure of how bright a star appears on Earth.

It is dependent on the star’s luminosity and distance from the Earth.

26
Q

Charge-Coupled Device (CCD)

A

A chip found behind the lens in a digital camera that stores images.

27
Q

Hydrostatic Equilibrium

A

When the thermal pressure outwards from a star balances the gravitational
force inwards.

28
Q

Proton-Proton chain

A

A three stage process in which stars produce energy by converting hydrogen
into helium through nuclear fusion.

29
Q

H-R Diagram

A

Relates a star’s luminosity to its temperature.
Stars are plotted on the diagram according to their size and luminosity and they
are found to fall into groups: main sequence, giants, supergiants and white
dwarfs.

30
Q

White dwarf

A

The last stage in the life cycle of a low mass (Sun like) star.

31
Q

Neutron Star

A

The last stage in the life cycle of a high mass star.