D. Astrophysics SL Flashcards

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1
Q

Comet

A

a celestial object consisting of a nucleus of ice and dust and, when near the sun, a ‘tail’ of gas and dust particles pointing away from the sun.

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2
Q

Asteroid

A

 Asteroid = a small rocky body orbiting the sun. Large numbers of these, ranging enormously in size, are found between the orbits of Mars and Jupiter, though some have more eccentric orbits.

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3
Q

Planet

A

 Planet = a spherical body moving in an elliptical orbit round a star.

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4
Q

Conditions for being a planet

A

o Clear the area around it with its gravity
o Orbit a star with a low eccentricity
o Have sufficient mass to form a spherical shape

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5
Q

Star

A

 Star = a luminous sphere of plasma held together by its own gravity.

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6
Q

Binary stars

A

o Binary stars are two stars orbiting around the centre of mass of both stars.

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7
Q

Planetary system

A

 Planetary system = a group of gravitationally bound non-stellar objects in orbit around either a star or a star system.

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8
Q

Constellation

A

 Constellation = A group of stars forming a recognisable pattern in the sky often named after the mythological character they represent.

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9
Q

Stellar cluster

A

 Stellar cluster = A group of stars that are close together and are formed from the same gas cloud.

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10
Q

Open cluster

A

o An open cluster is a group of up to a few thousand stars that were formed from the same giant molecular cloud and have roughly the same age (<10 billion years old).

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11
Q

Globular cluster

A

o A globular cluster is a spherical collection of stars that orbits a galactic core as a satellite. Globular clusters are very tightly bound by gravity, which gives them their spherical shapes and relatively high stellar densities towards their centres (>10 billion years old).

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12
Q

Nebula

A

 Nebula = a region of dust and gas where stars are born.

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13
Q

Galaxy

A

 Galaxy = a large collection of stars (hundreds of billions) held together by their mutual gravity.

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14
Q

Spiral galaxy

A

o Spiral galaxies consist of a rotating disk of stars and interstellar medium with a central bulge of (generally) older stars. Extending outward from the bulge are relatively bright arms.

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15
Q

Elliptical galaxy

A

o Elliptical galaxies range in shape from nearly spherical to highly flattened ellipsoids and range in size from hundreds of millions to over one trillion stars. They could be formed from the collisions of spiral galaxies.

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16
Q

Irregular galaxy

A

o Irregular galaxies have no specific structure. This could be because other, more massive galaxies have drawn away their matter.

17
Q

Cluster of galaxies

A

 Cluster of galaxies = a structure that consists of anywhere from hundreds to thousands of galaxies that are bound together by gravity with typical masses ranging from 10^14–10^15 solar masses.

18
Q

Super cluster of galaxies

A

 Super cluster of galaxies = a large group of smaller galaxy clusters or galaxy groups, which is among the largest-known structures of the cosmos.

19
Q

 Luminosity =

A

the total energy emitted by the star per second.

20
Q

 Apparent brightness =

A

the energy reaching a square metre on Earth per second.

21
Q

 Black body = .

A

an object that absorbs all radiation that falls on it and emits all radiation within it

22
Q

 Stefan-Boltzmann law =

A

the luminosity of a star depends on its surface area and absolute temperature according to L = sigmaAT^4

23
Q

Hydrostatic equilibrium

A

Where the radiation pressure is a balanced by the gravitational attraction.

24
Q

Main sequence star

A

Stars that produce energy through the fusion of hydrogen into helium.

25
Q

Cepheid variable

A

Stars that have a luminosity that varies periodically

26
Q

Big bang

A

The rapid expansion of soace and time from a state of extremely high density and temperature.

27
Q

CMBR

A

Em radiation left over from the early stages of the universe

28
Q

Chandrasekhar limit

A

Minimum mass a star remnant must have to become a neutron star (1.4 solar masses)

29
Q

Oppenheimer Volkoff limit

A

Minimum mass a neutron star must have to become a black hole (3 solar masses)