OP- D Astrophysics Flashcards

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1
Q

apparent brightness

A

amount of energy received per second per unit area by an observer (Wm-2)

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2
Q

astronomical unit

A

the mean distance from the centre of the Earth to the centre of the Sun
(1.50 x 10^11)

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3
Q

binary stars

A

two stars orbiting their common centre of mass

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4
Q

three types of binary stars

A
  • visual: can see two distinct stars
  • eclipsing: periodic variation of brightness
  • spectroscopic: change in wavelength of light receive from star (Doppler effect)
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5
Q

cepheid variable

A

a star that undergoes a periodic expansion of its outer layers that gives a periodic variation in its luminosity

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6
Q

Chandrasekhar limit

A

Maximum star remnant mass (1.4Ms) where electron degeneracy pressure prevent further gravitational collapse

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7
Q

constellation

A

a group of star that appears to make a pattern in the sky but they may not necessarily be close to each other in space.

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8
Q

cosmic microwave background (CMB) radiation

A

radiation emitted by the universe constituent with s temperature of 2.7K

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9
Q

cosmic scale factor (R)

A

gives a measure of the expansion that has taken place in the universe

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10
Q

dark energy

A

invisible energy source that my be accelerating the expansion of the universe

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11
Q

electron degeneracy pressure

A

where electron repulsion prevents further gravitational collapse of a star

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12
Q

galactic cluster

A

a group of galaxies bound together, orbiting around a common centre of gravity.

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13
Q

galaxy

A

a large scale collection of stars, gas, and dust held together by gravity.

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14
Q

globular stellar cluster

A

symmetrically arranged stellar cluster of 10^4 - 10^5 old stars

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15
Q

Hertzsprung-Russell diagram

A

graph plotting luminosity of stars against their temperature

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16
Q

Hubble’s Law

A

the speed at which galaxies are moving away from Earth (recession speed) is directly proportional to their distance from earth.

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17
Q

L⊙ and M⊙

A

symbols for luminosity and mass of the Sun

18
Q

light year (ly)

A

the distance light travels in one year.

19
Q

luminosity (L)

A

total amount of energy emitted per second by a star (unit: W)

20
Q

main sequence star

A

a “normal” star that is fusing hydrogen into helium

21
Q

nebula

A

intergalactic cloud of dust and gas

22
Q

Newton’s model of the universe

A

the universe is infinite in space and time, uniform and static

23
Q

open stellar cluster

A

irregular shaped stellar cluster of several hundred young stars

24
Q

Oppenheimer-Volkoff limit

A

maximum star remnant mass (3M⊙) where neutron degeneracy pressure prevents further gravitational collapse.

25
Q

parsec

A

distance at which the angle subtended by the radius of the Earth’s orbit is one arc-second

26
Q

planetary nebula

A

the ejection of outer layers of a small star (< 4M⊙) once fusion has stopped

27
Q

planetary system

A

a group of planet orbiting a star

28
Q

pulsar

A

a rotating neutron star

29
Q

recession speed

A

the speed at which an object is moving away from an observer

30
Q

red giant (and supergiant)

A
  • large (mass & surface area),
  • relatively cool star,
  • red in colour
  • late stage in a star’s life cycle
31
Q

redshift

A

apparent increase in the wavelength of light from distant galaxies due to their motion away from us

32
Q

redshift ratio (z)

A

ratio of change in wavelength due to the Doppler effect to original wavelength emitted by a galaxy moving relative to Earth.

33
Q

singularity

A

point containing the entire universe at the start of the Big Bang.

34
Q

stellar cluster

A

a close group of gravitationally bound stars, gas and dust (within a galaxy)

35
Q

stellar parallax

A

method used to measure distances to stars based on their apparent movement in position relative to distant background stars over a 6 month period.

36
Q

supercluster

A

a large grouping of galactic clusters

37
Q

supernova

A

the ejection of the outer layers of a large star (> 8M⊙) once fusion has stopped.

38
Q

type Ia supernova

A

type of supernova with a known luminosity that occurs in binary star systems where one of the stars is a white dwarf.

39
Q

white dwarf

A
  • small (mass & surface area)
  • relatively hot star
  • white in colour
  • final stage for a small star
  • no longer fusion, cooling down
40
Q
A