Astrophysics SL Flashcards

(57 cards)

1
Q

apparent brightness (b)

A

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

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2
Q

astronomical unit (AU)

A

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

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3
Q

binary stars

A

two stars orbiting their common centre of mass

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4
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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5
Q

Chandrasekhar limit

A

maximum star remnant mass (1.4M⊙) where electron degeneracy pressure prevents further gravitational collapse

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6
Q

constellation

A

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

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7
Q

cosmic microwave
background (CMB) radiation

A

radiation emitted by the universe consistent with a temperature of 2.7K

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8
Q

cosmic scale factor (R) (expansion)

A

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

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9
Q

dark energy

A

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

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10
Q

electron degeneracy
pressure

A

where electron repulsion prevents further gravitational collapse of a star

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11
Q

galactic cluster

A

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

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12
Q

galaxy

A

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

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13
Q

globular stellar cluster

A

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

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14
Q

Hertzsprung-Russell
diagram

A

graph plotting the luminosity of stars against their temperature

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15
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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16
Q

L⊙ and M⊙

A

symbols for luminosity and mass of the Sun

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17
Q

light year (ly)

A

the distance light travels in one year

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18
Q

luminosity (L)

A

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

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19
Q

main sequence star

A

a “normal” star that is fusing hydrogen into helium

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20
Q

nebula

A

intergalactic cloud of dust and gas

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21
Q

neutron degeneracy
pressure

A

where neutron repulsion prevents further gravitational collapse of a star

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22
Q

Newton’s model of the
universe

A

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

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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
parsec
distance at which the angle subtended by the radius of the Earth’s orbit is one arc-second
26
planetary nebula
the ejection of the outer layers of a small star (< 8M⊙) once fusion has stopped
27
planetary system
a group of planets orbiting a star
28
pulsar
a rotating neutron star
29
recession speed
the speed at which an object is moving away from an observer
30
red giant (and supergiant)
large (mass & surface area), relatively cool star, red in colour
31
redshift
apparent increase in the wavelength of light from distant galaxies due to their motion away from us
32
redshift ratio (z)
ratio of change in wavelength due to cosmological redshift to original wavelength emitted by a galaxy moving relative to Earth
33
singularity
point containing the entire universe at the start of the Big Bang
34
stellar cluster
a close group of gravitationally bound stars, gas and dust (within a galaxy)
35
stellar parallax
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
supercluster
a large grouping of galactic clusters
37
supernova
the ejection of the outer layers of a large star (> 8M⊙) once fusion has stopped
38
type Ia supernova
type of supernova with a known luminosity that occurs in binary star systems where one of the stars is a white dwarf
39
white dwarf
small (mass & surface area), relatively hot star, white in colour
40
cosmic scale factor (relative)
a measure of the relative size of the Universe
41
accelerating universe outcome
expansion continues at an increasing rate due to dark energy
42
type Ia supernovae (formation)
formed when a white dwarf in a binary system gains mass from its companion star and explodes due to fusion restarting
43
closed universe outcome
gravity causes the Universe to collapse back in on itself - the Big Crunch
44
open universe outcome
gravity slows expansion but is not strong enough to stop it
45
flat universe outcome
gravity slows expansion but takes an infinite time to do so
46
MACHOS
Massive Compact Halo Objects - high density compact stars at the ends of their lives
47
Jeans mass (Mj)
minimum mass required for a gas cloud to collapse and star formation to occur
48
r-process
neutron capture where there is not time for beta decay to occur before further neutron capture
49
s-process
neutron capture where there is time for newly formed nuclides to undergo beta decay and form a new element
50
CNO cycle
process by which hydrogen undergoes fusion to create helium in stars with a mass greater than four solar masses
51
proton-proton chain
process by which hydrogen undergoes fusion to create helium in the Sun
52
nucleosynthesis
process of forming different nuclides by nuclear fusion
53
type II supernovae
result from the rapid collapse and violent explosion of a massive star (> 8 solar masses)
54
density parameter (Ωo)
the ratio of the actual density of the Universe (ρ) to the critical density (ρc)
55
isotropic
the same in all directions
56
WIMPS
Weakly Interacting Massive Particles - subatomic particles
57
the Cosmological Principle
when viewed on a large scale, the Universe is homogenous and isotropic