Cosmology Flashcards

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1
Q

what is the cosmological principle

A

the universe is homogenous and isotropic

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2
Q

define homogoneous

A

uniform distribution of matter

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3
Q

define isotropic

A

physical property which is measured to be the same in all directions

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4
Q

what is 1AU (definition and value)

A

astronomical unit - average distance from the earth to the sun

1.5 x 10^11 m

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5
Q

define a light year

A

distance travelled by light in a vacuum in a year

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6
Q

define the parsec

A

the distance at which a radius of 1AU subtends an angle of one arcsecond

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7
Q

what is 1 degree in arcseconds

A

1 degree = 60 arcminutes = 3600 arcseconds

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8
Q

what is stellar parallax

A

a technique used to measure the distance of stars relatively close to us

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9
Q

what is parallax

A

the apparent shift in the position of a relatively close star against a backdrop of more distant stars

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10
Q

define the doppler effect

A

the apparent change in wavelength due to relative motion to an observer

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11
Q

what is red shifting

A

when a star/galaxy is moving away from an observer, the spectra lines will red shift (increased wavelength)

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12
Q

what is hubble’s law

A

recessional velocity of a galaxy is proportional to its distance from us

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13
Q

where can hubble’s law be applied

A

stars/galaxies outside of our own galaxy

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14
Q

why can hubble’s law not be used on very large or very short scales

A

short scale - gravitational attraction effects velocity
large scale - non-linear expansion rate may not be constant

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15
Q

what is evidence of the big bang

A
  • in every direction, the universe is red-shifting
  • in every direction, the temperature is about 2.7K
  • EM radiation started as gamma, but as universe expanded and cooled, wavelength stretched to microwave radiation ( λmaxT = constant)
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16
Q

what happened up to 1 second after the big bang

A

-started off as a hot, dense singularity
- time and space created
- inflation occurs
- expansion leads to cooling
- energy pair production - matter and antimatter elementary particles
- more matter than antimatter
- quarks combine to form protons and neutrons

17
Q

what happened up to 100 seconds after the big bang

A

protons and neutrons fuse to form hydrogen nuclei and primordial helium

18
Q

what happened up to 380,000 years after the big bang

A
  • atoms form as electrons cool down and combine with nuclei
  • universe becomes transparent - photons free to travel as gamma radiation
  • expansion of universe - gamma radiation now microwave radiation
19
Q

what happened up to 30 million years after the big bang

A
  • first stars appear
  • first heavier elements appear
20
Q

what happens up to 200 million years after the big bang

A

our galaxy forms as gravitational forces pull clouds of hydrogen and existing stars together

21
Q

what is dark matter and how was it discovered

A
  • discovered that stars at the edge of galaxies are moving faster than they should given the distribution of stars
  • this violates newton’s law
  • we call this missing mass ‘dark matter’
  • estimated 25% of the universe
22
Q

what is dark energy and how was its presence theorised

A
  • everything has gravity, therefore expansion of the universe should slow over time, or at least remain constant
  • however, the universe is expanding at an ever increasing rate
    scientists use dark energy to explain this, energy we do not know of which accelerates stars and galaxies
  • estimated 75% of the universe