The Expanding Universe Flashcards

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1
Q

what is the doppler effect?

A

the apparent change in frequency of a wave when the source and observer are moving relative to each other

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2
Q

doppler effect: when to add or subtract

A

add when moving away

subtract when moving towards

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3
Q

doppler effect equation

A

fo=fs(v/(v+/-vs)

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4
Q

what is redshift?

A

the ratio of recessional velocity of a galaxy to the speed of light

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5
Q

what to remember about redshift

A

no units

will always be <1

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6
Q

difference between redshift and blueshift

A

redshift - travelling away

blueshift - travelling towards

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7
Q

two scenarios for the future of the universe

A
  1. closed universe - slow its expansion then contract

2. open universe - will expand forever

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8
Q

what is Hubble’s law?

A

v=Hod

further away galaxies travelling faster

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9
Q

what is Hubble’s constant?

A

2.3x10^-18 s^-1

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10
Q

how to prove age of the universe

A

using hubble’s constant and d=vt

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11
Q

chocolate muffin analogy

A

galaxies moving away from each other

not individual galaxies expanding

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12
Q

dark matter

A

a considerable amount of matter in galaxies that we cannot see

accounts for the observation of unusually high orbital speeds of stars in the outer arms of galaxies

thought to make up around 22% of all matter in the Universe

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13
Q

dark energy

A

force which acts against gravitational force of attraction, pushing matter apart

accounts for observation that expansion of Universe is accelerating

It is thought to make up around 74% of all matter in the Universe

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14
Q

what does the temperature of an object determine?

A

the frequency of light that it emits

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15
Q

very hot stars are what colour

A

blue

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16
Q

is the peak wavelength small or large for hot stars?

A

small

17
Q

stars emit light over a…

A

range of wavelengths

18
Q

4 pieces of evidence for Big Bang theory

A
  1. Abundance of hydrogen and helium
  2. Cosmic Microwave Background Radiation
  3. Olber’s Paradox
  4. Expansion of the Universe
19
Q

abundance of hydrogen and helium

A

H and He are the simplest to form and should be most abundant as atoms only formed when the Universe was cold enough

Other elements formed inside stars

20
Q

Cosmic Microwave Background Radiation

A

should be residual background electromagnetic radiation from Big Bang

every direction in sky, small amount of microwave radiation - 2.7K

21
Q

Olber’s paradox

A

why isn’t the sky always bright/ star in every line of sight?

  1. we can only see 13.8 billion lightyears into the Universe
  2. Galaxies travelling away will redshift. Cannot see infrared