The Fate of the Universe Flashcards

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1
Q

why has there been variations in the values of the hubble constant

A

because of the different observational methods used to find it

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2
Q

why is having an inaccurate hubble constant value problematic

A
  • it gives a huge variation in possible ages of the universe

- ranging from 10 to 20 billion years

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3
Q

given that the hubble constant is used to calculate the age of the universe, will we ever truly know the age of the universe and why

A
  • no
  • because the hubble constant is measured using experimental methods and instruments
  • which have their own uncertainties
  • so we can only get more accurate answers
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4
Q

what is the universe constantly doing

A

expanding

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5
Q

will the universe continue to expand forever

A

we dont know

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6
Q

what factors determine what route the universe will take over the many years

A
  • the mass of the universe

- the density of the matter within the universe

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7
Q

what force naturally opposes the expansion of the universe given that there is matter within the universe

A

gravity

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8
Q

what is the big crunch

A
  • a possible theory for the future of the universe
  • where gravity overcomes the expansion of the universe
  • causing it to contract back inwards into a singular point
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9
Q

what condition needs to be met in order for the expansion of the universe to forever continue

A
  • the matter in the universe has to be sparse

- specifically below a critical density

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10
Q

why does this condition need to be met

A
  • the force of gravity between particles decreases as the distance between them increases
  • if matter in the universe is sparse the gravitational forces between matter will be generally weak
  • meaning gravity wont ever be able to overcome the expansion of the universe
  • so it will continue forever
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11
Q

therefore what condition needs to be met for the big crunch

A

the matter in the universe has exceeded the critical density

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12
Q

what is a flat universe

A
  • a universe which reaches a size where its expansion and gravity are balanced
  • so its size doesnt change after it reaches its maximum size
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13
Q

what is a closed universe

A
  • a universe which reaches its maximum size
  • then will begin to contract due to gravity
  • the big crunch scenario basically
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14
Q

what is an open universe

A
  • a universe which continues expanding forever

- the ‘below critical density’ scenario

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15
Q

what would a graph of size over time look like for a flat, closed and open universe

A
  • the flat line would look like an logx graph (+ve gradient but naturally plateaus)
  • the closed line would look like a -x^2 graph (molehill)
  • the open line would be a straight line with a +ve gradient
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16
Q

when trying to work out the density of the universe, what did vera rubin discover about the stars in Andromeda

A
  • the stars in the galaxies tend to rotate at similar speeds

- whatever their distance from the centre of the galaxy

17
Q

why was this a peculiar find

A
  • because the stars closest to the centre shouldve been rotating at quicker speeds
  • similar to our solar system where the planets further away from the sun rotate slower
18
Q

what can we estimate from working out the luminosity of a galaxy

A

the mass of all its stars

19
Q

what force should all the stars in a galaxy be feeling if the galaxy is rotating

A

a centripetal force towards the centre of the galaxy

20
Q

what problem did scientists come across when measuring the rotational speed of the stars in the galaxy and their relationship to their mass suggested by the luminosity calculations

A
  • that their mass was not enough to create the centripetal force needed to keep the galaxy spinning
  • in other words, the gravitational centripetal force shouldnt have been enough to hold the stars in place against their rotational velocity
21
Q

what was the only conclusion the scientists had to make because of this

A

that galaxies contain a lot of mass that does not emit light

22
Q

what is this mystery mass called

A

dark matter

23
Q

what percentage of mass was actually detectable in the galaxies of that that shouldve actually been there

A

about 10%

24
Q

what two possible candidates did we have for dark matter

A
  • black holes

- interstellar gases

25
Q

yet what is the problem with these two suggestions

A
  • they are also not observed in sufficient quantities

- so even if they did contribute, there would still be more mystery matter present

26
Q

what does einsteins theory of gravity simply state

A
  • that large masses will deform space-time (the fabric of the universe)
  • so that it accelerates things
27
Q

how has his theory been supported by photos of deep space

A
  • we have observed light bending around large masses
  • like black holes or galaxies
  • rather than passing through them like a lens
  • suggesting space-time itself was curved
28
Q

what did the hubble space telescope discover about the expansion of the universe

A
  • it is not slowing down

- but it is actually accelerating

29
Q

where is this energy powering the accelerating expansion of the universe, which seems to defy its own gravity, coming from

A

we dont know

30
Q

what is the name given to this mystery energy

A

dark energy

31
Q

what are the percentages of ordinary matter, dark matter and dark energy that compose the universe

A
  • ordinary matter = 5%
  • dark matter = 27%
  • dark energy = 68%