12 - Current Scientific Cosmology Flashcards

1
Q

a branch of astronomical science that focuses on where everything came from (origin + development of the universe)

A

cosmology

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1
Q

places the universe timeline of events on a 12 month calendar (13.89Gy). In the last 30 seconds of this calendar, humanity was created

A

cosmic calendar

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2
Q

everything that exists

A

the universe

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3
Q

a portion of the universe that can be seen from your location in space/time (finite)

A

observable universe

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4
Q

time in years equal to the distance of the object in light years, ex to the moon its 1.3 seconds, sun is 8 mins, nearest star is 4 years from earth

A

look-back time

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5
Q

In theory, with the amount of stars we have in the universe, the night sky should be bright, but the night sky is not bright, and is mostly dark! What is this paradox called and what is its solution?

A

Olbers’ Theory
A. the most distant stars are so far away that light from them hasn’t reached earth. that’s why the night sky is dark because the universe had a beginning

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6
Q

galaxies are moving away from Earth at speeds proportional to their distance. In other words, the farther they are, the faster they are moving away from Earth

A

Hubble Law

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7
Q

The universe’s expansion rate

A

Hubble Constant

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8
Q

provides an estimate of the age of the universe based on the current rate of expansion. this helps us figure out the universe’s age (14 GY)

A

hubble time

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9
Q

radiation of hot matter of universe soon after big bang, found by accident. It’s a low hum from the birth of the universe

A

Cosmic Microwave Background (CMB)

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10
Q

universe matter + energy compressed into a high-density, high-temperature state

A

big bang

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11
Q

What are the four steps of the Big Bang?

A
  1. Inflation (exponential expansion of space/time)
  2. Hot Big Bang (radiation, nucleosynthesis)
  3. Recombination (dark age where nothing happens, continuation of expansion in darkness)
  4. Reionization (first stars, light - it’s bright again)
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12
Q

Isotropy (same observable properties) + Homogeneity (matter is uniformly spread) =

A

Cosmological Principle

observer in any galaxy sees the same general universe, the same general properties, minor local and evolutionary variations, no centre or edge.

provide a basis for the assumption that the physical laws that govern the universe are the same everywhere and in every direction on a large scale.

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13
Q

phenomenon in which the light emitted by objects in the universe appears to be shifted toward longer wavelengths, specifically toward the red end of the electromagnetic spectrum.

A

cosmic red shift

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14
Q

what are three models of the universe?

A
  1. open universe: space-time curved in, the universe is infinite
  2. closed universe: space time is curved to meet itself, finite universe
  3. space-time is not curved and grows forever
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15
Q

refers to the density of matter and energy required for the universe to be exactly flat on cosmological scales. It plays a crucial role in determining the overall geometry and fate of the universe.

A

critical density

16
Q

proposed dark matter particles other than protons and neutrons. It’s a mystery. Recent models suggest cold dark matter (made of slow moving particles)

A

Nonbaryonic matter

17
Q

why was the universe so close to exactly flat with no space-time curvature, at the time of the big bang?

A

flatness problem

18
Q

how did every part of the observable universe get to be so nearly the same temperature by the time of recombination?

A

Horizon Problem

19
Q

a solution that says there was an extra expansion in the big bang, where a very young universe expanded and cooled

A

inflationary big bang

20
Q

Einstein added to space-time equations representing force of repulsion modern astronomers believe drives acceleration

A

cosmological constant

21
Q

energy driving universe expansion acceleration

A

dark energy

22
Q

if dark energy increases with time, expansion acceleration shred galaxies, stars, and atoms

A

big rip

23
Q

distribution of superclusters in filaments of walls enclosing voids, the Sloan Great Wall is the largest known structure in the universe and it is 1.4 billion LY long

A

large-scale structure