Unit 12: Cosmology Flashcards

1
Q

What is the distance ladder?

A

Step 1: Parallax distances to measure luminosity of cepheids
Step 2: Cepheid distances to measure luminosity of SNe
Step 3: SNe to measure distances to far-away galaxies

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2
Q

What is Hubble time?

A

The estimate as to how old the Universe is; If the universe were to expand at a constant rate, then inverse of the expansion rate is the age

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2
Q

What is the difference between dark matter and dark energy?

A

-Dark matter: Yet to be found particles that make up most of the matter in the Universe
-Dark energy: Property of spacetime that makes space want to expand

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3
Q

Dark energy accounts for the majority of what?

A

Density

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4
Q

Since dark energy is a property of space and space expands, what happens to the relative fraction of dark energy?

A

It increases

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5
Q

What is the Cosmic Microwave Background?

A

The temperature of the Universe’s blackbody radiation decreases (from 3000K to 3000K/1100 since photons are redshifted by a factor of 1100). This puts the peak wavelength of the radiation at ~2mm, in the microwave range.

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6
Q

How do physicists predict the Universe will expand?

A

They predict that the Universe will expand forever at an increasing rate

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7
Q

What percent of matter IN TOTAL is dark matter?

A

25%

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8
Q

Of the 30% matter in the Universe, what percent is dark matter?

A

85%

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9
Q

Of the 5% of ordinary matter, what percent is in luminous galaxies?

A

1%

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10
Q

What two things combined tell us the distance of galaxies?

A

Their Hubble expansion rate and the redshift of galaxies

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