The Expanding Universe Flashcards

1
Q

what did 20th century astronomers photograph?

A

the spectra of galaxies

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2
Q

what did the photos of spectra of galaxies allow astronomers to measure?

A

Doppler shift, and thus the radial velocity

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3
Q

Vesto Slipher

A

1912: obtained 1st measurement of Andromeda galaxy

- determined it was moving toward us at 300 km/s

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4
Q

how many galaxies were redshifted (moving away from us)

A

21 out of 25 galaxies

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5
Q

what did Hubble work to obtain?

A

distances to the galaxies

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6
Q

what did Hubble use to measure distances to galaxies?

A

Cepheid variable stars

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7
Q

Hubble’s 1929 Discovery

A

the further away a galaxy was, the larger the recessional velocity

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8
Q

what two things did Hubble deal with?

A

recessional velocity and distance

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9
Q

Spectra

A

the combined light of many stars

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10
Q

what measurement can you get from the spectra of a galaxy?

A

you can derive the recession velocity

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11
Q

what is the most fundamental method for distance?

A

stellar parallax

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12
Q

brightness formula

A

luminosity/4 x pi x d^2

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13
Q

what are 3 standard candles

A

main sequence stars
cepheid variable stars
type 1a supernovae

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14
Q

type 1a is related to what kind of star

A

white dwarf

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15
Q

what are cepheid variable stars

A

pulsating stars that vary in light output

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16
Q

combining brightness and lumin. gives you

A

the distance

17
Q

key project for Hubble space telescope

A

using Cepheids to determine distance to galaxies (w/in 25 Mpc)

18
Q

what do type 1a supernova result from

A

detonation of white dwarf stars

19
Q

when do white dwarf stars detonate

A

slightly after mass exceeds 1.4 solar masses

20
Q

Type 1a luminosity

A

very luminous 9detected at over 1 billion pc)

21
Q

what can be serve as cosmological probes?

A

type 1a supernova, since they can be detected from billions of parsecs away

22
Q

Hubble’s law

A

relation b/w distance and velocity

23
Q

Hubble Law formula

A

v = H x d

24
Q

what is the Hubble law telling us about the universe?

A

that it’s expanding

25
Q

are we in a preferred location in the universe?

A

NO

26
Q

Einstein’s cosmological constant

A

opposes gravity and makes Universe static

27
Q

George Lemaitre

A

proposed that the observed recession of galaxies was evidence for the expansion

28
Q

Big Bang Universe

A

A universe w/ a well defined beginning

-time where separation of galaxies was very small

29
Q

Nature of the Expansion of Universe

A

doesn’t have a center, but rather the “fabric” of space time carrying the galaxies is expanding

30
Q

If fabric of space/time expands by a factor of two, the distance b/w galaxies will…?

A

increase by a factor of 2

31
Q

why are galaxies redshifted?

A

not due to doppler shift, but due to expansion of space

32
Q

cosmological redshift

A

wavelength of light is stretched as Universe expands

33
Q

redshift

A

shift of spectral lines to longer wavelengths

34
Q

redshift formula

A

z = obs wav - emitted wav/emitted wav

35
Q

when you measure cosmological redshift, we often express it as…?

A

a recession velocity

36
Q

What to use to measure distance to very distant galaxies?

A

Hubble law

v = H x d

37
Q

redshift can be used as a measure of what?

A

distance

38
Q

what device performed the largest redshift survey of galaxies?

A

SDSS

Sloan Digital Sky Survey

39
Q

cosmic web

A

non uniform distribution of galaxies and galaxy clusters