The Expanding Universe Flashcards

(39 cards)

1
Q

what did 20th century astronomers photograph?

A

the spectra of galaxies

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
2
Q

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

A

Doppler shift, and thus the radial velocity

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
3
Q

Vesto Slipher

A

1912: obtained 1st measurement of Andromeda galaxy

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

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
4
Q

how many galaxies were redshifted (moving away from us)

A

21 out of 25 galaxies

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
5
Q

what did Hubble work to obtain?

A

distances to the galaxies

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
6
Q

what did Hubble use to measure distances to galaxies?

A

Cepheid variable stars

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
7
Q

Hubble’s 1929 Discovery

A

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

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
8
Q

what two things did Hubble deal with?

A

recessional velocity and distance

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
9
Q

Spectra

A

the combined light of many stars

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
10
Q

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

A

you can derive the recession velocity

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
11
Q

what is the most fundamental method for distance?

A

stellar parallax

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
12
Q

brightness formula

A

luminosity/4 x pi x d^2

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
13
Q

what are 3 standard candles

A

main sequence stars
cepheid variable stars
type 1a supernovae

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
14
Q

type 1a is related to what kind of star

A

white dwarf

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
15
Q

what are cepheid variable stars

A

pulsating stars that vary in light output

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
16
Q

combining brightness and lumin. gives you

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

24
Q

what is the Hubble law telling us about the universe?

A

that it’s expanding

25
are we in a preferred location in the universe?
NO
26
Einstein's cosmological constant
opposes gravity and makes Universe static
27
George Lemaitre
proposed that the observed recession of galaxies was evidence for the expansion
28
Big Bang Universe
A universe w/ a well defined beginning | -time where separation of galaxies was very small
29
Nature of the Expansion of Universe
doesn't have a center, but rather the "fabric" of space time carrying the galaxies is expanding
30
If fabric of space/time expands by a factor of two, the distance b/w galaxies will...?
increase by a factor of 2
31
why are galaxies redshifted?
not due to doppler shift, but due to expansion of space
32
cosmological redshift
wavelength of light is stretched as Universe expands
33
redshift
shift of spectral lines to longer wavelengths
34
redshift formula
z = obs wav - emitted wav/emitted wav
35
when you measure cosmological redshift, we often express it as...?
a recession velocity
36
What to use to measure distance to very distant galaxies?
Hubble law | v = H x d
37
redshift can be used as a measure of what?
distance
38
what device performed the largest redshift survey of galaxies?
SDSS | Sloan Digital Sky Survey
39
cosmic web
non uniform distribution of galaxies and galaxy clusters