Lecture 12 Flashcards

(33 cards)

1
Q

luminosity is the measure of what?

what is the unit?

A

E output

J/s = W

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

stefan boltzmann law is for what variables?

A

intrinsic luminosity (depending on radius and temp)

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

what does the hertzsprung russell diagram show?

A

luminosity of stars vs temperature

shows the main sequence, and other groups of stars (white dwarfs, giants, supergiants)

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

what does the main sequence represent?

A

all stars which have their primary E source as nuclear fusion of H

stars off the main sequence have a different primary E source

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

what is fusion of H also called?

A

H burning

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

describe the two components of hydrostatic equilibrium

A

forces pointing inward: pressure b/c of gravity

forces pointing outward: radiation pressure

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

what determines where a H burning star will sit on the main sequence?

A

mass

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

massive stars use nuclear fuel _____ than lighter stars

faster/slower?

A

faster

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

the lifetime of a star depends on what two factors?

A

mass of star (how much fuel it has)

luminosity of star (how fast it uses up fuel)

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

____ (high/low) mass stars stay on the main sequence for a ____ (long/short) time

A

high mass stars –> short time on MS

low mass stars –> stay on MS for long time

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

when does a star leave the main sequence?

what happens when this occurs?

A

when it runs out of H to fuse

star will move to red giant branch of HR diagram; the primary E source is still nuclear fusion, but the internal structure changes

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

a high turn off point means that the cluster is _____

a low turn off point means that the cluster is ___

A

young (at higher luminosity and temp)

old (at lower luminosity and temp)

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

what is used to measure masses of stars?

what is it?

A

binary star systems (when 2 stars are gravitationally bound and orbits around a common centre of mass)

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

with the doppler shift, is the frequency higher in front or behind the car?

A

higher frequency in front

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

in a blue shift, how is the wavelength affected?

A

shorter wavelength

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

in a red shift, how is the wavelength affected?

A

longer wavelength

17
Q

motion AWAY from observer causes which type of shift?

18
Q

motion TOWARD observer causes what type of shift?

19
Q

stars with higher velocity have ____ (lower/higher) mass

20
Q

how can you determine mass ratio of stars?

A

double line binary

21
Q

how can you determine orbital inclination angle

A

single line binary

22
Q

which binary gives all information about orbit and masses?

A

binary must be visual/eclipsing AND double-line

23
Q

cooler stars are ____ massive than hotter stars

24
Q

what are 4 phases of stellar evolution?

A

1) formulation and pre main sequence
2) main sequence
3) post main sequence
4) death

25
describe star formation
- forms from gas in molecular clouds - lots of dust which obscures light (only infrared light can be seen) - star formation regions appear dark and reddish
26
describe the "core" in star formation
- formed due to high density - cores collapse gravitationally - as core material becomes more dense, nuclear rxns begin - this leaves a pre-main sequence star which is supported from further collapse
27
what is the protostar?
pre-main sequence star undergoing gravitational collapse b/c of little inside pressure
28
describe the pre-main-sequence star?
interior pressure increases, which slows collapse no nuclear rxns yet very bright and short phase
29
in the pre main sequence, where does the star get E from?
gravitational E
30
do all protostars get to MS? why?
no b/c you need M>0.08 solar masses to have enough gravity for nuclear rxns to begin
31
what are brown dwarfs?
objects that didn't make it to star status
32
describe protostars with M>100 solar masses
v unstable and easily will explode
33
what is ZAMS?
zero age main sequence where stars of same chemical composition start