Test 2 Flashcards

1
Q

Phases during stellar evolution

A

I. Collapse of a gas cloud to form a star (book stages 1-6)
II. Main Sequence (stage 7)
III. Red Giant
IV. Helium Flash
V. Second Red Giant (Asymptotic Giant Branch [AGB])
VI. Planetary Nebula and formation of White Dwarf

It is helpful to keep in mind that stars are a battle between
gravity and nuclear energy. And gravity always wins

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2
Q

What is the main sequence?

A

The energy of a main sequence star is produced by fusion of H to He in the star’s core.

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3
Q

What is hydrostatic balance

A

Recall that stars are a
balance between pressure
pushing stuff out and
gravity pulling stuff in.

Because stars are
constantly losing energy,
they would contract if it
were not for a heat source
(nuclear fusion) in the
center
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4
Q

What is the Red giant phase?

A
Eventually the star
gets hot enough to
burn hydrogen in the
outer layer around the
He core.
This is called
hydrogen shell
burning.

This is the Red Giant
stage

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5
Q

Why is a red giant red?

A

Because of the vast expansion, the photosphere
of a red giant is cooler - and therefore redder -
than that of the main sequence star from which it
evolved.
As the shell around the core burns, more helium
is added to the core, which contracts faster and
makes the shell still hotter, so the star keeps
getting larger and brighter.

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6
Q

What happens during stages 8 and 9

A
  1. The inner core has fused to helium and begins to contract
    and heat up.
  2. The core is now hot enough to drive a furious rate of fusion
    of H to He in a shell around the core. The outer part of the
    star vastly expands from the combined energy of contraction
    and furious shell burning. The core continues to contract and
    heat up.
    The red giant stage ends when the core is finally hot enough
    at 100 million K to fuse helium to carbon.
    Not all stars get to this point, which depends on
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7
Q

Helium Flash (stage 9)

A

For stars with M > 0.4 Msun, the temperature will reach 100
million K, hot enough to ignite the fusion of He in the core to
produce C.
Three helium nuclei combine to form a carbon nucleus:

4He + 4He + 4He → 12C
Fusion of helium to carbon begins explosively throughout the
core, and the burst of energy released is called the helium
flash. The core re-expands, the H burning in the shell slows
because the shell is now cooler, and the outer layers of the
star contract.

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8
Q

In an H-R diagram, stars with the smallest radius are found in the ___________ of the diagram

A

lower left corner

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9
Q

We know that giant stars are larger in diameter than the sun because

A

they are more luminous but have about the same temperature.

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10
Q

The most common stars are

A

lower main sequence stars

less luminous

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11
Q

The ____________ of a star is a measure of the total energy radiated by the star across all wavelengths in one second.

A

Luminosity

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12
Q

To determine the period of a visual binary, we must measure

A

position

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13
Q

Spectroscopic binaries are difficult to analyze because

A

We can’t see the shape of the orbit

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14
Q

Stars on the main sequence with the greatest mass

A

are spectral type O stars

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15
Q

An eclipsing binary will

A

always be a spectroscopic binary

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16
Q

In the HR diagram, 90% of all stars are

A

on the main sequence

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17
Q

Which star in the diagram is most like the sun?

A

HR 5337

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18
Q

Which star in the HR diagram above has the greatest surface temperature?

A

Alnilam

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19
Q

Which of the stars in the HR diagram above has the largest absolute visual magnitude?

A

Sirius B

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20
Q

To measure the parallax of the most distant stars measurable, we would make two measurements of the star’s position on the sky separated by

A

6 months

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21
Q

Parallax is used to measure a star’s

A

distance

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22
Q

How is the distance to a star related to its parallax?

A

Distance is inversely proportional to parallax

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23
Q

A parsec is measure of

A

size and distance

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24
Q

Star A and star B appear equally bright, but star A is twice as far from us as star B. Which of the following is true?

A

Star A is four times as luminous as star B

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25
Q

Star A and star B both have the same temperature, but different sizes and distances. As a result, star A is more luminous than star B, but star B is brighter than star A. Which of these statements about the absolute and apparent magnitudes of the two stars is correct?

A

Star A has a larger apparent magnitude, while star B has a larger absolute magnitude

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26
Q

Stars that have spectral type B _________ in temperature compared with stars that have spectral type M.

A

are hotter

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27
Q

Star A is a red star. Star B is a blue star. Which star is hotter?

A

Star B

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28
Q

Two stars with similar temperatures but different sizes will have

A

similar spectral types but different luminosities

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29
Q

Stars are mostly made of

A

Hydrogen

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30
Q

Star C is a red star. Star D is a blue star. Which has a larger radius?

A

We also need to know the luminosities of the stars to determine their radii

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31
Q

Star E is the same temperature as star F, but star E is four times as luminous as star F. How to the radii of the stars compare?

A

The radius of star E is twice that of star F

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32
Q

Which of the following is NOT evidence of the existence of an interstellar medium?

A

molecular absorption lines in the spectra of cool stars

`

33
Q

Compared with the spectral lines in the solar spectrum, lines in a supergiant star’s spectrum are

A

more narrow

34
Q

The spectra of most galaxies tell us that

A

most galaxies appear to be moving away from us

35
Q

Where are elements heavier than iron primarily produced?

A

Supernovae

36
Q

The explosion of a supernova typically leaves behind

a shell of

A

hot, expanding gas with a pulsar at the center.

37
Q

After what evolutionary stage does a star become a white dwarf?

A

Giant

38
Q

Stars that have ejected a planetary nebula eventually become

A

white dwarfs.

39
Q

What nuclear fusion mechanism does an isolated white dwarf use to generate energy?

A

White dwarfs don’t generate their own energy.

40
Q

What are the two longest stages in the life of a one solar mass star?

A

main sequence, white dwarf

41
Q

For a star of Sun-like mass, what is the last stage of the nuclear fusion?

A

helium to carbon and oxygen

42
Q

About how long will a 0.5 star spend on the main sequence?

A

57 billion years

43
Q

A planetary nebula has a radius of 0.5 pc and is expanding at 20 km/sec. What is the approximate age of this planetary nebula? (1 pc is equal to 3×1013 km, and 1 year is equal to 3.15×107 seconds.)

A

24,000 years

44
Q

The diagram below shows a light curve from a supernova. How many days after maximum light did it take for the supernova to decrease in brightness by a factor of 100?

A

150

45
Q

As a white dwarf cools its radius will not change because

A

pressure does not depend on temperature for a white dwarf because the electrons are degenerate.

46
Q

If the theory that novae occur in close binary systems is correct, then novae should

A

repeat after some interval.

47
Q

What does a planetary nebula produce?

A

an emission spectrum

48
Q

A white dwarf is composed of

A

carbon and oxygen nuclei and degenerate elections

49
Q

When material expanding away from a star in a binary system reaches the Roche surface

A

the material is no longer gravitationally bound to the star

50
Q

A nova is almost always associated with

A

a white dwarf in a close binary system.

51
Q

A planetary nebula is

A

the expelled outer envelope of a medium mass star.

52
Q

The lowest mass stars cannot become giants because

A

they cannot heat their centers hot enough.

53
Q

If the stars at the turnoff point of a cluster have a mass of 3 M, what is the age of the cluster?

A

6.4x10^8 years

54
Q

Stars in a star cluster all ____________

A

have the same age

have the same chemical composition

55
Q

Stars in a star cluster don’t have

A

the same Mass

56
Q

Helium flash occurs

A

because degenerate electrons in the core do not allow the core to expand as it heats up.

57
Q

star clusters are important to our study of stars because

A

they give us a method to test the theories and models of stellar evolution

58
Q

The Crab nebula is

A

a supernova remnant

59
Q

_______is a form of electromagnetic radiation produced by rapidly moving electrons spiraling through magnetic fields.

A

Synchrotron radiation

60
Q

Stars within a cluster that are at the turnoff point

A

have life expectancies that are equal to the age of the cluster

61
Q

A(n)______ is a collection of 105 to 106 stars in a region 10 to 30 pc in diameter. The stars in the collection tend to be more than 109 years old and mostly yellow and red stars.

A

globular cluster

62
Q

A(n) _______ is a collectin of 100 to 1000 stars in a region about 25 pc in diameter. The stars in the collection are typically quite young.

A

Open cluster

63
Q

What do you need to form stars

A

ionized gas in the Intercellular medium

64
Q

Shortwave light(blue) gets ___________ than long wavelight (red)

A

scattered more

65
Q

Stars form in regions that are

A

coldest and densest

66
Q

Absolute visual magnitude is

A

the apparent magnitude of a star observed from a distance of 10 pc.

67
Q

A star’s absolute magnitude depends only on the star’s

A

Temp and diameter

68
Q

In an H-R Diagram, stars with the smallest radius are found in the _______________ of the diagram.

A

Lower left corner

69
Q

In the H-R diagram, 90 percent of all stars are

A

On the main sequence

70
Q

We know giant stars are larger in diameter than the sun because

A

they are more luminous but have about the same temperature.

71
Q

Giant stars

A

I, II, III, & IV

72
Q

The most common stars are

A

lower main sequence stars

73
Q

The _______________ of a star is a measure of the total energy radiated by the star in one second

A

Luminosity

74
Q

What is the distance to a star that has a parallax angle of 0.5 arc seconds?

A

Two parsecs

75
Q

At what distance must a star be to have its apparent magnitude equal to its absolute magnitude?

A

10 parsecs

76
Q

How can a cool star be more luminous than a hot star?

A

It can be more luminous if it is larger.

77
Q

To which luminosity class does the mass-luminosity relationship apply?

A

The main sequence

78
Q

Which luminosity class has stars of the lowest density, some even less dense than air at sea level?

A

The supergiant

79
Q

In a given volume of space the Red Dwarf (or lower main sequence) stars are the most abundant, however, on many H-R diagrams very few of these stars are plotted. Why?

A

They have very low luminosity and are difficult to identify