Astrophysics and Stellar Evolution: Key Concepts and Laws

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66 Terms

1
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How do the laws of physics change for moving observers?

None of the laws change.

2
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What did Einstein show about Newton's physics?

Accurate only at low velocities.

3
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What ultimately determines an isolated star's fate?

Mass.

4
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As a star moves along the red giant branch, how does it move on the HR diagram?

Upward and to the right.

5
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During which evolutionary phases will the Sun undergo fusion in its core?

Main sequence and horizontal branch.

6
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How were essentially all elements heavier than iron formed in our Milky Way?

By supernovae.

7
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Why is the Schwarzschild radius significant?

It is the distance within which nothing can escape a black hole.

8
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What do astronomers believe exists in the center of nearly every galaxy?

A black hole.

9
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What happens to the central temperature and luminosity of a low-mass protostar as it approaches the main sequence?

Temperature increases; luminosity decreases.

10
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Why do massive stars use the CNO cycle instead of the proton-proton chain?

Massive stars have hotter cores; increased temperature sensitivity of the CNO cycle allows for greater energy production.

11
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What kind of stars are most likely to form black holes?

Stars with masses greater than 30 solar masses.

12
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What stops the collapse of the most massive stars at the end of their lives?

Nothing.

13
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Which type of light is most strongly affected by interstellar dust?

Visible light.

14
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Why does stellar fusion end with an iron core?

Iron does not produce energy when it undergoes fusion.

15
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What will the Sun end its life as?

White dwarf.

16
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Which object is closest in radius to a neutron star?

A small city.

17
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What does the general theory of relativity explain?

Gravity and space-time.

18
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Why does a satellite orbit Earth according to general relativity?

Earth has deformed space-time so the satellite falls freely through it.

19
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How has stellar evolution been best understood?

By analyzing the properties of a large number of stars at a single instant.

20
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What quantities must be measured to calculate the luminosity of a star?

Brightness and distance.

21
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Which energy transport mechanism does NOT occur significantly in the Sun?

Conduction.

22
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What forces maintain hydrostatic equilibrium in an object?

Pressure and gravity.

23
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What determines the location of a star on the main sequence?

Mass.

24
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How do massive stars burn their fuel compared to low-mass stars?

They burn their fuel rapidly, so they have shorter lifetimes.

25
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What can an astronomer determine from an HR diagram of a star cluster?

The age of the cluster.

26
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What powers a star?

Fusion.

27
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What has provided the best data about the interior of the Sun?

Helioseismology.

28
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What is created by solar magnetic activity?

All of the above (sunspots, prominences, coronal mass ejections, solar flares).

29
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When does a fusion reaction between nuclei A and B release energy?

If the resulting nucleus is less massive than the total mass of A and B.

30
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What is a key constituent of the interstellar medium?

Gas and dust.

31
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What principle is responsible for accretion disks forming around protostars?

Conservation of angular momentum.

32
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When does a protostar become a star?

When nuclear fusion begins.

33
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What is a brown dwarf?

A failed star.

34
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What is the order of spectral types of stars from hottest to coolest?

OBAFGKM.

35
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Why can Type Ia supernovae be used to determine a galaxy's distance?

Most Type Ia supernovae have approximately the same luminosity.

36
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How do neutrinos help us understand the core of the Sun?

Neutrinos from the interior of the Sun easily escape.

37
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What does the Initial Mass Function tell astronomers about stellar masses?

There are more low mass stars than high mass stars.

38
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What is required for nuclear fusion to occur?

Extremely high temperatures for protons and neutrons to collide at high velocities.

39
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What describes changes to a star when it first moves off the main sequence?

Increased radius and decreased surface temperature, increased luminosity.

40
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What are the seven spectral categories of stars in order from coolest to hottest?

MKGFABO.

41
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When do the predictions of Special Relativity match those of Newtonian physics?

When objects are moving slowly.

42
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What is the definition of a standard candle?

An object whose luminosity is known.

43
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How is heat transported from the bottom of a pot to the water's surface?

Convection.

44
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What energy source begins nuclear fusion in a protostar?

The gravitational potential energy of the protostar.

45
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What primarily makes it difficult to observe star formation?

They occur in dusty regions.

46
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What is the result of mass distorting the fabric of spacetime?

Gravity.

47
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What primarily causes solar activity?

The magnetic field of the Sun.

48
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What does the Chandrasekhar limit refer to?

The maximum mass of a white dwarf.

49
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What will observers in different inertial frames of reference always agree on?

The laws of physics.

50
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What forms a planetary nebula?

The ejection of mass from a low-mass star.

51
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How can black holes that are stellar remnants be found?

By searching for variable X-ray sources.

52
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What does the HR diagram of a cluster not tell astronomers?

The rotation of the cluster.

53
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What is true about white dwarfs?

They first appear at the center of a planetary nebula.

54
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Why are about 90% of the stars we observe on the main sequence?

Stars spend most of their life on the main sequence.

55
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Why can an iron core not support a massive main-sequence star?

Because iron cannot fuse to make heavier nuclei and produce energy.

56
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What is the order of the layers of the Sun from inside to outside?

Core → Radiative Zone → Convective Zone → Photosphere → Chromosphere → Corona.

57
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Why do sunspots appear dark?

They are cooler than their surroundings.

58
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What type of star is located on the upper right of the HR diagram?

A giant.

59
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What does the main sequence show?

The distribution of core hydrogen-fusing stars by mass.

60
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Which type of star has the highest density?

Neutron star.

61
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How often does the number of sunspots and their location change?

Over an 11-year cycle.

62
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How are elements heavier than iron formed?

In supernova explosions.

63
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Which figure represents the oldest star cluster?

Figure D.

64
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The Sun will undergo fusion in its core during which evolutionaery phases?

Main sequence and horizontal branch

65
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Nuclear fusion requires extremely high temperatures so that collisions of protons and neutrons occur at velocities high enough to overcome the strong nuclear force

True

66
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Why do massive stars use the CNO cycle to generate energy, rather than the proton-proton chain?

Because massive stars have hotter cores; the increased temperature sensitivity of the CNO cycle allows for greater energy production.