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What is the main component of the central bulge of our galaxy?


A) gas and dust
B) population I stars
C) stars associated with the spherical component of our galaxy
D) stars associated with the disk component of our galaxy

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  -In the diagram,the approximate absolute magnitude of a Type II Cepheid with a period of 30 days is _________________. -In the diagram,the approximate absolute magnitude of a Type II Cepheid with a period of 30 days is _________________.

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Which of the following is NOT explained by the traditional theory of the formation of our galaxy?


A) the existence of the nuclear bulge
B) the existence of the disk of the galaxy
C) the fact that the oldest stars in the galaxy are not metal-free
D) the difference in metal abundance of the population I and II stars

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What do radio maps of the spiral arms of our galaxy show?


A) They reveal that our galaxy is a grand design spiral.
B) They map the location of dense neutral hydrogen clouds.
C) They reveal that the Sun is currently located in the centre of a spiral arm.
D) They map the location of hot O and B stars by the radio radiation they emit.

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Why does the rotation of our galaxy suggest that it is more massive than previously thought?

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  -Refer to the figure.Polaris is a Type I Cepheid with a period of 4 days.What is its absolute magnitude? A) +1 B) 0.0 C) -1.0 D) -3.5 -Refer to the figure.Polaris is a Type I Cepheid with a period of 4 days.What is its absolute magnitude?


A) +1
B) 0.0
C) -1.0
D) -3.5

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What is the difference between a population I star and a population II star?

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The orbits of halo stars are typically circular and have a low inclination with respect to the disk.

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Giant molecular cloud complexes are located in spiral arms.

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How does the traditional theory of the formation of the galaxy explain the origin of globular clusters?


A) They formed in the disk and were later ejected to the halo.
B) They built up over time from the collisions of stars in the halo.
C) They formed in other galaxies and were captured by close interactions.
D) They formed early on during the free-fall collapse of the proto-galactic material.

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Discuss how astronomers know that our galaxy contains spiral arms in its disk.

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The disk of the galaxy is older than the halo.

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  -Refer to the figure.If you observe the period of a type II Cepheid and mistakenly think it's a type I Cepheid,what incorrect conclusion will you draw? A) You will measure the wrong period. B) You will think the Cepheid is farther away than it actually is. C) You will think the Cepheid is closer than it actually is. D) You will think the Cepheid is less luminous than it actually is. -Refer to the figure.If you observe the period of a type II Cepheid and mistakenly think it's a type I Cepheid,what incorrect conclusion will you draw?


A) You will measure the wrong period.
B) You will think the Cepheid is farther away than it actually is.
C) You will think the Cepheid is closer than it actually is.
D) You will think the Cepheid is less luminous than it actually is.

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How does the density wave theory explain the presence of young stars in the spiral arms?

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Why are O and B stars good tracers of spiral structure?


A) They are young and luminous.
B) They are old and have been part of the galaxy for a long time.
C) They are young and moving with large radial velocities.
D) They were formed in the galaxy's halo.

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If spiral density waves were the only thing producing spiral arms,what result would be expected?


A) All spiral arms would be gas- and dust-free.
B) All galaxies would have only two smooth spiral arms.
C) The Milky Way would show an irregular pattern of short arms.
D) The halo component of the Milky Way would show spiral arms as well.

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Spiral tracers tend to be old,luminous stars.

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What behaviour of galactic rotation curves suggests the existence of dark matter in an extended halo?


A) Small velocities are seen at large distances from the galactic centre.
B) Small velocities are seen at distances close to the galactic centre.
C) Large velocities are seen at large distances from the galactic centre.
D) Large velocities are seen at distances close to the galactic centre.

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What is the difference between an open cluster,an association,and a globular cluster? In which parts of the galaxy is each found?

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Answered by ExamLex AI

Answered by ExamLex AI

Open clusters, also known as galactic cl...

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Compare and contrast the properties of disk and halo stars.

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