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The first stars to form in our galaxy


A) had circular orbits.
B) had highly elongated elliptical orbits.
C) were population I stars.
D) all had orbits in the same plane.
E) formed the galactic clusters we see today.

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___________ of the Milky Way contains mostly old (population II) stars and globular clusters.


A) The disk component
B) The spherical halo component
C) The hydrogen gas in the disk
D) The spiral arms
E) Sgr A*

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  What color in the above image best represents the bulge? A)  pink B)  blue C)  black D)  milky white What color in the above image best represents the bulge?


A) pink
B) blue
C) black
D) milky white

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The Herschels' grindstone model of the Milky Way star system was too small because


A) they did not count the brightest stars.
B) they did not study the southern sky.
C) they did not have large enough telescopes.
D) they only observed stars in the disk of the galaxy and not the halo.
E) they did not know about interstellar dust clouds.

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Compared to stars within the disk, halo stars


A) orbit at random inclinations to the galactic plane
B) orbit at different speeds
C) orbit with paths crossing
D) All of the other choices are correct.

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Spiral tracers tend to be old, luminous stars.

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  The galaxy shown above is ___________. A)  a grand design B)  a flocculent C)  in between a grand design and a flocculent D)  the Milky Way galaxy The galaxy shown above is ___________.


A) a grand design
B) a flocculent
C) in between a grand design and a flocculent
D) the Milky Way galaxy

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What evidence do we have that the center of our galaxy is a powerful source of energy and a supermassive black hole?

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A stronomers have been able to use large...

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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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The disk of our galaxy consists of


A) the nine known planets.
B) only stars.
C) stars, dust, and gas.
D) quasars.
E) only black holes.

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Stars motion within the disk of the Milky Way galaxy are ordered in that they the all go in the same direction, counter-clockwise, as viewed from above (e.g., as viewed from above the north rotational axis of the Sun),

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How did Harlow Shapley use the period-luminosity relationship of RR Lyrae variables to determine the size of the Milky Way galaxy?


A) He determined the proper motion of globular clusters in the outer disk of the galaxy.
B) He found the distances to individual variables free floating in the halo.
C) He found the distances to open clusters found throughout the disk of the galaxy.
D) He found the distances to globular clusters distributed about the center of the galaxy.

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  The blue color in this visual wavelength image indicates A)  globular clusters. B)  halo stars. C)  young stars. D)  cool stars. The blue color in this visual wavelength image indicates


A) globular clusters.
B) halo stars.
C) young stars.
D) cool stars.

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Old stars are poor in heavy elements because there were very few previous generations of stars before the old stars formed.

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

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The best observations of the rotation cu...

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Good tracers of the spiral arms of our galaxy are all I. very old. II. very young. III. very luminous. IV. moving with large radial velocities.


A) I & III
B) I & IV
C) II & III
D) II & IV
E) I, III, & IV

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​ Compare and contrast the properties of disk and halo stars.

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Most of the stars in the disk are mid...

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  Which mass star experiences more pulsations than the others shown at the time the systems were plotted in the above H-R diagram? A)  9-solar-mass star B)  5-solar-mass star C)  3-solar-mass star D)  RR Lyrae Which mass star experiences more pulsations than the others shown at the time the systems were plotted in the above H-R diagram?


A) 9-solar-mass star
B) 5-solar-mass star
C) 3-solar-mass star
D) RR Lyrae

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____________________ are groups of 100,000 to 1,000,000 population II stars firmly bound by gravity.

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The center of our galaxy is located in the direction of the constellation of Orion.

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