A) a significant fraction of its mass is in the form of globular clusters, distributed in a spherical halo centered on the galactic center.
B) a large black hole is slowly clearing out the mass near the galactic center, leaving a cold, dark void.
C) enormous amounts of energy are pouring out of a compact but very massive source at its center.
D) most of its mass is in the spiral arms extending out into space.
Correct Answer
verified
Multiple Choice
A) throughout the whole Galaxy
B) at the galactic center
C) in the disk and spiral arms
D) in globular clusters and in the galactic halo
Correct Answer
verified
Multiple Choice
A) Giant molecular clouds occur primarily in the spiral arms.
B) Giant molecular clouds are distributed uniformly throughout the disk.
C) Giant molecular clouds are concentrated close to the galactic center.
D) Giant molecular clouds are distributed throughout the halo, with greater density toward the center.
Correct Answer
verified
Multiple Choice
A) ultraviolet.
B) X-ray.
C) infrared.
D) radio.
Correct Answer
verified
Multiple Choice
A) distribution of globular clusters
B) distribution of O and B stars
C) distribution of emission nebulae (H II regions)
D) distribution of giant molecular clouds
Correct Answer
verified
Multiple Choice
A) Variable stars are important spiral arm tracers and thus defined the shape of the Milky Way Galaxy.
B) The brightness variations of variable stars allowed accurate distances to be measured.
C) Variable stars emit copious amounts of infrared radiation and are thus visible through interstellar dust that obscures visible light.
D) Variable stars are concentrated in the galactic center and so defined its direction.
Correct Answer
verified
Multiple Choice
A) 1.3 * 106 solar masses
B) 2.6 * 106 solar masses
C) 3.7 *106 solar masses
D) 9.4* 106 solar masses
Correct Answer
verified
Multiple Choice
A) Mars
B) Jupiter
C) Sun
D) Milky Way Galaxy
Correct Answer
verified
Multiple Choice
A) by counting stars, assuming an average stellar mass, and calculating the total mass
B) by observing the bending of light from distant galaxies as the light passes near the center of the Milky Way
C) by observing the movement of the Galaxy toward neighboring galaxies because of mutual gravitational attraction
D) by applying Kepler's law to the motion of the Sun and other nearby stars
Correct Answer
verified
Multiple Choice
A) it is relatively easily absorbed by hydrogen gas in the Milky Way, so measurements are not confused by emission of this radiation from other galaxies beyond the Milky Way. It originates only from cold hydrogen gas and can be used to map this important component.
B) radio waves easily penetrate the Milky Way dust and gas, and they are a very narrow-wavelength line emission; thus its Doppler shift can be used to measure gas motions.
C) Doppler shift of this narrow-wavelength line emission is caused by the temperature of the hot hydrogen gas and therefore can be used to measure the distribution and temperature of this important component of the Milky Way.
D) this emission can easily penetrate the Milky Way gas and dust and comes only from hot gas, hence its ability to be used to map the distribution of hot hydrogen gas.
Correct Answer
verified
Multiple Choice
A) the redshift of the more distant stars made them invisible to Herschel.
B) Herschel counted all "stars" in each star field and included many galaxies that were outside the Milky Way, thus confusing the distribution.
C) the large quantity of absorbing dust between stars obscured the more distant regions of the Galaxy.
D) emissions from hot hydrogen gas clouds served to hide the more distant stars, localizing his search.
Correct Answer
verified
Multiple Choice
A) the Milky Way Galaxy.
B) the Whirlpool Galaxy (M51) .
C) the Andromeda Galaxy (M31) .
D) the Small Magellanic Cloud.
Correct Answer
verified
Multiple Choice
A) gravitational radiation emitted by stars as they are swallowed by the black hole.
B) powerful magnetic fields in the huge filaments arching away from (or toward) the center.
C) the number of globular clusters that concentrate toward the galactic center.
D) the very high orbital speed of stars orbiting the galactic center.
Correct Answer
verified
Multiple Choice
A) The H-R diagram should always give larger distances.
B) The H-R diagram should always give smaller distances.
C) There should be no difference in the distances.
D) The distances should be different, but sometimes the H-R diagram should give the larger distance and sometimes the smaller distance depending on the actual distance to the cluster.
Correct Answer
verified
Multiple Choice
A) it emits synchrotron radiation at radio wavelengths.
B) its gravitational pull affects orbital motions in the Galaxy.
C) it bends light from distant quasars.
D) it blocks out the light from distant stars in the plane of the Galaxy.
Correct Answer
verified
Multiple Choice
A) the average velocity of nearby galaxies
B) the black hole at the galactic center
C) the average velocity of the globular clusters
D) cosmic background radiation
Correct Answer
verified
Multiple Choice
A) inside the spiral arms
B) in globular clusters
C) in the outermost regions of the disk, where much of the "dark matter" is located
D) between the spiral arms, where there is less absorbing material
Correct Answer
verified
Multiple Choice
A) the peak wavelength of their spectra and their surface temperatures.
B) their luminosity, or absolute magnitude, and their pulsation period.
C) the redshift of their spectra and their distance from the Sun.
D) their apparent magnitude and their pulsation period.
Correct Answer
verified
Multiple Choice
A) in the Scutum-Centaurus arm
B) in the Sagittarius arm
C) in the Perseus arm
D) between the Sagittarius and Perseus arms
Correct Answer
verified
Multiple Choice
A) measurement of the distances to stars
B) measurement of the rotation speeds of galaxies
C) measurement of the surface temperatures of stars
D) keeping of accurate time
Correct Answer
verified
Showing 121 - 140 of 157
Related Exams