Multiple Choice
Identify the
letter of the choice that best completes the statement or answers the question.
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1.
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Which
of the following is not a characteristic of the stars of the disk component of our
galaxy? a. | circular
orbits | b. | randomly inclined orbits | c. | higher metal
abundance | d. | young stars | e. | star formation
regions | | |
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2.
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Younger stars have more heavy elements because a. | old stars
destroy heavy elements as they age. | b. | young stars burn their nuclear fuels
faster. | c. | the heavy elements were made in previous generations of
stars. | d. | heavy elements haven't had time to settle to the core of these
younger stars. | e. | all of these | | |
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3.
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The
first stars to form in our galaxy a. | had circular orbits. | b. | had highly
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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4.
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Good
spiral tracers 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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5.
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Radio
maps of our galaxy show spiral arms because a. | the arms have larger Doppler shifts. | b. | the gas in the
spiral arms is very hot. | c. | the dust in spiral arms is denser. | d. | the gas in
spiral arms is denser. | e. | the stars in the spiral arms emit most of their energy at radio
wavelengths. | | |
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6.
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Population II stars
I. | are primarily
found in the disk of the galaxy. | II. | contain more heavy metals than population I
stars. | III. | are primarily old low mass stars. | IV. | are located in
globular clusters. | | |
a. | III &
IV | b. | I &
II | c. | II | d. | IV | e. | I, II, & III | | |
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7.
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The
chemical abundance of population I stars a. | indicates that they were formed before the population II
stars. | b. | indicates that the material they formed from had been enriched
with material from supernovae. | c. | indicates that they contain very few heavy metals compared to
halo stars. | d. | depends on the temperature of the
star. | e. | depends on the mass of the star. | | |
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8.
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The
center of our galaxy lies in the direction of the constellation of a. | Ursa
Minor. | b. | Ursa Major. | c. | Sagittarius. | d. | Orion. | e. | Monoceros. | | |
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9.
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The
nuclear bulge of our galaxy a. | contains stars that are primarily population I
stars. | b. | contains relatively large amounts of gas and
dust. | c. | contains stars primarily associated with the spherical
component of our galaxy. | d. | contains stars primarily associated with the disk component of
our galaxy. | e. | a, b and d | | |
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10.
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The
orbits of population I stars
I. | are confined to
disk of the galaxy. | II. | are very elliptical. | III. | are nearly
circular. | IV. | are randomly inclined to the disk of the
galaxy. | | |
a. | I | b. | IV | c. | I & IV | d. | II &
IV | e. | I &
III | | |
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11.
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Radio
maps of the spiral arms of our galaxy a. | reveal that our galaxy is a grand design
spiral. | b. | map the location of Hot O and B stars by the radio radiation
they emit. | c. | reveal that the spiral arms are winding up and growing closer
together. | d. | reveal that the sun is currently located in the center of a
spiral arm. | e. | map the location of dense neutral hydrogen
clouds. | | |
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12.
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Sgr
A* is believed to be the center of the Milky Way galaxy because
I.
| It lies in the general direction of the center of the galaxy based on
observations of globular clusters. | II.
| It is located near the galactic corona. | III. | It is easily visible with optical telescopes and has the
appearance of a massive black hole. | IV.
| It does not move with respect to the rest of the
galaxy. | | |
a. | I &
II | b. | II &
III | c. | I &
IV | d. | II &
IV | e. | I, III, &
IV | | |
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13.
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A
Type I Cepheid has been located in an open cluster. The period of the Cepheid variable is 30 days and
the variables apparent visual magnitude is 10. What is the distance to this open
cluster?
a. | 100
pc | b. | 10,000
pc | c. | 20
pc | d. | 300
pc | e. | 2500
pc | | |
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14.
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An E
galaxy contains a. | mostly
lower-main sequence stars and giants. | b. | mostly upper main sequence stars and
giants. | c. | mostly upper main sequence stars and gas and
dust. | d. | roughly equal numbers of upper and lower main sequence
stars. | e. | mostly white dwarfs and supergiants. | | |
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15.
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An
irregular galaxy contains a. | mostly lower-main sequence stars and
giants. | b. | mostly upper main sequence stars and
giants. | c. | mostly upper main sequence stars and gas and
dust. | d. | mostly upper and lower main sequence stars and gas and
dust. | e. | mostly white dwarfs and supergiants. | | |
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16.
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The
look-back time is a. | how long the
light from an object takes to reach Earth. | b. | numerically equal to the distance in
light-years. | c. | smaller for more distant objects. | d. | all of the
above | e. | a and b above | | |
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17.
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Astronomers now speculate that a galaxy's shape depends on all of the following
except a. | the rate of star
formation. | b. | the history of past collisions. | c. | the
mass. | d. | the chemical composition. | e. | All of these are
important in determining a galaxy's shape. | | |
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18.
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We
should expect galaxies to collide fairly often because a. | they are large
with respect to their separation distances. | b. | galaxies contain
large amounts of neutral hydrogen. | c. | galaxies occur in clusters. | d. | a and
c | e. | none of the
above | | |
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19.
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A
tuning fork diagram is shown below. Which of the labeled figures represents an SBa
galaxy?
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20.
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A
tuning fork diagram is shown below. Which of the labeled figures represents an Sc
galaxy?
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21.
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A
tuning fork diagram is shown below. Which of the labeled figures represents an SBc
galaxy?
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22.
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A
tuning fork diagram is shown below. Which of the labeled figures represents an E0
galaxy?
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23.
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_________ galaxies contain large clouds of gas and dust, both young and old stars, but
have no obvious spiral arms or nucleus. a. | Irregular | b. | S0 | c. | E7 | d. | Sa | e. | E0 | | |
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24.
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The
dark matter in galaxies has been hypothesized to be composed of a. | neutral hydrogen
clouds. | b. | red dwarfs. | c. | weakly
interacting massive particles. | d. | H II regions. | e. | all of the
above. | | |
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25.
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Observations of galaxies and clusters of galaxies indicate that about _________ per
cent of the universe is dark matter.
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26.
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Starburst galaxies a. | contain a large number of very young stars, but very little
evidence of gas clouds. | b. | contain a large number of very old stars and almost no gas or
dust. | c. | are often associated with a galaxy that is colliding with
another galaxy. | d. | are common in rich clusters. | e. | are composed of
filaments and voids. | | |
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27.
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An
elliptical galaxy could a. | evolve into an irregular galaxy when it has used up all of its
gas and dust. | b. | be formed from the collision and merger of spiral
galaxies. | c. | evolve from a single spiral galaxy when the spiral has used up
all of its gas and dust. | d. | become a starburst galaxy if it were to move through the hot
intergalactic medium of a cluster. | e. | evolve from an S0 galaxy if the S0 galaxy were to increase its
rotation rate. | | |
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28.
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If a
galaxy has a radial velocity of 8000 km/sec and the Hubble constant is 70 km/sec/Mpc, what is the
distance to this galaxy? a. | 8.75 x 103 Mpc | b. | 2.4 x
109 Mpc | c. | 5.6 x 105 Mpc | d. | 114
Mpc | e. | 8.75 x
10-3 Mpc | | |
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29.
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If
the absolute magnitude of a supernova is -19 and a galaxy is found that contains a supernova with an
apparent magnitude of 16, what is the distance to the galaxy? a. | 100
AU | b. | 100
pc | c. | 100
ly | d. | 100
kpc | e. | 100
Mpc | | |
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30.
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The
radio lobes that flank some radio galaxies produce mainly a. | 21-cm
radiation. | b. | synchrotron radiation. | c. | black body
radiation. | d. | emission lies due to hydrogen. | e. | absorption lines
due to hydrogen. | | |
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31.
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Centaurus A is a radio galaxy that has a galaxy at the center. This central galaxy of
Centaurus A contains an elliptical galaxy encircled by a ring of dust. The elliptical galaxy rotates
about an axis that is in the plane of the dust ring. The dust ring rotates about an axis that is
perpendicular to the axis of rotation of the elliptical galaxy. What does this suggest about this
central galaxy of Centaurus A? a. | The radio jets have caused the dust disk to be driven around
the elliptical galaxy. | b. | There are at least two black holes at the center of the
elliptical galaxy. | c. | Centaurus A is probably the result of a merger of an elliptical
galaxy and a spiral galaxy. | d. | Dust is produced as the jets interact with the intergalactic
medium. | e. | Elliptical galaxies often contain dust that forms a disk along
their rotation axis. | | |
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32.
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If
the red shifts of quasars arise from the expansion of the universe, a. | a quasar must be
very small. | b. | a quasar must be within the Local
Group. | c. | a quasar must be single star with an extremely large
mass. | d. | a quasar must be moving toward Earth with a large radial
velocity. | e. | a quasar must be very luminous. | | |
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33.
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We
suspect that quasars are the active centers of galaxies because a. | quasar fuzz
produces stellar spectra. | b. | a few quasars have large red shifts. | c. | some quasars
fluctuate rapidly. | d. | all of the above. | e. | none of the
above | | |
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34.
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The
discovery of the gravitational lens effect for quasars a. | shows that
quasars were located within the local group of galaxies. | b. | shows that
quasars were giant elliptical galaxies at very great distances. | c. | shows that
quasars are much further away than the distant galaxy that forms the gravitational
lens. | d. | proves Newton's theory of gravitation by showing that the
photon was affected by gravity. | e. | proves the existence of super massive black holes at the center
of active galactic nuclei. | | |
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35.
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Statistical evidence a. | can be used to draw conclusions about a specific
cases. | b. | is applicable to classes of objects where only a few objects
from the class have been studied. | c. | allows scientists to determine the mechanism that produces the
dust ring in Centaurus A. | d. | allows scientists to deduce general characteristics about a
class of objects with similar properties. | e. | provides insight into the behavior of an individual object
based on careful observations of it. | | |
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36.
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Evidence that supports quasars being the nuclei of very distant galaxies
includes a. | the existence of
quasar fuzz. | b. | the observation of a supernova near a quasar and at the same
distance. | c. | gravitational lensing of some quasars by nearby
galaxies. | d. | all of the above | e. | none of the
above | | |
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37.
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A BL
Lac object is the same as a a. | Type 1 Seyfert. | b. | Type 2
Seyfert. | c. | double-lobed radio galaxy. | d. | blazar. | e. | quasar. | | |
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38.
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_________ is (are) observed when light from a distant quasar travels past a massive
galaxy between us and the quasar, and this light is focused to form two or more images of the same
quasar. a. | A double-lobed
radio galaxy | b. | Superluminal expansion | c. | The
gravitational lens effect | d. | A blazar | e. | Gravitational
waves | | |
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39.
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Seyfert galaxies a. | are more common in close pairs of galaxies than in isolated
systems. | b. | emit more energy at x-ray, ultraviolet, infrared, or radio
wavelengths than normal spiral galaxies. | c. | generally show red shifts greater than
1. | d. | a and
b | e. | a, b and
c | | |
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40.
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The
assumption of universality states that a. | the universe looks the same at all
epochs. | b. | the universe looks the same from all locations over
sufficiently great distances. | c. | the universe looks the same in all directions over sufficiently
great distances. | d. | the physical laws we observe on Earth apply everywhere in the
universe. | e. | all of the above | | |
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41.
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The
assumption of isotropy states that a. | the universe looks the same at all
epochs. | b. | the universe looks the same from all locations over
sufficiently great distances. | c. | the universe looks the same in all directions over sufficiently
great distances. | d. | all of the above | e. | none of the
above. | | |
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42.
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The
assumption of homogeneity states that a. | the universe looks the same at all
epochs. | b. | the universe looks the same from all locations over
sufficiently great distances. | c. | the universe looks the same in all directions over sufficiently
great distances. | d. | all of the above | e. | none of the
above. | | |
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43.
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During the first moments of the big bang, nuclear fusion reactions made few heavy
elements because a. | all heavy nuclei
are unstable. | b. | no stable nuclei exist with masses of 5 or 8 hydrogen
masses. | c. | the helium nucleus is unstable. | d. | the temperature
and density were too low. | e. | no nuclei heavier than helium could form since there weren't
any electrons formed. | | |
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44.
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If
galaxy A is four times more distant than galaxy B, then according to the Hubble Law, galaxy A will
recede ___________ than galaxy B. a. | 16 times faster | b. | 4 times
faster | c. | 2 times faster | d. | 1.2 times
faster | e. | 0.25 times faster | | |
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45.
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The
universe is said to be closed if
I. | gravity is
strong enough to stop the expansion in a finite time. | II. | the density of the universe is less than the critical
density. | III. | the universe is finite. | | |
a. | I & II | b. | I &
III | c. | II &
III | d. | I, I, &
III | e. | none of the
above | | |
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46.
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If
the universe is closed, then its age will be a. | less than two-thirds of 1/H. | b. | more than
two-thirds of 1/H. | c. | equal to 1/H | d. | equal to H
squared. | e. | equal to the square-root of H. | | |
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47.
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If
the universe is closed and finite, then a. | the universe has a center and an
edge. | b. | the universe will expand forever. | c. | the final fate
of the universe will be very cold and of extremely low density. | d. | the space-time
of the universe is negatively curved | e. | none of the above | | |
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48.
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_________ cause a sudden brightening of distant stars by gravitationally lensing the
light from those stars. This processes causes the distant stars to grow brighter over a period of a
few tens of days. a. | WIMPs | b. | neutrinos | c. | globular
clusters | d. | MACHOs | e. | none of the
above | | |
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49.
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Measured ages of globular clusters and a study of the time required for massive stars
to build up the present abundance of heavy elements suggests that the universe is a. | no more than 20
billion years old. | b. | no more than 10 billion years old | c. | at least 14
billion years old | d. | flat | e. | closed | | |
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50.
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If
the universe is flat a. | its age will be equal to 1/H. | b. | its age will be
equal two-thirds of 1/H. | c. | the density of the universe is less than the critical
density. | d. | the density of the universe is greater than the critical
density. | e. | dark matter accounts for a small fraction of the density of the
universe. | | |
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51.
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The
flatness problem and horizon problem a. | are solved if there was a sudden inflation of the universe at
time before recombination occurred. | b. | show that the universe cannot be described by the steady state
theory. | c. | show that dark matter must be a small fraction of the total
mass of the universe. | d. | imply that the universe was once much hotter than it is
now. | e. | imply that the
inflationary theory is incorrect. | | |
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52.
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Galaxy seeds around which galaxies, clusters and walls grew may have
been a. | caused by hot
dark matter. | b. | caused by baryons. | c. | the result of
the separation of the electromagnetic and weak forces. | d. | the result of
freezing water molecules shortly after the universe became transparent to
photons. | e. | caused by defects in space-time. | | |
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53.
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If a
two dimensional universe has a negative curvature a. | the area of a circle will be greater than ðr2. | b. | the area of a circle will be equal to ðr2. | c. | the universe is infinite. | d. | the universe is
finite but bounded | e. | the universe will have a center | | |
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54.
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Whether the universe is open, closed or flat depends on the ________ of the
universe. a. | luminosity | b. | density | c. | temperature | d. | radius | e. | rotation
rate | | |
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55.
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The
age of the universe can be determined if a. | the universe is flat. | b. | the amount of
dark matter in the universe can be accurately determined. | c. | the rate of
recession of the galaxies in the Local Group can be accurately determined. | d. | the temperature
of the cosmic background radiation can be accurately determined. | e. | the Hubble
constant and density of the universe can be accurately determined. | | |
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56.
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If a
galaxy is located at a distance of 18 Mpc and it is found to have recessional velocity of 1170
km/sec, what is Hubble's constant based only on this galaxy? a. | 65
km/sec | b. | 75 km/sec | c. | 55
km/sec | d. | 85 km/sec | e. | 95
km/sec | | |
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57.
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The
oldest rocks found on Earth are about _________ years old. a. | 10
billion | b. | 5.3 billion | c. | 4.6
billion | d. | 3.9 billion | e. | 6.2
million | | |
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58.
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Which
of the following is not a characteristic of the terrestrial planets? a. | low average
density | b. | orbits inside the asteroids | c. | craters in old
surfaces | d. | small diameters | e. | very few
satellites | | |
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59.
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A
future news release might report that a new planet has been found around a star very similar to our
sun. This newly discovered planet is claimed to have a mass 40 times that of Earth and is located
nearly 25 AU from the star it orbits. Which of the following would be a reasonable prediction about
this planet?
I. | The planet will probably have a mean density of around 5
g/cm3. | II. | The planet will probably have a radius of around five to ten
times greater than Earth's. | III. | The planet will probably have several
satellites. | IV. | The planet will probably have a composition that is mostly
hydrogen and helium. | | |
a. | I &
IV | b. | I, II, &
III | c. | II, III, &
IV | d. | I, II, &
IV | e. | I, II, III,
& IV | | |
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60.
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A(n)
_________ is a solar system object that enters Earth's atmosphere and becomes very hot due to
friction between the object and Earth's atmosphere. < |