Astronomy 1020 - Practice Questions
Dr. Gudehus
- 1)
- 
  An Ångstrom unit is  
- (a)
- 
 larger than a micron.
- 
(b)
- 
 the same as an electron volt.
- 
(c)
- 
 smaller than a micron.
- 
(d)
- 
 bigger than a millimeter.
- 2)
- 
  The sequence of colors in a spectrum is in the order of 
- (a)
- 
 red, violet, yellow.
- 
(b)
- 
 green, blue, orange.
- 
(c)
- 
 violet, red, orange.
- 
(d)
- 
 red, orange, yellow.
- 3)
- 
  The electromagnetic force is 
- (a)
- 
 stronger than the nuclear force.
- 
(b)
- 
 weaker than gravity.
- 
(c)
- 
 stronger than the weak force.
- 
(d)
- 
 agrees with all of the above statements.
- 4)
- 
 When light passes through a small opening, it undergoes
- (a)
- 
 refraction.
- 
(b)
- 
 interference.
- 
(c)
- 
 dispersion.
- 
(d)
- 
 diffraction.
- 5)
- 
  In order to produce a bright line spectrum, we need to start with
- (a)
- 
 a hot gas.
- 
(b)
- 
 a hot solid.
- 
(c)
- 
 a blackbody.
- 
(d)
- 
 a cool gas.
- 6)
- 
  In hydrogen, the series visible to human eyes is the
- (a)
- 
 Balmer series.
- 
(b)
- 
 Paschen series.
- 
(c)
- 
 Lyman series.
- 
(d)
- 
 World series.
- 7)
- 
  In order to broaden a spectral line, we should  
- (a)
- 
 make the gas hotter and decrease the pressure.
- 
(b)
- 
 make the gas hotter and increase the pressure.
- 
(c)
- 
 make the gas cooler and decrease the pressure.
- 
(d)
- 
 make the gas cooler and increase the pressure.
- 8)
- 
  If a star is approaching us, its lines are 
- (a)
- 
 shifted blueward.
- 
(b)
- 
 shifted redward.
- 
(c)
- 
 not shifted.
- 
(d)
- 
 doubled.
- 9)
- 
  If the temperature of a blackbody is doubled, its radiated power
- (a)
- 
 is increased twofold.
- 
(b)
- 
 is increased fourfold.
- 
(c)
- 
 is increased eightfold.
- 
(d)
- 
 is increased sixteenfold.
- 10)
- 
  If the temperature of a blackbody is doubled, the wavelength of
its peak output
- (a)
- 
 is doubled.
- 
(b)
- 
 is halved.
- 
(c)
- 
 is unaffected.
- 
(d)
- 
 is quadrupled.
- 11)
- 
  The sun generates its energy in its
- (a)
- 
 photosphere.
- 
(b)
- 
 corona.
- 
(c)
- 
 core.
- 
(d)
- 
 chromosphere.
- 12)
- 
 The period of the sunspot cycle is 
- (a)
- 
 29 days.
- 
(b)
- 
 11 years.
- 
(c)
- 
 1 year.
- 
(d)
- 
 24 hours.
- 13)
- 
  The corona is hotter than
- (a)
- 
 the photosphere.
- 
(b)
- 
 the chromosphere.
- 
(c)
- 
 sunspots.
- 
(d)
- 
 all of the above.
- 14)
- 
  Prominences are
- (a)
- 
 also known as aurorae.
- 
(b)
- 
 found above the chromosphere.
- 
(c)
- 
 found below the photosphere.
- 
(d)
- 
 another name for sunspots.
- 15)
- 
 An historic period of few sunspots and cool weather is known as 
- (a)
- 
 the dark ages.
- 
(b)
- 
 the crash of '29.
- 
(c)
- 
 the epicycle.
- 
(d)
- 
 the Maunder minimum.
- 16)
- 
  The solar wind is a stream of _________ 
that passes by the planets.
- (a)
- 
 hot hydrogen
- 
(b)
- 
 electrons and protons
- 
(c)
- 
 gas from the corona
- 
(d)
- 
 all of the above
- 17)
- 
  The sun's rotational rate is 
- (a)
- 
 faster at its equator.
- 
(b)
- 
 faster near its poles.
- 
(c)
- 
 equal to that of the earth.
- 
(d)
- 
 similar to that of a solid body.
- 18)
- 
 The spectral class of the sun is
- (a)
- 
 O.
- 
(b)
- 
 F.
- 
(c)
- 
 G.
- 
(d)
- 
 M.
- 19)
- 
 The star which is bluest is the star with a color index of
- (a)
- 
  0.4.
- 
(b)
- 
 -0.4.
- 
(c)
- 
  0.0.
- 
(d)
- 
 2.0.
- 20)
- 
  Distances to nearby stars can be measured by
- (a)
- 
 radar.
- 
(b)
- 
 sonar.
- 
(c)
- 
 trigonometric parallax.
- 
(d)
- 
 their rotation rate.
- 21)
- 
  A star with a small proper motion would
- (a)
- 
 have a small tangential velocity and be nearby.
- 
(b)
- 
 have a small tangential velocity and be far away.
- 
(c)
- 
 have a large tangential velocity and be nearby.
- 
(d)
- 
 have a large tangential velocity and be far away.
- 22)
- 
  The absolute magnitude of a star refers to its magnitude
at a distance of
- (a)
- 
 1 parsec.
- 
(b)
- 
 10 parsecs.
- 
(c)
- 
 100 parsecs.
- 
(d)
- 
 1000 parsecs.
- 23)
- 
  The distance modulus of a star is equal to
- (a)
- 
 m-M.
- 
(b)
- 
 M-m.
- 
(c)
- 
 m-M+5.
- 
(d)
- 
 M-m+5.
- 24)
- 
  Which spectral class is hotter than the sun?
- (a)
- 
 G.
- 
(b)
- 
 M.
- 
(c)
- 
 K.
- 
(d)
- 
 B.
- 25)
- 
  A star of high luminosity has a
- (a)
- 
 low temperature and small radius.
- 
(b)
- 
 high temperature and small radius.
- 
(c)
- 
 low temperature and large radius.
- 
(d)
- 
 high temperature and large radius.
- 26)
- 
  The coolest spectral class is
- (a)
- 
 A.
- 
(b)
- 
 B.
- 
(c)
- 
 F.
- 
(d)
- 
 K.
- 27)
- 
  The Hertzsprung-Russell diagram is a plot of
- (a)
- 
 temperature against spectral class.
- 
(b)
- 
 spectral class against radius.
- 
(c)
- 
 luminosity against spectral class.
- 
(d)
- 
 radius against luminosity.
- 28)
- 
  Which is the coolest star?
- (a)
- 
 a red giant.
- 
(b)
- 
 a blue supergiant.
- 
(c)
- 
 a white dwarf.
- 
(d)
- 
 the sun.
- 29)
- 
  Which does not belong?
- (a)
- 
 spectroscopic binary.
- 
(b)
- 
 visual binary.
- 
(c)
- 
 optical binary.
- 
(d)
- 
 eclipsing binary.
- 30)
- 
  An astrometric binary is a binary
- (a)
- 
 whose orbit lies in the plane of the sky.
- 
(b)
- 
 whose orbit is a parabola.
- 
(c)
- 
 whose distance is greater than 10 parsecs.
- 
(d)
- 
 in which one of the members is not visible.
- 31)
- 
  In order to derive the masses of the stars in a binary, we
need to employ
- (a)
- 
 the blackbody formula.
- 
(b)
- 
 Newton's law of gravity.
- 
(c)
- 
 the conservation of angular momentum.
- 
(d)
- 
 the H-R diagram.
- 32)
- 
  A binary system is more likely to be a spectroscopic binary if
- (a)
- 
 the stars are close together.
- 
(b)
- 
 the masses are large.
- 
(c)
- 
 the orbit is perpendicular to the plane of the sky.
- 
(d)
- 
 all of the above.
- 33)
- 
  The masses we derive from spectroscopic binaries are
- (a)
- 
 true masses.
- 
(b)
- 
 underestimates.
- 
(c)
- 
 overestimates.
- 
(d)
- 
 true masses if spectra of both stars are visible.
- 34)
- 
  A binary system is more likely to be an eclipsing binary if
- (a)
- 
 the stars are large compared to their separation.
- 
(b)
- 
 the separation is small compared to the stars' radii.
- 
(c)
- 
 the plane of the orbit is perpendicular to that of the sky.
- 
(d)
- 
 all of the above.
- 35)
- 
  The star Algol or b Persei is a famous  example of
- (a)
- 
 a visual binary.
- 
(b)
- 
 a spectroscopic binary.
- 
(c)
- 
 an eclipsing binary.
- 
(d)
- 
 an astrometric binary.
- 36)
- 
  The stars which deviate from the mass-luminosity
relation are
- (a)
- 
 red giants only.
- 
(b)
- 
 main sequence stars.
- 
(c)
- 
 red giants and white dwarfs.
- 
(d)
- 
 all of the above.
- 37)
- 
  Bok globules are 
- (a)
- 
 ionized hydrogen regions.
- 
(b)
- 
 large dark nebulae.
- 
(c)
- 
 remnants of old stars.
- 
(d)
- 
 small dark nebulae.
- 38)
- 
  Interstellar dust makes starlight
- (a)
- 
 dimmer and bluer.
- 
(b)
- 
 dimmer and redder.
- 
(c)
- 
 only bluer.
- 
(d)
- 
 only redder.
- 39)
- 
  Interstellar absorption lines are 
- (a)
- 
 broad and highly redshifted.
- 
(b)
- 
 narrow and highly redshifted.
- 
(c)
- 
 broad and of various redshifts and blueshifts.
- 
(d)
- 
 narrow and of various redshifts and blueshifts.
- 40)
- 
  What radiates at a wavelength of 21 cm?
- (a)
- 
 ionized hydrogen.
- 
(b)
- 
 neutral hydrogen.
- 
(c)
- 
 molecular hydrogen.
- 
(d)
- 
 all of the above.
- 41)
- 
  The most massive stars are about
- (a)
- 
 10 MSun.
- 
(b)
- 
 100 MSun.
- 
(c)
- 
 1000 MSun.
- 
(d)
- 
 10000 MSun.
- 42)
- 
 Helium undergoes fusion into  carbon
- (a)
- 
 while a star is on the main sequence
- 
(b)
- 
 while a star is contracting from a molecular cloud.
- 
(c)
- 
 while a star is a red giant.
- 
(d)
- 
 while a star is a white dwarf.
- 43)
- 
  When a star exhuasts its supply of hydrogen in its core,
- (a)
- 
 the core contracts and the envelope expands.
- 
(b)
- 
 the core expands and the envelope expands.
- 
(c)
- 
 the core contracts and the envelope contracts.
- 
(d)
- 
 the core expands and the envelope contracts.
- 44)
- 
  A helium flash occurs because 
- (a)
- 
 the helium is initially at a low temperature.
- 
(b)
- 
 the helium is initially at a low density.
- 
(c)
- 
 the helium is initially degenerate.
- 
(d)
- 
 the helium is initially not in the core.
- 45)
- 
  When a star becomes a red giant, 
- (a)
- 
 its temperature increases and its radius increases.
- 
(b)
- 
 its temperature decreases and its radius increases.
- 
(c)
- 
 its temperature increases and its radius decreases.
- 
(d)
- 
 its temperature decreases and its radius decreases.
- 46)
- 
  For a Cepheid variable,
- (a)
- 
 a longer period means a lower luminosity.
- 
(b)
- 
 the periods are typically less than a day.
- 
(c)
- 
 the star lies on the main sequence.
- 
(d)
- 
 the longer the period, the more luminous the star.
- 47)
- 
  When we plot a star cluster in the H-R diagram,
- (a)
- 
 we can test stellar models against observations.
- 
(b)
- 
 we can estimate the age of a cluster.
- 
(c)
- 
 we can assume than the stars are of about the same age and
composition.
- 
(d)
- 
 all of the above.
- 48)
- 
  Low mass stars on the lower main sequence will
- (a)
- 
 eventually burn helium into carbon.
- 
(b)
- 
 eventually burn helium into hydrogen.
- 
(c)
- 
 eventually contract and become white dwarfs.
- 
(d)
- 
 eventually become red giants.
- 49)
- 
  A planetary nebula is
- (a)
- 
 a nebula from which a young star with planets will form.
- 
(b)
- 
 a shell of gas ejected from a red giant.
- 
(c)
- 
 an accretion disk around a white dwarf.
- 
(d)
- 
 a shell of gas which collects around a main sequence star.
- 50)
- 
  A teaspoon of material from a white dwarf would on the average
have as much mass as
- (a)
- 
 a lead brick.
- 
(b)
- 
 a person.
- 
(c)
- 
 a truck.
- 
(d)
- 
 the moon.
- 51)
- 
  If a star accumulates a core of iron,
- (a)
- 
 it continues producing energy in the form of iron fusion.
- 
(b)
- 
 it slowly contracts.
- 
(c)
- 
 it collapses and then explodes as a supernova.
- 
(d)
- 
 it becomes a nova.
- 52)
- 
  In order to have synchrotron radiation, one must have 
- (a)
- 
 moving neutral particles and a magnetic field.
- 
(b)
- 
 moving charged particles and no magnetic field.
- 
(c)
- 
 moving neutral particles and no magnetic field.
- 
(d)
- 
 moving charged particles and a magnetic field.
- 53)
- 
 When mass is transferred from one star of a binary star system
to the other, the mass 
- (a)
- 
 accumulates in an accretion disk.
- 
(b)
- 
 passes through the Langrangian point.
- 
(c)
- 
 heats up.
- 
(d)
- 
 all of the above.
- 54)
- 
  When a star becomes a nova,
- (a)
- 
 it is usually a young star.
- 
(b)
- 
 it is usually a main sequence star.
- 
(c)
- 
 it is usually a red giant.
- 
(d)
- 
 it is usually a white dwarf.
- 55)
- 
  Neutron stars
- (a)
- 
 are slightly smaller than the sun.
- 
(b)
- 
 are slightly smaller than a white dwarf.
- 
(c)
- 
 are slightly smaller than a red giant.
- 
(d)
- 
 none of the above are true.
- 56)
- 
  Pulsars can be explained by the
- (a)
- 
 vibrations of a white dwarf.
- 
(b)
- 
 vibrations of a neutron star.
- 
(c)
- 
 lighthouse theory.
- 
(d)
- 
 Herbig-Haro theory.
- 57)
- 
  The more massive a white dwarf is,
- (a)
- 
 the slower it vibrates.
- 
(b)
- 
 the smaller its radius is.
- 
(c)
- 
 the hotter it is.
- 
(d)
- 
 all of the above.
- 58)
- 
  Pulsars slow down with time because
- (a)
- 
 they are running out of nuclear fuel.
- 
(b)
- 
 they are becomming less dense.
- 
(c)
- 
 they are converting rotational energy into radiation.
- 
(d)
- 
 they are evaporating.
- 59)
- 
  The most likely stage before a neutron star is
- (a)
- 
 the nova stage.
- 
(b)
- 
 the T Tauri stage.
- 
(c)
- 
 the main sequence stage.
- 
(d)
- 
 the supernova stage.
- 60)
- 
  A pulsar glitch is a 
- (a)
- 
 burst of X-rays.
- 
(b)
- 
 burst of radio waves.
- 
(c)
- 
 sudden change in the pulsar's period.
- 
(d)
- 
 sudden change in the pulsar's position.
- 61)
- 
  Light can escape from the vicinity of a black hole if
- (a)
- 
 it starts from inside the event horizon.
- 
(b)
- 
 it starts from outside the event horizon.
- 
(c)
- 
 it starts from inside the event horizon and is directed
straight away from the black hole.
- 
(d)
- 
 it starts from inside the light circle and is directed 
straight at the black hole.
- 62)
- 
  The expression "black holes have no hair" means
- (a)
- 
 black holes have not been verified.
- 
(b)
- 
 black holes are old.
- 
(c)
- 
 black holes are easy to explain.
- 
(d)
- 
 black holes are described by their mass, angular momentum,
and charge.
- 63)
- 
  Special relativity tells us that a moving clock
- (a)
- 
 passes time more slowly as seen by a stationary observer.
- 
(b)
- 
 passes time more rapidly as seen by a stationary observer.
- 
(c)
- 
 passes time more slowly as seen by an observer traveling with 
the clock.
- 
(d)
- 
 passes time at the same rate as seen by a stationary observer.
- 64)
- 
  General relativity
- (a)
- 
 correctly explains the advance of Mercury's perihelion.
- 
(b)
- 
 correctly explains the deflection of starlight by the sun.
- 
(c)
- 
 correctly explains the reddening of light in a gravitational 
field.
- 
(d)
- 
 correctly explains all of the above.
- 65)
- 
 The Milky Way galaxy is  
- (a)
- 
 a spiral galaxy.
- 
(b)
- 
 an elliptical galaxy.
- 
(c)
- 
 an irregular galaxy.
- 
(d)
- 
 a peculiar galaxy.
- 66)
- 
  The Magellanic Clouds can best be seen from 
- (a)
- 
 Alaska.
- 
(b)
- 
 Secaucus, New Jersey.
- 
(c)
- 
 South America.
- 
(d)
- 
 Ponca City, Oklahoma.
- 67)
- 
  The method called "star gauging" was conceived by
- (a)
- 
 Galileo.
- 
(b)
- 
 Herschel.
- 
(c)
- 
 Hubble.
- 
(d)
- 
 Ptolemy.
- 68)
- 
  In order to determine the sun's location in the Galaxy, 
Shapley used
- (a)
- 
 the brightnesses of novae.
- 
(b)
- 
 the parallaxes of dwarf stars.
- 
(c)
- 
 the diameters of ellipticals.
- 
(d)
- 
 the brightnesses of RR Lyrae stars and globular cluster
diameters.
- 69)
- 
  The Galaxy's dust and gas is found in its
- (a)
- 
 central bulge.
- 
(b)
- 
 halo.
- 
(c)
- 
 disk.
- 
(d)
- 
 nucleus.
- 70)
- 
  The distance of the sun from the center of the Galaxy is
- (a)
- 
 10 parsecs.
- 
(b)
- 
 8.5 kiloparsecs.
- 
(c)
- 
 1 AU.
- 
(d)
- 
 8.5 megaparsecs.
- 71)
- 
  Cosmic rays become trapped in the disk because of the Galaxy's
- (a)
- 
 intense gravity.
- 
(b)
- 
 absorbing dust layer.
- 
(c)
- 
 magnetic field.
- 
(d)
- 
 large number of stars.
- 72)
- 
  The oldest stars in the Galaxy are found in the
- (a)
- 
 disk.
- 
(b)
- 
 halo.
- 
(c)
- 
 spiral arms.
- 
(d)
- 
 molecular clouds.
- 73)
- 
  The sun is
- (a)
- 
 a population I star.
- 
(b)
- 
 a population II star.
- 
(c)
- 
 a Cepheid.
- 
(d)
- 
 an RR Lyrae.
- 74)
- 
  Which would not be a good wavelength region to observe the
center of the Galaxy in?
- (a)
- 
 Radio.
- 
(b)
- 
 Optical.
- 
(c)
- 
 Infrared.
- 
(d)
- 
 Gamma ray.
- 75)
- 
  Cepheids are useful for measuring distances to galaxies because
their
- (a)
- 
 light output is constant.
- 
(b)
- 
 high luminosity is correlated with their period.
- 
(c)
- 
 absolute magnitudes are always greater than that of the sun.
- 
(d)
- 
 diameters are easily measured.
- 76)
- 
  Which is not a way to measure the mass of a galaxy?
- (a)
- 
 Measurement of its rotation curve.
- 
(b)
- 
 Double galaxy method.
- 
(c)
- 
 Velocity dispersion method.
- 
(d)
- 
 Measurement of its lookback time.
- 77)
- 
  Most galaxies are
- (a)
- 
 ellipticals.
- 
(b)
- 
 spirals.
- 
(c)
- 
 irregulars.
- 
(d)
- 
 peculiar.
- 78)
- 
  The tuning fork diagram of galaxy types was conceived of by
- (a)
- 
 Harlow Shapley.
- 
(b)
- 
 Henrietta Leavitt.
- 
(c)
- 
 Edwin Hubble.
- 
(d)
- 
 Johannes Kepler.
- 79)
- 
  S0 galaxies fit between
- (a)
- 
 ellipticals and irregulars.
- 
(b)
- 
 spirals and irregulars.
- 
(c)
- 
 ellipticals and spirals.
- 
(d)
- 
 Sb galaxies and Sc galaxies.
- 80)
- 
  Galactic cannibalism refers to
- (a)
- 
 the merging of galaxies.
- 
(b)
- 
 black holes at the centers of galaxies.
- 
(c)
- 
 rapidly rotating galaxies.
- 
(d)
- 
 galaxies which have dark matter.
- 81)
- 
  The arms of spiral galaxies appear prominent because
- (a)
- 
 they contain stars like the sun.
- 
(b)
- 
 they contain O and B stars.
- 
(c)
- 
 they contain dust.
- 
(d)
- 
 they contain gas.
- 82)
- 
  Starburst galaxies are triggered by
- (a)
- 
 aging.
- 
(b)
- 
 cosmic rays.
- 
(c)
- 
 collisions of galaxies.
- 
(d)
- 
 dwarf stars.
- 83)
- 
  The Milky Way galaxy is a member of 
- (a)
- 
 the Virgo cluster.
- 
(b)
- 
 the Coma cluster.
- 
(c)
- 
 the Local Group.
- 
(d)
- 
 the Andromeda nebula.
- 84)
- 
  The 3C catalogue is a list of
- (a)
- 
 X-ray sources.
- 
(b)
- 
gamma-ray sources.
- 
(c)
- 
 infrared sources.
- 
(d)
- 
 radio sources.
- 85)
- 
  Synchrotron radiation is produced by
- (a)
- 
 charged particles moving in a gravitational field.
- 
(b)
- 
 charged particles moving in a magnetic field.
- 
(c)
- 
 radioactive atoms.
- 
(d)
- 
 neutral atoms moving in an electric field.
- 86)
- 
  Some radio galaxies have huge double lobes.  These
lobes are probably
- (a)
- 
 star clusters.
- 
(b)
- 
 clouds of high speed charged particles.
- 
(c)
- 
 clouds of dust.
- 
(d)
- 
 dark matter.
- 87)
- 
  Head-tail radio galaxies are galaxies that are
- (a)
- 
 motionless.
- 
(b)
- 
 moving throught the intergalactic medium.
- 
(c)
- 
 radio-silent.
- 
(d)
- 
 featureless.
- 88)
- 
  The centers of active galaxies probably contain
- (a)
- 
 massive neutron stars.
- 
(b)
- 
 massive white dwarfs.
- 
(c)
- 
 massive black holes.
- 
(d)
- 
 massive planets.
- 89)
- 
  Seyfert galaxies
- (a)
- 
 are objects with a fairly constant light output.
- 
(b)
- 
 have cores which are no different than ordinary
galaxies.
- 
(c)
- 
 have emission lines from high velocity ionized gas.
- 
(d)
- 
 are never spirals.
- 90)
- 
  The galaxy M87
- (a)
- 
 is a spiral galaxy.
- 
(b)
- 
 has a broad light distribution in its center.
- 
(c)
- 
 shows no sign of being unusual.
- 
(d)
- 
 has a sharply peaked light distribution in its
center.
- 91)
- 
  The appearance of a quasar is 
- (a)
- 
 like that of an irregular galaxy.
- 
(b)
- 
 like that of a star.
- 
(c)
- 
 like that of a spiral galaxy.
- 
(d)
- 
 like that of a nebula.
- 92)
- 
  Quasars generally have 
- (a)
- 
 low redshifts.
- 
(b)
- 
 high redshifts.
- 
(c)
- 
 low luminosity.
- 
(d)
- 
 constant light output.
- 93)
- 
  The redshift of an object is a measure of
- (a)
- 
 the shift in wavelength of its spectral features.
- 
(b)
- 
 its shift in position on the sky.
- 
(c)
- 
 the change in intensity of its red light.
- 
(d)
- 
 its red light.
- 94)
- 
  Which does not belong?
- (a)
- 
 Seyfert galaxy.
- 
(b)
- 
 Andromeda galaxy.
- 
(c)
- 
 Quasar.
- 
(d)
- 
 BL Lacertid.
- 95)
- 
  A gravitational lens would describe
- (a)
- 
 a distant object imaged by a nearby low mass object.
- 
(b)
- 
 a nearby object imaged by a distant low mass object.
- 
(c)
- 
 a distant object imaged by a nearby massive object.
- 
(d)
- 
 a nearby object imaged by a distant massive object.
- 96)
- 
  Superluminal expansion is explained by 
- (a)
- 
 objects traveling faster than the speed of light.
- 
(b)
- 
 objects traveling almost directly toward us at high
velocity.
- 
(c)
- 
 objects traveling almost directly toward us at low
velocity. 
- 
(d)
- 
 objects traveling at right angles to our line of
sight.
- 97)
- 
  The sky is dark at night because
- (a)
- 
 of dark matter.
- 
(b)
- 
 of absorbing dust.
- 
(c)
- 
 of the expanding universe and the finite ages of
stars. 
- 
(d)
- 
 the universe is infinite.
- 98)
- 
  The cosmological principle states that the universe is
- (a)
- 
 inhomogeneous and isotropic.
- 
(b)
- 
 homogeneous and isotropic.
- 
(c)
- 
 the same at all times.
- 
(d)
- 
 always changing.
- 99)
- 
  The expansion of the universe refers to
- (a)
- 
 the random movement of galaxies in space. 
- 
(b)
- 
 the expansion of space, carrying the galaxies along
with it. 
- 
(c)
- 
 the exploding centers of galaxies.
- 
(d)
- 
 the gravitational repulsion of galaxies.
- 100)
- 
  If the universe is closed, it 
- (a)
- 
 is finite.
- 
(b)
- 
 has no edge.
- 
(c)
- 
 has a positive curvature.
- 
(d)
- 
 All of the above are true.
- 101)
- 
  The big bang refers to
- (a)
- 
 the end of the universe.
- 
(b)
- 
 the explosive beginning of the universe.
- 
(c)
- 
 the noise made by exploding black holes.
- 
(d)
- 
 a collision of superclusters.
- 102)
- 
  If the universe has the critical density,
- (a)
- 
 galaxies will expand to infinity while coasting to a halt.
- 
(b)
- 
 its curvature is flat or Euclidean.
- 
(c)
- 
 it would contain about 90% dark matter.
- 
(d)
- 
 All the above are true.
- 103)
- 
  The Hubble constant refers to
- (a)
- 
 a nonexpanding universe.
- 
(b)
- 
 the ratio of velocity to distance for the expanding
universe. 
- 
(c)
- 
 the curvature of the universe.
- 
(d)
- 
 a number in the steady state theory.
- 104)
- 
  The inflationary universe refers to
- (a)
- 
 the present economic situation.
- 
(b)
- 
 a theory of stellar winds.
- 
(c)
- 
 Olber's paradox.
- 
(d)
- 
 a dramatic expansion of the universe when it was
10-35 seconds old.
- 105)
- 
  Most of the helium in the universe was made 
- (a)
- 
 in the first few minutes of the universe.
- 
(b)
- 
 in the cores of red giants.
- 
(c)
- 
 at the time of recombination, when the universe was
about 106 years old.
- 
(d)
- 
 inside black holes.
- 106)
- 
  The most likely place for planets to form is
- (a)
- 
 around old red giants.
- 
(b)
- 
 inside "planetary nebulae".
- 
(c)
- 
 around young stars.
- 
(d)
- 
 in the vacuum of interstellar space.
- 107)
- 
  The Miller experiment was designed to  
- (a)
- 
 determine the age of blue-green algae.
- 
(b)
- 
 determine the mutation rate from cosmic rays.
- 
(c)
- 
 reproduce the conditions under which life began on Earth.
- 
(d)
- 
 create cells.
- 108)
- 
  The physical basis upon which life extracts energy from its
surroundings is based on   
- (a)
- 
 the chemistry of silicon.
- 
(b)
- 
 the chemistry of carbon.
- 
(c)
- 
 the chemistry of lead.
- 
(d)
- 
 the chemistry of hydrogen.
- 109)
- 
  The significance of the Murchison meteorite is that it  
- (a)
- 
 is a fossil.
- 
(b)
- 
 came from Mars.
- 
(c)
- 
 contains DNA.
- 
(d)
- 
 contains amino acids.
- 110)
- 
  Proteins consists of  
- (a)
- 
 Strands of DNA.
- 
(b)
- 
 Strands of RNA.
- 
(c)
- 
 Amino acids linked together.
- 
(d)
- 
 Alternating base pairs.
- 111)
- 
  Living organisms evolve toward  
- (a)
- 
 increasing complexity.
- 
(b)
- 
 decreasing complexity.
- 
(c)
- 
 shorter and shorter strands of DNA.
- 
(d)
- 
 Organisms do not evolve.
- 112)
- 
  In order to communicate with extraterrestrial societies,  
- (a)
- 
 we should send a spaceship to a likely star.
- 
(b)
- 
 we should send synchrotron emission to a likely star.
- 
(c)
- 
 use as long a wavelength as possible.
- 
(d)
- 
 use frequencies near the "water hole".
 
File translated from TEX by TTH, version 2.21.
On  2 Jan 2000, 19:42.
