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.