Name __________________________
INSTRUCTIONS: Fill in your
Student ID# and the FORM NUMBER of your
exam on the answer sheet.
Choose the BEST answer for each question and
mark your choice on the answer
sheet. Use a #2 pencil only.
1. The atmosphere that we
are now breathing is
*a. the third atmosphere
that the Earth has had.
b. the second atmosphere
that the Earth has had.
c. the first atmosphere
that the Earth has had.
d. the seventh atmosphere
that the Earth has had.
2. How is interferometry used
in radio astronomy?
a. Signals from different
places around the dish of a radio
telescope
are combined to produce interference and increase the
angular
resolution of the telescope.
b. Signals from a radio
source are combined with a time delay that
causes
interference and increases the angular resolution of the
telescope.
*c. Signals from two different
radio telescopes are combined to
produce
a single image of greater angular resolution than from
either
telescope alone.
d. Signals from different
parts of a radio source are combined to
increase
the angular resolution of the telescope.
3. What future awaits Triton,
the largest satellite of Neptune?
*a. Tidal break-up as it
spirals closer to Neptune
b. Escape from Neptune
after billions of years, as Triton gradually
spirals
outward
c. Gravitational capture
by Pluto
d. Probable destruction
from impact by Pluto
4. Most surface rocks on the
Earth are younger than a few million years
old, whereas
ages of lunar rocks have been measured in billions of
years. Why is
this?
a. The ages of Earth
and Moon are fundamentally different, the Moon
being
an old object captured from space by a younger Earth.
b. Most early surface
rocks on Earth have been washed into the sea
by weathering
and rainwater, and this does not happen on the
Moon.
*c. Much of the Earth's surface
is continually recycled (created and
subducted)
by the underlying mantle because of plate tectonic
activity,
and this does not occur on the Moon.
d. The complete surface
of the Earth has been covered periodically
by younger
material from intense volcanic eruptions in the last
few million
years. No such activity occurred on the Moon.
5. To what does "planetary
differentiation" refer?
*a. The sinking of heavier
elements towards the center of a planet
and the
rising of lighter elements towards the surface.
b. The formation of
rocky planets in the hotter, inner solar system
and gas
giants in the colder, outer regions.
c. The large-scale
convection of rock in the mantle of a planet,
which
on the Earth causes continental drift.
d. The circulation
of iron in the core of a planet, resulting in the
generation
of a magnetic field.
6. What is the overall composition
of Jupiter, excluding its rocky
core?
*a. 86% hydrogen, 13% helium,
1% everything else.
b. 75% hydrogen, 15%
helium, 10% everything else.
c. Pure hydrogen.
d. Hydrogen and helium
only, nothing else.
7. It is difficult to improve
the angular resolution of optical
telescopes on
the surface of the Earth because
a. large telescopes
are always reflecting telescopes and these
suffer
from too much chromatic aberration.
b. we would need to
build large telescopes and this is very
expensive.
c. spherical mirrors
suffer from too much aberration.
*d. air turbulence distorts
the star images more than the telescopes
do.
8. Scientists have now examined
rocks that came from Mars in their
laboratories
on Earth because
a. a large impact that
occurred on the Martian surface early in its
history
created a vast dust cloud through which Earth passes once
per year
and samples of this dust have now been collected by the
Space
Shuttle.
b. an orbiting spacecraft
scooped up Martian dust during its passage
by Mars
and then returned to Earth.
*c. several meteorites found
in Antarctica are now thought to have
been knocked
off Mars and fallen to Earth.
d. spacecraft have
been to the surface of Mars and have returned
with samples
of Martian rocks and soil.
9. How is the Earth's magnetic
field generated?
*a. By electric currents
in the Earth's core.
b. By electric currents
in the Earth's mantle.
c. By electrons and
ions in the Earth's magnetosphere.
d. By permanent magnetism
in the Earth's crustal rocks.
10. Why was adaptive optics
developed?
a. To compensate for
spherical aberration.
*b. To compensate for distortion
caused by the Earth's atmosphere.
c. To prevent distortion
by sagging in very thin, light-weight
mirrors.
d. To prevent distortion
of mirrors by the vacuum of space.
11. The pressures of the atmospheres
at the surfaces of Mercury, Venus,
and Mars,
in terms of the pressure at the surface of the Earth,
(known
as 1 atmosphere) are
a. 0.01 atmosphere;
almost 100 atmospheres; 1/10 atmosphere.
b. 0; about 10 atmospheres;
0.1 atmosphere.
*c. 0; almost 100 atmospheres;
0.01 atmosphere.
d. 0.1 atmosphere;
almost 100 atmospheres; 1/10 atmosphere.
12. Which of the following
characteristics of an astronomical telescope
is the
most important for determining the angular resolution?
*a. The diameter of the objective
lens or mirror.
b. The focal length
of the objective lens or mirror.
c. The magnifying power
of the telescope.
d. The focal length
of the eyepiece.
13. In a single photograph
of a comet and its tail, the only direction
that one
can determine with certainty is
a. the direction in
which the comet is moving, from the trailing
tail.
b. the direction towards
Jupiter, since the gravity of this giant
planet
pulls the tail material towards it.
*c. the direction away from
the Sun, since the tail is pushed in this
direction
by the solar wind.
d. the direction towards
the Sun indicated by the tail direction,
since
gas and dust in the tail is attracted towards the Sun by
its gravity.
14. In telescopes, the angular
resolution is worse for
a. larger diameter
lenses or mirrors and longer wavelength light (of
other
electromagnetic radiation).
*b. smaller diameter lenses
or mirrors and longer wavelength light
(or other
electromagnetic radiation).
c. smaller diameter
lenses or mirrors and shorter wavelength light
(of other
electromagnetic radiation).
d. larger diameter
lenses or mirrors and shorter wavelength light
(or other
electromagnetic radiation).
15. The main reason for the
very high temperature (750 K) on the surface
of Venus
is thought to be
a. chemical reactions
between constituents of the atmosphere,
particularly
sulfuric acid.
b. the radiation from
hot lava, produced by intense and continuous
volcanic
action.
c. the continuous bombardment
of the surface by solar wind particles
and meteoroids.
*d. the absorption of visible
radiation by Venus's surface and the
subsequent
trapping by the atmosphere and clouds of infrared
radiation
emitted by the surface.
16. Chromatic aberration is
the failure of a telescope objective to
bring
all colors of light to the same focus, and appears
a. in all telescopes,
since it is a basic property of light.
b. only in a reflecting
telescope.
c. in both reflecting
and refracting telescopes.
*d. only in a refracting
telescope.
17. How did Comet Shoemaker-Levy
9 achieve lasting fame?
*a. It crashed into Jupiter.
b. It just missed the
Earth, passing closer than the Moon.
c. It exploded after
passing too close to the Sun.
d. It became the first
comet to be visited by spacecraft.
18. What is the mass of Jupiter
compared to other objects in the solar
system?
*a. Twice the mass of all
other planets combined.
b. Twenty times the
mass of all other planets combined.
c. As large as the
mass of Saturn and Neptune combined.
d. Half the mass of
the Sun.
19. Cassini's division in
the rings of Saturn are thought to be due to
tidal
gravitational forces from the moon, Mimas. If the revolution
period
of Mimas is 22.6 hours, what would be the orbital period of
any particles
that exist within Cassini's division?
*a. 11.3 hours, or 1/2 of
Mimas' period.
b. 45.2 hours, or 2
x Mimas' period.
c. 7.5 hours, or 1/3
of Mimas' period.
d. 22.6 hours, since
Mimas moves within Cassini's division.
20. Which of the following
statements is NOT true for asteroids?
a. Some asteroids have
orbits that carry them inside the Earth's
orbit.
*b. Only a minority of all
asteroids are in the asteroid belt.
c. Some asteroids occupy
the same orbit as Jupiter.
d. The total mass of
all asteroids is much smaller than the mass of
the Earth.
21. The surface features and
overall topology of Venus have been
determined
primarily by
*a. radar methods from Venus-orbiting
spacecraft, measuring radio
echoes
from the surface.
b. balloon-borne spacecraft,
launched into Venus's atmosphere by
spacecraft.
c. surface landing
vehicles that have explored the surface
thoroughly.
d. visible and UV photography
from the Space Shuttle.
22. What method do geologists
and geophysicists use to probe the
structure
of the Earth's core and mantle?
*a. Studying the deflection
of seismic waves from earthquakes.
b. Direct sampling
of interior rock by deep drilling through the
ocean
floor.
c. X-ray analysis from
satellites.
d. Extrapolation of
surface features (e.g., mountain chains) into
the deep
interior.
23. One of the most important
sources of heat in the interiors of moons
that orbit
close to giant planets is
*a. continuous tidal distortion
from the planet and other moons.
b. re-radiation of
thermal energy received from the planet.
c. decay of radioactive
elements within the moons.
d. reflection of sunlight
from the planet's surface.
24. The Earth's stratosphere
is warmer than the layers above and below
it because
*a. ozone in the stratosphere
absorbs ultraviolet radiation from the
Sun.
b. CO_2 in the stratosphere
absorbs infrared light radiated outward
by the
ground.
c. the methane released
when we burn fossil fuel collects in this
layer
and absorbs infrared light.
d. warm air heated
by contact with the ground rises into the
stratosphere
and heats it.
25. The metal that is relatively
abundant in meteorites but that is
generally
rare upon Earth has been found in specific layers of clay
throughout
the world, and its study is helping to evaluate the
effect
of meteor impacts upon the Earth's climate and its
inhabitants
in recent geological time (e.g., dinosaurs). This metal
is
a. cobalt.
b. iron.
c. nickel.
*d. iridium.
26. An Earth-based telescopic
view of Venus shows
a. evidence of ice-covered
polar caps and huge dust storms.
b. a crater-covered
surface of reddish color.
c. a smooth, dark surface
with few mountain ranges.
*d. a completely cloud-shrouded
planet with high atmospheric wind
speeds.
27. Many amateur astronomers
have telescopes with mirrors 20 cm (1/5 m)
in diameter.
In comparison, the largest astronomical telescope in
the world
is the Keck telescope, with a diameter of 10 m. How many
times
larger is the light-gathering power of the Keck telescope
than a
20-cm telescope?
a. 125,000 times larger
b. 7 times larger
c. 50 times larger
*d. 2,500 times larger
28. If astronauts were to
set up a permanent settlement at Tranquility
Base on
the Moon, how many times each year would the Earth rise and
set as
seen by a resident of this base?
*a. Never - the Earth would
remain essentially motionless in the sky.
b. Once each year.
c. 12 times each year.
d. 13 times each year.
29. Which is the only satellite
in the solar system known to possess a
permanent,
dense, atmosphere?
*a. Titan
b. Ganymede
c. Callisto
d. Charon
30. What are the characteristic
features on the visible surface of
Jupiter?
*a. Light and dark bands
of clouds parallel to the equator.
b. Large volcanoes
and a long, deep rift valley.
c. A greenish, almost
featureless cloud layer.
d. A bluish tint with
high, white clouds and dark storms.
31. Billions of years ago,
the Earth's atmosphere was composed primarily
of carbon
dioxide. Where might you go to find a large fraction of
this carbon
dioxide today?
*a. To the Rocky Mountains,
which are composed largely of limestone.
b. Anywhere, most of
the carbon dioxide is still in the atmosphere,
but nitrogen
and oxygen have since been added to it.
c. Nowhere, most of
the carbon dioxide escaped into space.
d. To extinct volcanoes
like Mt. Edziza, British Columbia, which are
composed
of rock from the Earth's interior.
32. When electromagnetic radiation
(e.g., light) is Doppler-shifted by
motion
of the source away from the detector,
*a. the measured wavelength
is longer than the emitted wavelength.
b. the measured frequency
is higher than the emitted frequency.
c. the speed of the
radiation is less than the emitted speed.
d. the measured frequency
of the radiation remains the same, but its
wavelength
is shortened, compared to the emitted radiation.
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