General test-taking advice for this exam: Below,
you will find 27 fill in the blank, true/false and multiple choice questions
worth a total of 54 points (out of 100). These should take you 20-25
minutes. Questions 28-30 require written answers of at least several sentences.
While I don't expect you to write a book in a time-limited exam setting,
I expect concise, logically complete answers.
Sign on the line below to indicate that you understand the rules of this exam and the Vanderbilt Honor Code:
A. radioactive decay of radioactive elements inside Io
B. the gravity of Jupiter
C. the tidal influence of Jupiter in combination with the gravitational
influence of Europa
D. ultraviolet light from the Sun
E. Jupiter's magnetosphere
A. has a magnetic field.
B. has no solid surface.
C. rotates extremely fast.
D. has a pronounced equatorial bulge.
A. of the influence of Jupiter's strong magnetic field on Ganymede
compared to the weaker influence of Saturn's weaker magnetic
field on Titan
B. the presence of ring material from Saturn's rings, from which
Titan collects material for its atmosphere
C. Saturn is twice as far from the Sun as is Jupiter
D. of catastrophic events in the history of the solar system.
A. Jupiter is rich in radioactive material
B. Jupiter is a brown dwarf, generating a very small amount of
energy from nuclear fusion
C. Jupiter is still shrinking
D. Jupiter absorbs sunlight effectively at the equator and transfers
that energy to the cloud tops near at polar latitudes.
A. shepherd satellites and the moon Mimas hold the rings in place
B. shepherd satellites hold the rings in place.
C. Saturn's magnetic field holds the rings in place.
D. orbital resonances with Titan hold the rings in place.
A. rather than rotate on it's axis, it tumbles irregularly
B. it has small moons 60 degrees ahead of and behind it in it's orbit,
at the Lagrange points
C. it is two-faced, with a dark side and a bright side
D. has few impact craters and is extremely shiny, probably because it
is coated in fresh ice crystals from water volcanism
A. hydrogen and helium
B. noble gases
C. liquid metallic hydrogen
D. 10 earth masses of rock and iron
A. Io
B. Earth
C. Europa
D. Mars
A. 2,000 : 200
B. 200,000 : 200
C. 200,000,000 : 200
D. 200,000,000,000 : 200
27. [2 pts] Saturn radiates three times as much energy as it absorbs from the Sun. Saturn's energy source is
A. helium rain.
B. radioactivity.
C. nuclear fusion.
D. a mageto-dynamo.
28. [15 pts] In the light
of recent events at NASA (e.g, the loss of Mars Polar Lander [$150 M] last
week, the loss of Mars Surveyor 98 Orbiter [$150M] earlier this fall, the
loss of Mars Observer in 1993 [$1.5 B]; e.g., the successes of the Galileo
mission to Jupiter [$1.5 B], the Mars Pathfinder [$150 M] and Global Surveyor
[$150M] missions in 1997, the Hubble Space Telescope [$4 B]), write an
editorial for the Opinion page of The Hustler in which you take
a position either criticizing the continued expenditure of funds on space
exploration or commending the efforts of NASA and encouraging continued
support for space exploration.
29. Our basic model for the formation of the solar system
is very successful at
explaining almost all
known features of our solar system.
a) [5 pts] briefly describe the basic model for
the formation of the solar system
b) [5 pts] briefly explain which fundamental features
of the solar system are well
explained by this model
c) [5 pts] briefly explain why the discovery
of the extrasolar planets found thus far don't
match this model for planet formation
and how astrophysicists have improved the
model to account for existence of
these planets
d) [5 pts] briefly explain why the discovery
that Jupiter's atmosphere has 2.5 times as
much argon, krypton and xenon
as the Sun requires improving this model yet again
30. [10 pts] How do we explain the
densities of the four main moons of Jupiter?
[Data for Jupiter's four main
moons are given in the table below. ]
| Moon | Distance from Jupiter | Orbital Period | Diameter | Mass | Density |
| Io | 422,000 km | 1.77 days | 3640 km | 1.22 Moon masses | 3.5 gm/cc |
| Europa | 671,000 km | 3.55 days | 3130 km | 0.65 Moon masses | 3.0 gm/cc |
| Ganymede | 1,070,000 km | 7.15 days | 5270 km | 2.02 Moon masses | 1.9 gm/cc |
| Callisto | 1,880,000 km | 16.7 days | 4800 km | 1.46 Moon masses | 1.9 gm/cc |