Astronomy 101
Spring 2001
1st Midterm Exam
Rules for this exam: This examination is to be taken without help of
books or papers or notes. It is to
be worked on individually; the Vanderbilt Honor Code applies. You may
use calculators. Please write clearly.
General test-taking advice for this exam: Answers require a word,
a phrase, a sentence or perhaps a paragraph, a number or a brief calculation.
Each question has an assigned point value (in brackets), with the points
totaling 100 for the exam. While I don't expect you to write a book
in a time-limited exam setting, I expect logically complete, though concise,
answers. Correct but incomplete answers, or incorrect answers with
correct logical support will receive varying degrees of partial credit.
You must turn in your question sheet with your answer pages (or bluebook).
Name (printed):
Sign on the line below to indicate that you understand the rules
of this exam and the Vanderbilt Honor Code:
I understand the Honor Code of Vanderbilt
University and pledge, by signing,
that I have followed the rules of this
exam and the Honor Code.
Signature:
a) Row (your row number, where the front row of the class is #1):
b) Section (right = far from exit doors or middle or left = near exit doors):
c) Seat (within your row and section, where the left-most seat is #1):
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[5] If the Earth was formed with a population of 512 bazillion radioactive
uranium 235 atoms, and assuming U-235 has a half-life of 0.7 billion years
and the age of the Earth is about 4.2 billion years, how many U-235
atoms remain in the Earth today?
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[5] The moon is on your eastern horizon at midnight. What is the
phase of the moon?
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[5] You observe that high tide occurs at about 3:00 in the afternoon. What
is the approximate phase of the moon?
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[4] Based on radioactive dating, what are the ages of [4 answers required]
the oldest a) rocks found on Earth, b) mineral grains found on Earth, c)
known moon rocks, d) meteorites?
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[3] If the Moon were 30 times as far from the Earth as it is now, how would
the force of gravity between the Earth and Moon compare to its current
strength?
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[5] If the Moon were 30 times as far from the Earth as it is now, what
time(s) of day would low tide occur?
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[5] Comet Halley orbits the Sun in about 80 years; Uranus orbits the Sun
in about 80 years. Uranus' orbit is nearly circular, with a radius of 19.2
Astronomical Units. At perihelion (closest approach to the Sun),
C/Halley just reaches about 0.6 AU. Using the table, below, determine
which and how many planets' orbits C/Halley crosses.
| Mercury |
0.4 AU |
| Venus |
0.7 AU |
| Earth |
1.0 AU |
| Mars |
1.5 AU |
| Jupiter |
5.2 AU |
| Saturn |
9.5 AU |
| Uranus |
19.2 AU |
| Neptune |
30.1 AU |
| Pluto |
39.5 AU |
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[3] What is the principle source of heat inside the Earth?
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[3] Which has a length of 24 hours, a solar day or a sidereal day?
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[3] Which is longer, a solar or sidereal day? Is the difference best described
as a few seconds, a few minutes or a few hours?
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[3] Is the time from full moon to full moon shorter, longer or the same
as the time it takes the moon to orbit the Earth?
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[4] The day, month and year have obvious astronomical origins. What is
the astronomical origin of the unit of time we call a "week"?
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[6] The length of a year is not identical with the length of time required
for the Earth to complete exactly one orbit around the Sun. Why not?
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[6] What is the most important physical reason that we have seasons?
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[6] Two conditions are necessary in order for a solar eclipse to occur.
What are they? Why don't we have solar eclipses every month?
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[6] Tides have produced changes in three different aspects of the Earth-Moon
system. What are these three tidally induced changes?
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[4] Where, in the solar system, have these three aspects of tidal evolution
had the most profound effect? Briefly point out how this system has evolved
further, or more profoundly, than the Earth-Moon system.
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[6] Stable isotopes of carbon exist with 6 (Carbon-12) and 7 (Carbon-13)
neutrons. All, of course, have 6 protons. Why doesn't Carbon-10 exist as
a natural isotope in nature?
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[6] Given only an image of the surface of a cratered moon or planet, how
would you differentiate between craters of volcanic and impact origin?
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[6] What have we learned about the history of the Moon from "crater counting"?
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[6] In round numbers, the present distance to the Moon is about 400,000
km (i.e., the semi-major axis of the lunar orbit, which is fairly circular,
rather than extremely elliptical) and the orbital period of the moon is
27.3 days. If the average rate at which the moon has been spiraling outwards
from the Earth has been 10 cm (0.0001 km) per year for 3 billion years,
by what distance has the moon's orbit expanded over 3 billion years? What
was the Moon's distance from the Earth 3 billion years ago? What was the
orbital period of the Moon 3 billion years ago?