ASTRONOMY 301
HOMEWORK SET #2
DUE: 03 OCTOBER
How to maximize your marks on the homework:
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show all steps in the simple required calculations. That way, if
you make an arithmetic error on a question, it still may be
possible for us to assign partial credit.
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write complete sentences. Be legible! We can't give a grade to
something we can't read.
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cleanly labeled diagrams are almost always helpful and sometimes
are required for a complete explanation.
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come to the help sessions if you are not absolutely clear on how
to do any of the questions.
THE PURPOSE OF COMPUTING IS INSIGHT, NOT NUMBERS
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Suppose that magically one day our Sun is taken away and in its place is put a
star that is one-third times the Sun's mass. First, compute the length of our
new "year" (in days, say) if we insist in keeping the Earth at a distance of 1
AU from the new star, just as we now are from the Sun. Then compute how far
away we would orbit this new star (in AU, say) if we instead insisted on
keeping the length of the year the same as it is now. Comment!
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Compare your weight now (we are nearly at sea level) to the weight you would
have on top of Mount Everest. It is OK to keep this answer as a ratio, or you
can turn it into an actual number of pounds less or more that you would weigh
when on Mount Everest. Comment!
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What is the altitude above the Earth's surface of a "geosynchronous"
satellite (one that always hovers above the same spot on the Earth)?
Hint: begin with Kepler's Third Law. Comment!
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The planet Neptune was predicted to exist before it was actually
discovered, because the planet Uranus was obviously being pulled away from
its expected orbit by the gravitational pull of some other object.
At the point in time when Uranus and Neptune are lined up exactly on the
same side of the Sun, Neptune and the Sun pull on Uranus in opposite
directions. What is the ratio of the gravitational forces of these
two objects on Uranus at this time? Comment!
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Compare the Earth-Moon force of gravity on the side of the Earth
facing to the Moon to the force on the side facing away from the Moon.
Do the same thing for the Earth-Sun force of gravity. This should
tell you why the Moon has a higher tidal influence on the Earth
than the Sun does, right? Comment!
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Compare the light-gathering powers of a) a typical amateur
astronomer's telescope (D= 6 inches), the original McDonald Observatory
telescope (D= 82 inches) and c) the new Hobby-Eberly Telescope
(D= 360 inches, approximately).
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The Andromeda galaxy is our nearest very large neighboring spiral
galaxy. What is the angular diameter of the main stellar part of the
Andromeda galaxy (it is 40 kpc across and 670 kpc away from us)?
How does this compare with the angular size of the moon?
What is the angular diameter of the diameter of the bright nucleus
(which is 3 pc in size) at the center of the Andromeda Galaxy?
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