AST 309 (46575) Fall 2003
Quiz 2: Study List
Review Sessions
Review sessions have been scheduled for the following times
and places: Oct 30th (Thursday), 5-6:30PM in Garrison 1; Nov 3rd
(Monday), 5-6:30PM in Geology 2.324. Bring your questions!
Be sure to bring your calculator and your astrolabe
on the day of the quiz, as well as to the review session!
Reminder
You are reminded to make handwritten notes to yourself
on one side of an 8.5x11-inch piece of paper, which you may consult
during the quiz. These notes will count 10% of your grade. The
quiz questions will emphasize your ability to reason and think,
not memorize isolated facts, and the notes are intended to reduce
your reliance on rote memorization. Your notes must be signed
and attached to your quiz when you hand it in.
Study Questions
- Define Apparent Solar Time. Explain how it can be determined
by direct measurements of the Sun. Explain how the Equation of
Time results from the facts that the Earth's orbit is elliptical,
and that the Ecliptic is tilted with respect to the Celestial
Equator. Explain the difference between Local Apparent Solar
Time, Local Mean Solar Time, Standard (Zone) Time, and Universal
Time. List and explain the corrections that must be applied to
convert between them. Be able to apply these conversions using
your astrolabe.
- Define Sidereal Time. Explain how it can be measured from
observations of the sky. What is it used for? Explain how Sidereal
time is used as the practical method for determining Universal
Time. If you know the Sidereal Time, and also the date of the
year, explain how you would determine the Mean Solar Time. For
example, if today's date is October 22, one months after the
Autumnal Equinox, and it is 8 h Sidereal Time, what is the Local
Mean Solar Time? (Use your astrolabe).
- Explain how the Pendulum works, using the law of conservation
of energy. List and explain some ways that the pendulum can be
improved as a timekeeping mechanism. Define the "Q"
of a resonator such as the pendulum, and estimate the "Q"
of a typical pendulum such as the one we investigated in class
in terms of an actual experiment. (For example, suppose that
the pendulum is a 2-second pendulum, and it takes 2 minutes for
its swings to die down to 1/3 of the original. What would be
the "Q" of such a pendulum?) Explain why the "Q"
of a resonator is important for time keeping.
- Draw a block diagram of each of the clocks on the list below.
The diagram should show how the components of the clock relate
to each other, and should clearly explain the function of each
component. Identify the component of the clock that is most critical
to the accuracy and stability of the clock, and explain the physical
principle of its operation. Estimate the accuracy and stability
of the clock. Explain particular advantages and disadvantages
that each clock may have. Here are some clocks that you should
be prepared to discuss:
Water Clock (Clepsydra)
Pendulum Clock
Quartz Crystal Oscillator
Ammonia Resonator
Cesium Beam Clock
Rubidium Clock
Hydrogen Maser Clock
- Define UT-0, UT-1 and UT-2. Explain how each system of time
measurement is related to the next, and the physical reasons
why the three differ from each other. Define UTC. Explain how
"Leap seconds" are used to keep UTC in step with Earth
rotation time (UT-2), and why this is done. Explain the role
of the BIPM (Bureau International des Poids et Mésures)
in regulating the international system of timekeeping.
- Explain how ancient eclipses and even more ancient coral
reef deposits help us to learn about the history of the rotation
of the Earth. Explain the nature of the evidence and why it gives
us information about earth rotation in the past. Explain the
physical reasons for the slowing down of the rotation of the
Earth.
- What is Ephemeris Time (Dynamical Time)? How is it measured,
in practice? Why was the measurement of Ephemeris Time based
on the Moon, even though its definition is in terms of the Sun?
- For each of the following techniques or devices, explain
the principle of its operation and how it is used to determine
information about Earth Rotation or Time. Discuss the kinds of
errors that the technique is subject to, and how they may be
accounted for.
Lunar Laser Ranging
Very Long Baseline Interferometry (VLBI)
- Explain the basic principles of navigation: How can one use
astronomical measurements to determine latitude? Longitude? Distinguish
between astronomical and geodetic (map) latitude. What was the
Problem of Longitude? How did people propose that it should be
solved (list and explain the principle of at least 3 methods)?
How was it ultimately solved?
- Explain (a diagram would be very helpful) what a line (or
circle) of position is. Show how, with two lines (or circles)
of position, your location on the surface of the Earth can be
pinpointed. Explain the basic idea of how a line (or circle)
of position can be plotted, given an astronomical observation
of the altitude or zenith distance of a star. Why might a third
line (or circle) be needed to completely pinpoint ones location
on the surface of the Earth?
- What is Loran-C? Explain how it works. How many Loran stations
must you receive in order to obtain your position and the time
from Loran? Explain why we need this many stations. How accurate
is Loran-C in determining your position (rough error in meters),
given the fact that the typical error in the time of receipt
of the Loran signal is approximately 0.5 microseconds (millionths
of a second)? [Recall that in a nanosecond--a billionth of a
second--light travels about a foot.]
- What is GPS? Explain how it works. What is the minimum
number of GPS satellites one must receive in order to obtain
your postion and time using the GPS system? Explain why this
is so. How accurately can civilians use GPS to determine their
location? What factors limit the accuracy of GPS for civilian
users? How accurate is GPS in position determination for those
using military receivers? What techniques can civilians use in
order to get very precise information from GPS despite the deliberate
degradation that has been built into it for civilian use?
- Explain how the ratio of [235]U to [238]U can be used to
estimate the age of the heavy elements in the Earth, i.e., how
long ago it was when the supernova that produced the heavy elements
in the Earth's crust blew up. About how long ago was that event?
Suppose that the earth were one billion years old, and suppose
it started with equal proportions of [235]U and [238]U. What
would we expect the proportions of these isotopes to be today?
Be able to do similar calculations.
- Describe each of the following dating methods and explain
how it works: Explain the assumptions of the method, and how
the validity of the assumptions can be checked. What kind of
objects can be dated by each method? What do the various dating
methods tell us that the age of the Earth, Moon, and meteorites
is?
- Carbon-14 dating method.
- Uranium/Lead and Thorium/Lead [206]Pb/[238]U, [207]Pb/[235]U
and [208]Pb/[232]Th;
- Rubidium/Strontium Isochron ([87]Sr/[86]Sr versus [87]Rb/[86]Sr);
- Potassium/Argon ([40]K versus [40]Ar).
- Explain how the H-R diagrams of globular clusters are used
to estimate the ages of the most ancient stars in our galaxy.
Explain how the cooling curves of white dwarf stars can be used
to obtain the same information. Approximately what is the age
of the oldest stars in our galaxy, according to these methods?
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