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Program 3: Spaceship South Pole
Student Learning Objectives
- Define and compare Earth's "4 South Poles."
- Describe, using the videos and online resources, astronomical research
involving infrared light in Antarctica.
- Work cooperatively to design a new South Pole Station which reflects
climate, environmental considerations, and the human dimension of research
at the Pole.
Summary
Please note: This program will attempt the first-ever live telecast
from the South Pole. This opportunity has been made possible only by the
hard work of nsf, nasa, and the "loan" of a satellite from the National
Oceanic and Atmospheric Administration, noaa. "Firsts" are exciting but
also somewhat risky! We cannot predict what technical or other logistical
problems may result in late changes to program content!
(The New Explorers, hosted by Bill Kurtis, joins MPT to present this
special program and provide a live uplink site in Chicago. The New Explorers
is a co- production of WTTW/Chicago and Kurtis Productions, Ltd.)
Surviving at the Pole is about as good an analogy for living and working
in space as can be found anywhere on Earth, hence the program's title:
Spaceship South Pole. The Live from Antarctica video crew will have spent
the holidays at America's Amundsen-Scott South Pole Station. Students,
of course, know what the holiday is like at the North Pole, but this will
be a revealing and realistic look at the other end of the planet! You'll
see what the 150 or so scientists and support staff in residence get up
to on December 24.
We'll also show everyday life and work in some of the most extreme conditions
anywhere on Earth. The National Science Foundation has begun a total redesign
of the South Pole Station, to make it safer, more energy- efficient, and
better equipped with telecommunications tools in order to upgrade support
for science. We'll explain why the new living modules are raised high
on stilts, and why all other buildings will be situated under ice. We'll
also see plans, in which NASA is collaborating with NSF, to make the new
station far more self-sufficient in food and water-including ideas for
an edible park!
The end of the Earth is also a good place to study the origin of the
Universe, because Antarctica is one of the best astronomical sites on
our planet. Scientists from CARA, the Center for Astrophysical Research
in Antarctica, describe the new telescopes which have been assembled at
the South Pole over the past few years, and show spectacular images from
the impact of Comet Shoemaker-Levy into Jupiter, for which the SPIREX
(infrared) telescope had the most uninterrupted view of any observatory
on Earth. (CARA is a member of the Live from Antarctica educational team,
and has mounted many special files, of interest to teachers and students,
on-line. Please browse and download these to provide additional information
to background this program.)
This program will also feature, live and on camera, the annual repositioning
of the geographical South Pole, necessitated by the slippage of the ice
sheet over the underlying surface. (See April Whitt's "Dairy" entry about
last year's repositioning.) Seventeen-year-old Chicago student Elizabeth
Felton, selected to participate in an NSF program that takes teachers
and students to Antarctica, will help move the marker and have a chance
to make appropriate "ceremonial" comments. Animation from the United States
Geological Survey will describe how Earth's exact geographical South Pole
is determined using Global Positioning Satellites, and also explain the
other three South Poles.
Locations in Antarctica
- The Amundsen-Scott South Pole Station (site of the exact geographic
South Pole and the "ceremonial" Pole).
- Interior: the CARA-Amanda building (site of the controls of the SPIREX
telescope).
Locations in the U S
- Chicago (home of CARA and Elizabeth Felton).
- Virginia (home of third grade teacher April Lloyd, who will also be
at the Pole).
- Hawaii (the only U.S. school system likely to be "live" in regular
sessions during this broadcast, which will be late in the day because
of limited satellite visibilities).
Featured Experts and Educators
MARK HERELD heads the SPIREX (South Pole Infrared Explorer) investigation
at the South Pole. The SPIREX telescope surveys light in near-infrared
wavelengths, looking for galaxies and brown dwarf stars. Because the South
Pole points towards a "hole" in the celestial background, SPIREX can see
light from galaxies formed in the early universe.
NOAA LT. KATE McNITT works for the National Oceanic and Atmospheric
AdministrationÕs Climate Monitoring and Diagnostic Lab. She measures halocarbons,
carbon dioxide, and other substances that affect Earth's climate. She
writes: "I'm an officer in the NOAA Corps, one of 400 men and women commissioned
by the United States government to drive ships, fly airplanes, and serve
as managers for the National Oceanic and Atmospheric Administration. I
spent two years as a junior officer on the NOAA ship, Whiting. We used
sonar equipment to make contour maps of the ocean floor. My favorite parts
of that job were maneuvering the ship and scuba diving on shipwrecks.
I have wintered once before at the South Pole and I'm really looking forward
to a second year in this magic place."
APRIL LLOYD, a third grade teacher from Charlottesville, Virginia, will
spend two weeks at the South Pole. She writes: "I have taught third grade
for the past six years. I am an avid user of technology and believe that
reform in education must incorporate the inclusion of public schools in
the Internet Information Super Highway. My goal is to create a classroom
where students look forward to coming to school each day, where they like
to learn and feel comfortable looking for answers to difficult questions.
If children feel that they have the power to learn, with people available
to help them, our future is bright."
ELIZABETH FELTON: Go on-line for information about Elizabeth, her "Field
Journal" describing her travels from Chicago's public schools to the South
Pole and her dream of becoming an astronaut!
Activity 1: Working in a Freezer
Engage
Before scientists take equipment to the South Pole, they conduct tests
simulating the conditions under which it will have to work. Nothing behaves
quite the way it normally does under such extreme conditions, neither
equipment nor people! It takes about 2-3 times as long to complete a task
as it does under more normal circumstances. As your students go through
this activity, have them think about their own minds' and bodies' responses
to such conditions. Dry ice is very close to the temperature of the South
Pole.
Explore
Build a CO2 Test Box
Students will need a styrofoam cooler, cardboard box, ice chest, or
any type of closed container in which they can place a piece of dry ice.
Have them close the lid and let the "box" temperature stabilize. When
the temperature is constant throughout the inside, we say it is in thermal
equilibrium. Students will need to check the temperature using a thermometer.
When the temperature stops decreasing, students can begin placing objects
into the box to see how the cold affects their ability to work. Some objects
they might try are ball bearings, electric circuits, material samples
(rubber, cotton, wool), wet things, water at different temperatures in
different containers (plastic, paper, metal).
Students can invent their own experiments. Older students may want to
design simple machines, electrical circuits, or motors and compete for
the design that withstands the most cold.
Expand
Have students think about how the cold temperature affects the kind
of work that scientists must do in their research.
- What kinds of activities would be difficult that are easy in temperate
places?
- How does the design of instruments and buildings have to reflect the
cold, dry atmosphere?
- Students might want to go on-line and search CARA's files for letters
from John Briggs and others that contain anecdotes and details about
life at the Pole. (see fig.3.1)
Activity 2: Staking Out the Real South Pole
Engage
If you were to visit the Amundsen-Scott South Pole Station, one of the
first things you would probably do is to have your picture taken next
to the ceremonial South Pole. As you'll see in the videos, it is the one
with the barber pole stripe and reflecting globe on the top. Surrounding
it is a circle of flags of the nations who have signed the Antarctic Treaty.
It is placed where it is because it's in a convenient location close to
the station and within the aircraft "skiway" turnaround circle. But it
is not the true geographic South Pole of the Earth.
The real South Pole is a couple of hundred meters beyond the ceremonial
pole in the direction opposite to the station dome. It is a stake with
a brass plaque on top. Next to it is a sign that labels it as the Geographic
South Pole. This one is the real thing. But if you look beyond it you
see a long line of old pole stakes. In past years, each of these stakes
used to be the Geographic South Pole. Each stake is about twelve feet
long, but about two-thirds gets pounded into the ice. Due to blowing snow,
only the most recent markers are visible.
The reason the Geographic Pole needs to be restaked each year is not
because the Earth's pole itself is moving, but rather because the 3-km-thick
ice sheet is sliding across the continent 10 meters every year. The geographical
marker on the pole moves about 9.2 meters per year along with the flowing
ice.
Explore
If the first marker was staked in 1982, and one has been placed yearly
since then:
- How many are there?
- What is the distance from the first pole to the one staked in 1995?
- If the markers are in a straight line, does that indicate that the
ice sheet moves in a straight line?
- How long before the first marker reaches the ocean?
Students can sketch or trace a model of the continent and mark the South
Pole and their map to scale showing the numbers and positions of each
year's South Pole marker. They should be able to check any mathematical
calculations by their scale map in much the same way the GPS uses two
methods to verify the actual pole location. In addition, after January
12, they will be able to find on-line Elizabeth's and April's descriptions
of what it was like at the Pole.
Explain
There are actually four South Poles. Two, as we have seen, are at the
Amundsen-Scott South Pole Station, but one is not even on the Antarctic
continent! The one that is out in the sea is the south magnetic pole of
the Earth. This is the one that the tail of a compass needle points toward.
The magnetic pole is determined by the magnetic fields that are generated
deep in the Earth's core. These fields move about quite a bit and actually
flip from south to north over long time scales. Thus, the south magnetic
pole is rarely found near the real South Pole of the Earth. The fourth
South Pole is the geomagnetic pole, which is found at the center of the
aurora caused by the intervention of particles originating in the sun
and the Earth's magnetic fields.
At the South Pole, one is standing atop a nearly 3-km-thick icecap.
Over a long time, ice slowly moves downhill. In this case, downhill is
in the direction of the edge of the Ross Ice Shelf, some 1,200 km away.
At this rate, in about 120,000 years the current South Pole Station will
drop into the sea.
Activity 3: South Pole Station Gamma
Objective
To have students analyze and evaluate data and develop an appropriate
model
Engage
The United States owns and operates the Amundsen-Scott Station at the
South Pole. Named for the two explorers who led the first expeditions
to the Pole, it is the most inaccessible, hostile place on Earth, yet
an excellent place to conduct science.
The current facility is really the second to be erected at the South
Pole. The first was installed in the late 1950s, initially on the surface
but snow drifted over it. Another problem was that, over time, the ice
moved, making tunnels and rooms unsafe. It was abandoned in 1975. The
current facility was also built on the surface. (It too is being buried
by drifting snow!) At its centeris a geodesic dome (diameter = 160 ft.).
Under the dome are several separate buildings. Radiating from the dome
are storage and working "arches", large (width = 50 ft.), semi-circular
pieces of corrugated aluminum. Outside are smaller, specialized buildings,
even tents!
Mission: Your mission is to begin the design of the third South Pole
research station, named "Gamma" for the third letter of the Greek alphabet.
You will use elevated building structures as well as "arches." You may
also consider tunneling under the snow to connect the structures. The
structures will need to house about 30 people over the winter and up to
130-140 people in austral summer. The construction will need to be carried
out during the summer.
Explore
Phase 1: Planning the Station
Divide your group into five teams. Distribute a copy of "Cold Facts
About the South Pole" and unit fact sheets to each team. These teams will
work together to design plans for the construction of one of five separate
units of the base.
- Transportation and Engineering Unit
- Science and Technology Unit
- Habitat Support Unit
- Health and Recreation Unit
- Control Center Unit
At the end of your brainstorming time, you should have produced the
following:
- Some draft sketches to share with the whole group
- A set of challenges and questions for the cross-team discussion
- A list of the most important connections to the other four units
- A description of the main environmental problem faced by your unit
- A list of design questions that you would like to ask engineers, researchers,
or scientists regarding the construction of Gamma South Pole Station.
If you are linked to our on-line resources, you will have the opportunity
to send questions to our team of scientists and students working on this
project.
Phase 2: Building the Station
Discussion Questions: What is the most important thing you would need
to study to take your unit's design to the next stage?
Working as an integrated team, design the overall structure. Your class
might want this structure to be a 3-D scale model, blueprint, floor plan,
schematic drawing, or picture. If you have access to a computer with graphics
software, this could be designed on the screen. Each team should contribute
an overall design.
Environmental Issues
- The Antarctic Treaty aims to keep Antarctica the cleanest region in
the world. Except for human wastes, everything else at the South Pole
must be separated and sent back in a process called "retrograding."
- Nuclear wastes (but not nuclear power) and certain chemicals are banned.
- Energy is generated by burning diesel fuel brought in by aircraft.
Fact Sheet 1: Transportation and Engineering Unit
The TE unit is responsible for vehicular activity, construction, managing
and operating fire-fighting equipment.
Unit Facilities Include the following in your first draft:
- skiway operations
- tunneling
- fire fighting
- construction
- vehicles
Specific Constraints
- Outside construction only occurs during summer.
- Skiway maintenance requires keeping the runway snow packed down and
clear of drifts.
- Electric vehicle batteries don't fare well in cold.
- Tunnels between units are necessary. Coldest temperatures (below 70o
F) prevent outdoor travel.
- Aircraft rarely stay at the Pole. Pilots keep engines running, then
return to McMurdo.
Connection Questions
- How does this unit interact with others if a fire occurs?
- What might be used to fight fires? Is a small inside fire the same
problem as for large buildings?
- Where do materials and fuels off-loaded from the aircraft go? What
about things waiting to be loaded?
- What kinds and how many vehicles might be needed?
- How will the base get enough snow to melt for water?
Don't Forget!
- Fire is the greatest danger to the base.
- The aircraft runway, including taxiway and other structures needed
for aircraft.
- Vehicles need frequent maintenance.
- Engines need to be kept warm at all times.
- Construction requires material storage and tool shops.
Fact Sheet 2: Habitat Support Unit
The HS unit is necessary to the survival and operation of all buildings.
One of its most important functions is generating energy for the stations.
HS manages wastes, water, and storage of essential supplies. The unit
is responsible for emergency backup energy systems and stockpiling supplies.
It also separates, recycles, and prepares for shipment wastes that can't
be left at the base.
Unit Facilities Include the following in your first draft:
- temperature control
- energy generation and fuels
- waste management
- water management
- storage and backup
Specific Constraints
- At the present time, diesel fuel brought in by aircraft is the only
reliable and practical way to generate electrical and most heat energy.
- Waste water (dish water, etc.) can't be "dumped" into the snow. (At
this time, human waste is an exception.)
- All fresh water must be generated by melting snow. This requires "mining"
the snow and supplying enough energy to melt it and keep it liquid.
- If there were a power failure or other catastrophe requiring evacuation
of base personnel, delays of up to eight months could occur before an
aircraft could land. Remember, no planes are stationed at the Pole.
Connection Questions
- Should heat be generated in one place and "piped" around or should
it be generated at each building?
- What about water? How would you store and move it?
- Can everything that needs to be stored be frozen?
Don't Forget!
- If you run water pipes below the surface, they must be heated, because
the snow at the pole is -58o F
- Wastes for return to McMurdo must be separated and packed for shipping.
- You'll need toilets.
Fact Sheet 3: Science and Technology Unit
The ST unit conducts the basic science and technology research. It is
the primary reason all the other units exist. Astronomical research exploits
the clear, cold, and stable skies at the Pole. Atmospheric research concentrates
on studying the cleanest air on Earth as well as keeping a watch on the
ozone layer.
Unit Facilities: Include the following in your first draft:
- astronomical observatory (includes two telescopes--one is a radio
telescope dish 8 meters in diameter and the other is an optical telescope
2.5 meters in diameter and 5 meters long)
- human physiology and psychology
- atmospheric science (includes "sniffing" instruments as well as a
place to launch small balloons)
- experimental greenhouse (a provision must be made for lighting in
winter)
- solar energy research
Specific Constraints
- Both astronomy and atmospheric research need to be upwind and as far
as possible from the light, heat, and pollution of the other base activities.
- This unit's facilities also need to be located away from communication
antennas and other sources of electromagnetic pollution.
- Most of the research will be done during the dark winter time.
- The greenhouse is for fresh vegetables that can't be flown in, and
a place where people might enjoy working and being.
- Solar energy is only available in summer.
Connection Questions to get you started:
- If located away from other station units, how will scientists travel
to these facilities during the cold of winter?
- How can the sun's energy be utilized at the Pole?
- Is a reference library needed, and if so, where?
Don't Forget!
- Scientists will generate most of the station's computer information.
- Scientists need workshops and labs to prepare devices and to service
equipment.
- Research telescopes aren't viewed directly with the eye anymore. Astronomers
use video cameras.
Fact Sheet 4: Control Center Unit
The CC unit is the central nervous system of the base. It must monitor
and manage all the information flowing within the station. It's responsible
for all communications within the base as well as between the base and
the outside world.
Unit Facilities :Include the following in your first draft:
- systems monitoring
- environmental protection (This means monitoring weather changes and
alerting rest of crew when precautionary or emergency actions need to
be taken.)
- communications
- computing and information management
- general offices and meeting area
Specific Constraints
- Internal communications must rely on the station's own systems. There
is no outside-operated phone system.
- Data communications with the outside must be done using a satellite
that "wanders" into view for a few hours every day. All normal satellites
are below the horizon at the Pole.
- Voice communication with the outside world is on high-frequency (short-wave)
radios.
- The snow doesn't conduct electricity, so itÕs impossible to ground
everything properly. Furthermore, the extremely cold temperatures make
the transmission of weak electrical currents inefficient. This means
that buildings should be connected by nonconducting links--fiber optics
or radio.
Connection Questions
- What about recreational and personal communications using computers?
Should they be done here or in the HR unit?
- How important are personal communications with the outside world?
- What would happen to this area if there were any interruption in power?
Don't Forget!
- There must be a way to alert people when there is an emergency. That
means that this unit must be operated continuously.
- This unit handles its own as well as regional air-traffic control.
- You'll need to place the communications antennas well away from the
ST unit.
- Station computer is managed by this unit.
Fact Sheet 5: Health and Recreation Unit
The HR unit is where the station personnel will spend all of their time
when not working. They will sleep, eat, and play here. This unit also
contains the medical facilities where the doctor works and can perform
simple medical procedures.
Unit Facilities: Include the following facilities on your first-draft
design:
- leisure and exercise
- personal hygiene
- galley
- health maintenance
- crew quarters
Specific Constraints
- There is no broadcast TV or AM/FM radio at the Pole.
- Outdoor recreation is severely limited by the cold. There is some
cross-country skiing, but when it's very cold, all outside movement
is prohibited.
- The isolation and cramped quarters make individual bunk rooms desirable.
- Major medical problems are handled by evacuation. There is no need
to plan for hospital or surgical needs.
- Smoking is prohibited everywhere.
Connection Questions
- How much space will be needed to bunk everyone?
- What sort of wastes will be generated by this unit and who will have
to take care of them?
Don't Forget!
- The galley will provide food storage space.
- Facilities for cleaning clothes.
- The galley kitchen is a prime fire hazard.
- Recreation facilities should allow a well-rounded range of exercise
as well as some team-sport games.
- Provide facilities for nonathletic pursuits, reading, and board games.
Amundsen-Scott South Pole Station
The United States' Amundsen-Scott South Pole Station is named for the
two explorers who led the first expeditions there from 1911-1912. Located
in perhaps the most inaccessible and hostile environment on the earth,
it is also an excellent place to conduct many types of scientific research.
In many ways, it can be considered an analog to future bases on the Moon
or Mars. From this vantage point atop the three-kilometer-thick polar
ice sheet--the coldest, driest desert in the world--astronomers hope to
achieve the clearest views possible of the most distant reaches of the
observable universe from the surface of the earth.
The key to achieving their goals is establishing a base of operations
that will allow them to work and operate their telescopes through the
six-month- polar winter, when observing conditions are best, and living
conditions are worst! To that end, work has been proceeding for the past
several years on a new complex of telescopes and supporting laboratories
approximately one kilometer from the geodesic dome of the main South Pole
base. It is called the "dark sector," reflecting the fact that the telescopes
need to be isolated from the effects of light, heat, and electromagnetic
interference resulting from the other activities required to support life
in the harsh polar environment.
Telescopes now being installed at the site will support research by
the Center for Astrophysical Research in Antarctica (CARA) aimed at investigating
the formation of structure in the universe. The CARA telescopes include
SPIREX (the South Pole Infrared Explorer), COBRA (a Cosmic Microwave Background
Anisotropy experiment), and AST/RO (an Antarctic Submillimeter Telescope
and Remote Observatory). All of these telescopes make use of the special
properties of the polar environment and climate to observe types of radiation
that can't be seen by the human eye.
Note: Additional activities on the characteristics of infrared light
and its use in astronomy and in cryogenics can be found on-line.
Cold Facts About the South Pole
Site Conditions
- Temperatures: Mean = -58o F. Max. = +7.5o F. Min. = -117o F.
- Altitude: 9,300 feet. Cold and polar location make it effectively
10,600 feet elevation. Humidity is the lowest on Earth.
- Precipitation: Less than 1 foot accumulation per year. The topography
is flat for hundreds of miles around the South Pole. As a result, any
structure resting on the surface accumulates snow drifts and is eventually
buried.
- Wind: Average speeds are 12 mph. They rarely go above 20 mph, nor
change direction.
- Glacier: Ice thickness is 9,000 feet. and moves at a rate of about
30 feet per year at the Pole. The plateau maintains this elevation for
nearly one million square miles. The South Pole sits on the largest
source of fresh water in the world.
- Sunlight: The sun is totally above the horizon from Sept. 23 to March
21. Twilight lasts approximately a month, followed by polar night from
April 15 to Aug. 15.
Logistics & Communications
- Route: The South Pole is 800 miles from McMurdo Station, the US facility
that provides supplies and support.
- Aircraft: Six LC130 Hercules aircraft are able to land at the Pole.
Each can carry 11 tons of cargo. There are no winter landings.
- Communications: Normal geostationary satellites are not above the
horizon at the South Pole. Currently, the station depends upon an old
satellite (ATS-3) that is visible for a few hours per day. Land phone
lines are impossible considering the distances and environment. High-
frequency radio is used, but only for voice and it is often interrupted
by solar activity.
Repositioning the Pole, 1993
December. 26, 1993
Amundsen-Scott South Pole Station, Antarctica
Well, it's Boxing Day here at South Pole Station. It's also Sunday so
the ASA staff has the day off, and weÕre fending for ourselves on the
food front. The weather has been utterly beautiful. Yesterday was -25
F, windchill -60 F, but still not bad for short walks. Today there's some
breeze, and it's amazing how much colder that makes it feel!
At 2:00 this afternoon the official South Pole was placed in its carefully
calculated spot.
Cathleen McDermott and Dale Benson of the USGS (United States Geological
Survey) brought the pole with them on the plane trip to the Pole. The
geographical marker on the pole moves about 9.2 meters per year with the
flowing ice. They used two methods to find the new spot. One is called
the Shadow Tip method. If you stand where the pole is and look, you can
see the straight line of poles stretching off toward the distance. The
Shadow Tip method involves putting a tripod on top of the old marker and
sticking an eight foot pole on the tripod. When the sun gets to azimuth
40 degrees west of north, it is lined up with the other markers, and the
tip of the shadow of the eight foot pole marks where the new pole should
go. Early Saturday morning they made the measurements.
The other method used the Global Positioning System (GPS). A satellite
network was used to determine X and Y lines and their intersection was
0 degrees (or 90 south). The GPS reading is a few inches off from the
shadow- tip reading, so there is an official pole at the shadow tip and
a little pipe at the GPS spot.
The pole is about twelve feet long, but about two-thirds gets pounded
into the ground (ice). There were about 30-35 people out in the blowing
snow (the sky clouded over at about 10:30 this morning, the temperature
was -9 F, wind chill -46 F: colder than yesterday!) Dale explained how
the position of the pole was determined. He said that it has been 350
days since the last pole was placed (Jan. 8 of this year). Cathy put the
pole on the spot and Dave Fischer got to take the first whack at pounding
it in, with the special neon orange mallet.
Then each of us got to take a turn pounding it in ...The pole has a
decorative plaque on top, which was protected from our pounding by some
bubble wrap and a small block of wood held on with rubber bands. After
everyone had had their picture taken pounding on the pole, somebody finished
pounding it in the rest of the way, and the protective wood was removed.
The plaque has a little dome on it that looks like the station dome. When
I have time, and the wind dies down, I will go look more carefully at
the others. It was lots of fun, but the wind was so cold we went back
in for hot chocolate right away. And the REAL POLE is set for another
year.
April Whitt
(Editor's note: April Whitt, a high school educator, spent time at South
Pole in the austral summer of 1993.)
Resources
Books
Bender, Lionel. Telescopes. Rourke, 1991, 48 pp., illus,. gr. 5-8.
Chaple, Glenn F. Exploring with a Telescope. Watts, 1988, 128 pp., gr. 7-up.
Hackwell, John W. Desert of Ice: Life and Work in Antarctica. Charles
Scribner's Sons, 1991.
Our Changing Earth. National Geographic Society,
1993, 200 pp.
Taylor, Barb. Bouncing and Bending Light. Franklin Watts, 1990, 32 pp.
Taylor, Barb. Electricity and Magnets. Franklin Watts, 1990, 32 pp., gr. 5-8
Unlocking the Secrets of the Universe. National Geographic Society, 1993, 200
pp.
Magazine Articles
"Antarctic astronomy," anonymous, Sky and Telescope, April 1994, p. 10.
"Building a snow dome," by Cliff Jacobson, Boys Life, Dec. 1992, p. 66.
"In Antarctica, scientists go with the floe," by Michael Stroh, Science
News, Feb. 22, 1992, p. 115.
"Reclaiming a lost Antarctic base," by Michael Parfit, National Geographic,
March 1993, pp. 110-126.
Filmstrips and Videos
Science on Ice: Research in Antarctica, produced by Cable News Network,
available from Britannica, VHS video, 21 minutes.
Light and the Electronic Spectrum, Coronet/MTI Learning Corporation, VHS
video, 14 minutes, gr. 4-12.
Electricity and Magnetism, Coronet/ MTI Learning Corporation, VHS video,
17 minutes, gr. 4-12.
Global Forecasting, Coronet/MTI Learning Corporation, VHS video, 14
minutes, gr. 4-12
The Blue Planet, an IMAX Space Film about the Earth, 1990, VHS videotape,
40 minutes, for all grade levels.
Apparatus
Project STAR Spectrometer, Harvard Center for Astrophys Project STAR,
$19.95 (hands-on exploration of light with this spectrometer).
Project STAR Telescope, available from The Astronomical Society of the
Pacific, San Francisco, CA, $13.95.
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