MARS HABITAT
As part of the campus Life on Mars project involving a number of programs
at the college, Drafting Technology students developed designs for a Mars
habitat. On February 18th, they were judged. John Gaddis took first place,
Chi Lou Cheang took second, and Laurence Dolormente took third. The first
place design will be posted on this page following display of the projects
at public schools on the island.
Part of the campus project recently involved a visit by Dr. Cheick Diarra,
Mission Director for the NASA Pathfinder probe that will land on Mars
July 4, 1997. Dr. Diarra spoke to students and faculty about the project
and demonstrated the "rover" vehicle that will explore the planet.
Dr. Cheick Diarra at Honolulu Community College,
Feb. 5, 1997
Sojourner chassis; Sojourner
attempting to climb a wall
Model of the lander (shown disassembled by Dr.
Diarra in top right photo above)
Drafting Student Winners
in the Mars Project Competition

Left to right: Stephanie Bonsato (3rd Place, Art Competition),
John Gaddis (1st Place, Habitat Competition), Laurence Dolormente (3rd Place,
Habitat Competition), Chi Lou Cheang (2nd Place, Habitat Competition)
Habitat Project Parameters
- Expandable habitat accommodating roughly 12 people to start. 200
sq. ft. sleeping/ private space per person is approximately the minimum.
- Average low temperature about 50 degrees below zero, but temperatures of
of +191 have also been recorded. Mars is in a more eliptical orbit than
Earth's, and its distance from the sun varies by more than 26 million
miles, so temperatures vary greatly. The high temperatures that occur
despite its distance from the sun being greater than that of Earth, is
due to the extremely thin atmosphere that does not impede the sun rays
like on Earth. The habitat will therefore need to be insulated well,
but bulky materials cannot be transported.
- 200-300 mph winds, but air is much thinner than our air, so wind
pressure is not as great as its speed would seem to indicate. Wind
gusts, Marsquakes, etc. are much milder than on Earth. Habitat will probably
need to be sheltered.
- Gravity about 40% that of Earth.
- No significant surface water. It was probably present in the past
and has been proven to occur below the surface, but it is scarce. Polar
caps are probably more dust and dry ice (frozen carbon dioxide) than
water ice. Concrete that requires relatively large quantities of water,
for example, would probably be an inappropriate construction material.
- Atmosphere mostly carbon dioxide. Inhabitants will need to wear
spacesuits when outside. Trees, however, could grow except for the
scarcity of surface water. and extreme heat and cold. Trees use carbon
dioxide and emit oxygen. It would probably be desirable to recover the
oxygen, so trees might be grown in enclosed greenhouses (but heat loss
and heat gain through any glass or other transparent material will need
to be controlled). No protective ozone layer. Since inhabitants will
need to wear spacesuits, dexterity will be limited, and outdoor construction
and assembly activities will need to be minimized. Oxygen will need to
be conserved, and habitat exit-entry airlocks will be required.
- Atmospheric pressure is low, about the same as being 100,000 feet
above sea level on Earth.
- Interior of the planet is rocky. It's low in metal content, but
iron oxide is what gives much of the planet its reddish color. Iron
production, however, requires very high temperatures, an abundant fuel
source, etc., so iron would probably not be produced there until a much
later date. There is a dry clay soil on Mars, and some ideas of producing
brick have been advanced. Any brick manufacturing would need to be very
simple and involve little water -- probably a dry-press process. There
is also a volvacic stone which might be simply shaped somehow and used
as a building material.
-
Irregular terrain. A long valley is 3,100 miles long and 310 miles
wide. Mountain named Olympus Mons is 78,000 feet high and the size of
the state of Missouri at its base. Cliffs are four miles high. Surface
is scarred by lava flows and meteorite impacts.

WATCH FOR MORE TO COME
World Wide Web Address: http://www.hcc.hawaii.
edu/instruct/div6/drafting/mars.htm