The Case for Mars (57 page)

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Authors: Robert Zubrin

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Perigee:
The lowest point in an orbit around a planet.

 

Pyrolyze:
The use of heat to split a compound into its elemental constituents.

 

Regolith:
What most commonly refer to as dirt.

 

rem:
The measure of radiation dose most commonly used in the United States. One hundred rems equals one Sievert, the European unit. It is estimated that radiation doses of about 60 to 80 rem are sufficient to increase a person’s probability of fatal cancer at some time later in life by 1 percent. Typical background radiation on Earth is about 0.2 rem/year.

 

RWGS:
Reverse water-gas shift reaction.

 

RIG:
Radioisotope thermoelectric generator.

 

Sabatier reaction:
A reaction in which hydrogen and carbon dioxide are combined to produce methane and water. The Sabatier reaction is exothermic, with aypicalquilibrium constant (see above).

 

Saturn V:
The heavy-lift launch vehicle used to send the Apollo astronauts to the Moon. The Saturn V could lift about 140 tonnes to LEO.

 

SEI:
Space Exploration Initiative.

 

SNC meteorites:
Named for the locations where the first three were found (Shergotty, Nakhla, and Chassigny), SNC meteorites are believed on the basis of very strong chemical, geologic, and isotopic evidence to be debris thrown off of Mars by impacting meteorites.

 

Sol:
One Martian day; 24.6 hours long.

 

Solar flare:
A sudden eruption on the surface of the Sun that can deliver immense amounts of radiation across vast stretches of space.

 

SPE:
Solid polymer electrolyte.

 

Specific impulse:
The specific impulse of a rocket engine is the number of seconds it can make a pound of propellant deliver a pound of thrust. If you multiply the specific impulse of a rocket engine, given in seconds, by 9.8, you will obtain the engine’s exhaust velocity in units of meters/second. Specific impulse is generally viewed as the most important factor in judging a rocket engine’s performance. Frequently abbreviated “Isp.”

 

SRB:
Solid rocket booster.

 

SSME:
Space Shuttle main engine.

 

SSTO:
Single-stage-to-orbit.

 

Stable equilibrium:
An equilibrium condition, which, if displaced by some external force, will return on its own to its original state. A ball on top of a hill is in unstable equilibrium, because if pushed in either direction it will roll away, accelerating itself from its original position. A ball on a flat surface in the bottom of a bowl is in stable equilibrium, because if pushed, it will roll back to its starting point.

 

STR:
Solar thermal rocket.

 

Telerobotic operation:
Remote control of some device, such as a small Mars rover equipped with TV cameras, by human operators at a significant distance away.

 

Thrust:
The amount of force a rocket engine can exert to accelerate a spacecraft.

 

Titan IV:
An expendable launch vehicle manufactured by the Lockheed Martin Corporation capable of delivering 20,000 kg to LEO or 5,000 kg to a minimum energy trans-Mars trajectory.

 

TMI:
Trans-Mars injection, a maneuver which places a payload or spacecraft on a trajectory to Mars.

 

TW:
Terrawatt, one terrawatt equals 1,000,000 megawatts. Human civilization today uses about 13 TW

 

TW-year:
The total amount of energy associated with the use of one terrawatt for one year.

 

Unstable equilibnum: See
stable equilibrium, above.

 

Vapor pressure:
The pressure exerted by the gas emitted by a substance at a certain temperature. At 100°C, the vapor pressure of water is greater than the Earth’s atmospheric pressure and so it will boil.

 

W/kg:
watts per kilogram.

 

NOTES

 

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P. Berton,
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2.
G. Levin
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The NASA Mars Conference
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3.
N. Horowitz, “The Biological Question of Mars,” D. B. Reiber, ed.,
The NASA Mars Conference
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4.
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5. A. Cohen et al.,
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Government Printing Office, Washington, DC, 1989.

6.
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7.
T. Stafford et al.,
America at the Threshold: Report of the Synthesis Group on America’s Space Exploration Initiative
, U.S. Government Printing Office, Washington, DC, May 1991.

8.
R. Zubrin and D. Weaver, “Practical Methods for Near-Term Piloted Mars Missions,” AIAA 93-2089, 29th AIAA/ASME Joint Propulsion Conference, Monterey, CA, June 28-30, 1993. Republished in
Journal of the
British
Interplanetary Society
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9.
M. Goldman, “Cancer Risk of Low Level Exposure,”
Science
, March 29, 1996.

10.
S. Kondo, Health
Effects of Low Level Radiation
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11.
C. Comar et al., “The Effects on Populations of
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12.
B. Clark and L. Mason, “The Radiation Show Stopper to Mars Missions: A Solution,” presented to the AIAA Space Programs and Technologies Conference, Huntsville, AL, September 1990.

13.
L. Simonson, J. Nealy, L. Townsend, and J. Wilson, “Radiation Exposure for Manned Mars Surface Missions,” NASA Technical Publication-2979, Washington, DC, 1990.

14.
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Nature
, 330, no. 24 (1987):709-10.

15.
A. Thompson, “Ar
tificial Gravity for Long Duration Space missions,” presentation to Martin Marietta Scenario Development Team, February 1990.

16.
M.
Carr,
Water on Mars
, Oxford University Press, New York, 1996, pp. 24-29.

17.
J. Gooding, “2005 Sample Return: Martian Meteorites and Curatorial
Plans,” presentation to the Mars Exploration Long-Term Strategy Working Group, Johnson Space Center, Houston, TX, September 20, 1995.

18.
R. Zubrin, S. Price, L. Mason, and L. Clark, “Report on the Construction and Operation of a Mars In-Situ Propellant Production Plant,” AIAA-94-2844, 30th AIAA Joint Propulsion Conference, Indianapolis, IN, June 1994. Republished in
Journal of the British Interplanetary Society
, August 1995.

19.
R. Zubrin, S. Price, L. Mason, and L. Clark, “An End to End Demonstration of Mars In-Situ Propellant Production,” AIAA-95-2798, 31st AIAA/ASME Joint Propulsion Conference, San Diego, CA, July 10-12, 1995.

20.
B. Clark, “A Day in the Life of Mars Base 1
” Journal of the British Interplanetary Society
, November 1990.

21.
B Mackenzie, “Metric Ti
me for Mars,” AAS 87-269, in C. Stoker, ed., The
Case for Mars III
, Volume 75, Science and Technology Series of the American Astronautical Society, Univelt, San Diego, CA, 1989.

22.
B. Mackenzie, “Building Mars Habitats Using Local Materials,” AAS 87-216, in C. Stoker, ed., The
Case for Mars III
, Volume 74, Science and Technology Series of the American Astronautical Society, Univelt, San Diego, CA, 1989.

 

23.
R. Boyd, P. Thompson, and B. Clark, “Duricrete and Composites Construction on Mars,” AAS 87-213, in C. Stoker, ed., The
Case for Mars III
, Volume 74, Science and Technology Series of the American Astronautical Society, Univelt, San
Diego, CA, 1989.

24.
B. Jakowsky and A. Zent, “Water on Mars: Its History and Availability as a Resource,” in J. Lewis, M. Mathews, and M. Guerreri, eds.,
Resources of Near-Earth Space
, University of Arizona Press, Tucson, 1993.

25.
C. Stoker et al., “The Physical and Chemical Properties and Resource Potentials of Martian Surface Soils,” in J. Lewis, M. Mathews, and M. Guerreri, eds.,
Resources of Near-Earth Space
, University of Arizona Press, Tucson, 1993.

 

26.
T. Meyer and C. McKay, “The Atmosphere of Mars—Resources for the Exploration and Settlement of Mars,” AAS 81-244, in p. Boston, ed., The
Case for Mars
, Volume 57, Science and Technology Series of the American Astronaut
ical Society, Univelt, San Diego, CA, 1984.

27.
J. Williams, S. Coons, and A. Bruckner, “Design of a Water Vapor Adsorption Reactor for Martian In situ Resource Utilization,”
Journal of the British Interplanetary Society
, August 1995.

28.
G. O’Neill,
The High Frontier
, William Morrow, New York, 1977.

29.
J Lewis and R. Lewis,
Space Resources: Breaking the Bonds of Earth
, Ch
apter 9, Columbia University Press, New York, 1987.

30.
R. Zubrin, “Diborane
/CO
2
Engines for Mars Ascent Vehicles,” AIAA 95-2640, 31st AIAA Joint Propulsion Conference, San Diego, CA, July 10, 1995. Republished in
Journal of the British Interplanetary Society
, September 1995.

31.
S. Geels, J. Miller, and B. Clark, “Feasibility of Using Solar Power on Mars: Effects of Dust Storms on Incident Solar Radiation,” AAS-87-266, in C. Stoker, ed.,
The Case for Mars III
, Volume 75, Science and Technology Series of the
American Astronautical Society, Univelt, San Diego, CA, 1989.

32.
R. Haberle et al., “Atmospheric Effects on the Utility of Solar Power on Mars,” in J. Lewis, M. Mathews, and M. Guerreri, eds.,
Resources of Near-Earth Space
, University of Arizona Press, Tucson, 1993.

33.
M. Fogg, “Geothermal Power on Mars,”
Journal of the British Interplanetary Society
, Nov. 1996.

34.
R. Zubrin, “Nuclear Thermal Rockets
Using Indigenous Martian Propellants,” AIAA-89-2768, AIAA/ASME 25th Joint Propulsion Conference, Monterey, CA, July 1989.

35.
R. Zubrin, “Long Range Mobility on Mars,”
Journal of the British Interplanetary Society
, 45 (May 1992), pp. 203-210.

36.
B. Cordell, “A
Preliminary Assessment of Martian Natural Resource Potential,” AAS 84-185, in C. McKay, ed.,
The Case for Mars II
, Volume 62, Science and Technology Series of the American Astronautical Society, Univelt, San Diego, CA,
1985.

37.
R. Zubrin and D. Baker, “Mars Direct, Humans to the Red Planet by 1999,” IAF-90-672, 41st Congress of the International Astronautical Federation, Dresden, Germany, October 1990. Republished in
Acta Astronautica
, 26, no. 12 (1992): pp
. 899-912.

38.
R. Zubrin and D. Andrews, “Magnetic Sails and Interplanetary Travel,” AIAA-89-2441, AIAA/ASME, 25th Joint Propulsion Conference, Monterey, CA, July 1989. Published in
Journal of Spacecraft and Rockets
, April 1991.

 

39.
A. Clarke,
The Snows of Olympus: A Garden on Mars
, W.W. Norton, New York, 1995.

40.
M. Fogg,
Terraforming: Engineering Planetary Environments
, S
ociety of Automotive Engineers, Warrendale, PA, 1995.

41.
R. Forward, “The Statite: A N
on-Orbiting Spacecraft,” AIAA 89-2546, AIAA/ASME, 25th Joint Propulsion Conference, Monterey, CA, July 1989.

42.
C. Sagan
, “The Planet Venus,”
Science
, 133 (1961):849—858.

43.
J. Pollack and C. Sagan, “Planetary Engineering,” in J. Lewi
s, M. Mathews, and M. Guerreri, eds.,
Resources of Near-Earth Space
, University of Arizona Press, Tucson, 193.

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