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Space Transportation - mmmt_transportation.pdf - Moon Society

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MMM #10 - November 1987<br />

ESSAYS IN “M” Focus on Farside<br />

By Peter Kokh<br />

M is for Means of <strong>Transportation</strong> to and from a Farside Astronomy site.<br />

Powered portions of rocket (suborbital or not) landings and ascents to and from the lunar surface,<br />

ought not to be allowed in line-of-sight from a Farside Radio Astronomy installation in order to avoid<br />

interference. Instead “Farport” ought to be located at the end of a surface road from the radio telescope<br />

facility at least ten or more degrees away and around the <strong>Moon</strong>’s curvature [c. 200+ mi or 300+ km]. It<br />

might be best to locate Farport inside the farside zone which is within line-of-sight of the L4 and L5<br />

Lagrange points at all times, say within 35° of the central Farside meridian. Then communications too<br />

would be routed via-surface cable to Farport before being relayed to/from the S.E.T.I. telescope facility.<br />

MMM #30 - November 1989<br />

Nuclear rocket using Indigenous Martian Fuel<br />

An Enabling Technology for Manned Mars Missions<br />

with Global Access in a Single Launch<br />

[Body of Paper Condensed by MMM Editor]<br />

Robert M. Zubrin, Martin Marietta, Astronautics, Denver, CO<br />

ABSTRACT: This paper presents a preliminary examination of a novel concept for a Mars descent, ascent, and<br />

exploratory vehicle. Propulsion is provided by utilizing a nuclear thermal reactor to heat a propellant gas indigenous to<br />

Mars to form a high thrust rocket exhaust. Candidate propellants whose performance, materials, compatability, and<br />

ease of acquisition are examined include carbon dioxide, water, methane, nitrogen, carbon monoxide, and<br />

argon. Ballistic and winged supersonic vehicle configurations are discussed. It is shown that the use of this method of<br />

propulsion potentially offers high payoff to a manned Mars mission both by sharply reducing the initial mission mass<br />

required in low Earth orbit, and by providing Mars explorers with greatly enhanced mobility in traveling about the<br />

planet through the use of a vehicle that can refuel itself each time it lands. utilizing the nuclear landing craft in<br />

combination with a hydrogen fueled nuclear thermal interplanetary vehicle and a heavy lift booster, it is possible to<br />

achieve a manned Mars mission in one launch.<br />

INTRODUCTION: Interplanetary travel and colonization can be greatly facilitated if indigenous propellants can be<br />

used in place of those transported from Earth. Nuclear thermal rockets, which use a solid core fission reactor to heat a<br />

gaseous propellant, and which were successfully developed= during the 1960s under the ROVER/NERVA<br />

programs as hydrogen fueled interplanetary transfer vehicles, offer significant promise<br />

in this regard, since, in principle, any gas at all can be made to perform to some extent. In this paper we present a<br />

preliminary examination of the potential implementation of such a concept in the context of manned Mars<br />

missions. The vehicle in question we term a NIMF: Nuclear rocket using Indigenous Martian Fuel.<br />

Candidate Martian Propellants<br />

The atmosphere of Mars consists of 95.0% carbon dioxide [CO2], 2.7% nitrogen [N].1.6% argon [A], all of which are<br />

candidate fuels for NIMF.Water could also be used after harvesting ice or permafrost. Carbon monoxide [CO] and<br />

methane [CH4] can be produced from the above atmospheric gases by processing.<br />

Table 1: Ideal Specific Impulse of Martian Propellants<br />

Temp °K CO2 H2O CH4 CO/N2 A<br />

** 2800 283 370 606 253 165<br />

3000 310 393 625 264 172<br />

* 3200 337 418 644 274 178<br />

3500 381 458 671 289 187<br />

5

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