Mars exploration: Silanes as fuels for Martian ramjet and scramjet engines

F. Vergine, D. Simone, C. Bruno, B. Hidding

Research output: Chapter in Book/Report/Conference proceedingConference contribution book

2 Citations (Scopus)
2 Downloads (Pure)

Abstract

Mars is a rocky planet, with only half the diameter of Earth, a far thinner atmosphere (composed mainly of CO2) and a cold and SiO 2-rich desert-like surface; moreover, from time to time, Mars experience dust storms, growing thousands of kilometers across the atmosphere. These extreme conditions pose questions about propulsion and fuels useful to Mars exploration. The density of Mars atmosphere being less than one-hundredth of a bar makes chemical ground propulsion difficult, and in any case very slow due to the rugged terrain. Rapid survey and excursions over significant planetary distances become feasible only by flying; however, the thin Mars atmosphere cannot provide sufficient lift, unless by flying sufficiently fast to collect the 'right' amount of CO2. The Martian CO2 collected could then be reacted with light metals, as already proposed by Shafirovitch et al in the US and by Golovitchev in Sweden. Here we propose instead to rely on combustion reactions between Martian CO2 and hydrides. In particular, this paper focuses on silicon hydrides ('silanes') because of their interesting combustion and energetic properties; when used as fuels for ramjets and SCRJ, silanes in combination with atmospheric CO 2 seem, at this preliminary stage of analysis, an intriguing conceptual alternative to a conventional LOX/LH2 or LCH4 'hopping' rockets. That gas-turbine propulsion should be excluded on Mars because of dust storms effects on blades. Accordingly, this work explores the practical limits of application of silanes, including their performance for cruising and accelerating. Equilibrium composition of the combustion products of silanes, from monosilane up to pentasilane were calculated. Ideal ramjet and scramjet performance (specific thrust and specific impulse) were evaluated along constant dynamic pressure trajectories in the Mars atmosphere and compared to those with CH4/Air and H2/Air mixtures. High specific thrust is obtained as the equivalence ratio is increased; the Isp trend is the reverse, but still very appealing when weighted with the bulk density of silanes.

Original languageEnglish
Title of host publication61st International Astronautical Congress 2010, IAC 2010
Place of PublicationParis
Pages7473-7485
Number of pages13
Volume9
Publication statusPublished - 1 Dec 2010
Event61st International Astronautical Congress 2010, IAC 2010 - Prague, Czech Republic
Duration: 27 Sep 20101 Oct 2010

Conference

Conference61st International Astronautical Congress 2010, IAC 2010
CountryCzech Republic
CityPrague
Period27/09/101/10/10

Keywords

  • Mars
  • propulsion
  • space exploration
  • fuel
  • silanes

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