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Phase II Final Report - NASA's Institute for Advanced Concepts

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Planetary Exploration Using Biomimetics<br />

An Entomopter <strong>for</strong> Flight on Mars<br />

Table 3-16 lists the potential bipropellant combinations and monopropellants that would be<br />

applicable. Also given is the Isp of each propellant. This can be used to gauge the energy contained<br />

within the propellant. The higher the Isp the greater the energy released during combustion.<br />

Table 3-16: Propellant Candidates based on Temperature and Operational State<br />

Requirements<br />

Propellant Oxidizer/Fuel Ratio Isp<br />

Combustion<br />

Temperature ( o C)<br />

Fuel: Monomethyl Hydrazine<br />

Oxidizer: Nitrogen Tetroxide 2.20 288 3,122<br />

Fuel: Monomethyl Hydrazine<br />

Oxidizer: Chlorine Trifluoride 3.00 283 3,318<br />

Fuel: Monomethyl Hydrazine<br />

Oxidizer: IRFNA 2.50 274 2,848<br />

Fuel: UDMH<br />

Oxidizer: Nitrogen Tetroxide 2.70 286 3,162<br />

Fuel: UDMH<br />

Oxidizer: Chlorine Trifluoride 2.85 278 3,306<br />

Fuel: RP-1<br />

Oxidizer: IRFNA 4.90 263 2,881<br />

Monopropellant: Hydrogen Peroxide<br />

na 148 757<br />

Monopropellant: Ethylene Oxide na 199 1,004<br />

Monopropellant: Nitromethane na 245 2,192<br />

Monopropellant: n-Propyl Nitrate na 209 1,077<br />

Monopropellant: HPB na 200 ----<br />

Monopropellant: HAN na --- ----<br />

3.5.2.2 Fuel Production<br />

A key Entomopter capability is our ability to refuel it while it is on the Mars surface. One potential<br />

method <strong>for</strong> achieving this is to produce the fuel from resources found within the Mars environment.<br />

A list of the elements and compounds is given in the environmental section <strong>for</strong> both<br />

the soil and atmosphere. From the listing of elements and compounds available, it can be seen<br />

that there is very little hydrogen available on Mars. The only compound containing hydrogen is<br />

the trace water vapor within the Mars atmosphere, and this constitutes only 0.03% of the atmosphere<br />

makeup. However all the propellants listed in Table 3-13 require hydrogen. There<strong>for</strong>e it<br />

will need to be assumed that unless a water source is found on Mars, the hydrogen needed to<br />

produce the selected fuel will need to be brought from Earth. As of this writing, data from the<br />

Mars Odyssey spacecraft has indicated that there may be large quantities of subsurface water on<br />

176<br />

<strong>Phase</strong> <strong>II</strong> <strong>Final</strong> <strong>Report</strong>

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