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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 />

The magnetic field mapping requires use of a three-axis magnetometer. The magnetic field sensor<br />

would need to be mounted in a location that minimizes magnetic field contamination from<br />

other systems or instruments on the Entomopter. To minimize the magnetic signature of the<br />

Entomopter, it should have as little magnetic materials within it as possible. Also, any magnetic<br />

field-inducing devices (such as the power generation system) will have to be shielded and/or<br />

properly grounded to minimize the magnetic field effects. The mass and power of this type of<br />

device is on the order of 0.2 kg and 150 mW, respectively.<br />

1.3.3.3 Near Infrared and Neutron Spectroscopy<br />

The distribution of water (ice or liquid) is vital to the search <strong>for</strong> life. Neutron spectroscopy is a<br />

powerful technique <strong>for</strong> detecting an excess of hydrogen to a depth of about a meter. Such a technique<br />

can be implemented from orbit but has a resolution of several hundred kilometers. From<br />

the Entomopter plat<strong>for</strong>m, the spatial resolution is several orders of magnitude better, so the<br />

potential exists <strong>for</strong> locating kilometer-sized bodies or much smaller.<br />

Mineralogy is a key tool <strong>for</strong> investigating the <strong>for</strong>mation and geologic history of Mars. Near<br />

infrared spectroscopy can be used to provide data on the mineralogy of Mars. This includes<br />

measuring the pH, abundance and phase of water, atmospheric chemistry, temperature, and surface<br />

pressure. It can also be useful in examining the geologic processes of the planet, such as<br />

sedimentation, volcanism, and hydrothermal alteration.<br />

Mineral makeup can be determined through near infrared absorption and spectroscopic evaluation.<br />

This technique has been widely used in the past both on Earth and <strong>for</strong> planetary exploration.<br />

(It was used on Phobos to determine surface-mineral composition.) Near infrared<br />

spectroscopy (at the wavelengths between 0.7 mm and 2.5 mm) can provide in<strong>for</strong>mation on soil<br />

makeup and identify materials such as iron oxides, iron oxyhydroxides, carbonates, clays, olivines,<br />

and pyroxenes, as well as establish their degree of crystallinity. This type of science will<br />

allow the detection of these minerals and their abundance in the soil.<br />

The objective of any near infrared spectroscopy investigation should be to link the mineralogy<br />

with specific geologic <strong>for</strong>mations on the planet (imagery), thereby providing a more detailed<br />

understanding of the geologic processes of the planet.<br />

The ability to per<strong>for</strong>m imaging spectroscopy from the Entomopter vehicle probably will not be<br />

possible (unless there are significant advances in sensor technology). There<strong>for</strong>e, non-imaging<br />

spectroscopy would be the applicable choice <strong>for</strong> this type of data collection. However, to get<br />

useful data from a non-imaging spectroscopy system, it would need to be closely integrated with<br />

the camera imaging.<br />

1.3.3.4 Radar Sounding<br />

Radar sounding can investigate subsurface structure and search <strong>for</strong> buried ground ice and subsurface<br />

water. This type of exploration from orbiting space craft has been proposed, but by per<strong>for</strong>ming<br />

this from 100 m or so above the surface, increased spatial and depth resolution can be<br />

achieved. Aerial radar sounders have a proven capability to detect subsurface water beneath glacial<br />

ice at a depth of up to 4 km with more than 100 subglacial lakes identified in Antarctica.<br />

20<br />

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

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