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Distributed Spectrometer for use on
Mars
We will develop a mobile science instrumentation system capable of
doing wide-area surveys for the detection of biogenic gases that may serve
as indicators of life on Mars. Future surface rover missions of
astrobiology interest would benefit from a capability to increase in situ
measurement coverage and improve chances of detecting biosignatures. We
will provide this capability in the form of a distributed spectrometer
instrument system employing a rover and lander. Our goal is to develop a
spectroscopy system for survey, detection, and in situ measurements of
biogenic gases for their detection and quantification. Gases to be probed
include methane, ammonia, hydrogen sulfide, oxygen, carbon monoxide,
sulfur dioxide, nitrous oxide and formaldehyde. We will investigate the
feasibility of detecting isotopic ratios of key gases with the
instrument.
The instrument system is a variable path-length
spectrometer with components distributed as payloads on a mobile science
platform and stationary lander. The rover will carry an infrared diode
laser source and laser radiation detector. The lander will be fitted with
a passive retroreflector that reflects laser radiation from the source
back to the detector. The instrument will determine the presence and
concentration of biogenic gases in the laser beam between diode laser and
retroreflector. Autonomous mobility, navigation, and instrument control
technology will enable directed wide-area surveys.
Commercial rifle scope coupled with photodiode detector. |
Laser beam striking retroreflective material |
Diagram of scope mounting apparatus. |
Near Infrared Oxygen Laser |
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Home Ed Wilson Hybrid Rocket Motors Mars Spectrometer Atmospheric Kinetics USLI
Contact Group Leader Dr. Ed
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