Near-infrared detection of potential evidence for microscopic organisms on Europa.
The possibility of an ocean within the icy shell of Jupiter's moon Europa has established that world as a primary candidate in the search for extraterrestrial life within our Solar System. This paper evaluates the potential to detect evidence for microbial life by comparing laboratory studies of terrestrial microorganisms with measurements from the Galileo Near Infrared Imaging Spectrometer (NIMS). If the interior of Europa at one time harbored life, some evidence may remain in the surface materials. Examination of laboratory spectra of terrestrial extremophiles measured at cryogenic temperatures reveals distorted, asymmetric nearinfrared absorption features due to water of hydration. The band centers, widths, and shapes of these features closely match those observed in the Europa spectra. These features are strongest in reddish-brown, disrupted terrains such as linea and chaos regions. Narrow spectral features due to amide bonds in the microbe proteins provide a means of constraining the abundances of such materials using the NIMS data. The NIMS data of disrupted terrains exhibit distorted, asymmetric near-infrared absorption features consistent with the presence of water ice, sulfuric acid octahydrate, hydrated salts, and possibly as much as 0.2 mg cm(-3) of carbonaceous material that could be of biological origin. However, inherent noise in the observations and limitations of spectral sampling must be taken into account when discussing these findings.
Dalton
J Brad
JB
SETI Institute, NASA Ames Research Center, Mountain View, Moffitt Field, California 94035-1000, USA. dalton@mail.arc.nasa.gov
Mogul
Rakesh
R
Kagawa
Hiromi K
HK
Chan
Suzanne L
SL
Jamieson
Corey S
CS
D005118:Extraterrestrial Environment; D005615:Freezing; D018538:Jupiter; D019369:Life; D013055:Spectrophotometry, Infrared / Q000295:instrumentation* / Q000379:methods