Infrared Detection of Evidence for Microscopic Organisms on Europa

Biology – Quantitative Biology – Biomolecules

Scientific paper

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5410 Composition, 5464 Remote Sensing, 5470 Surface Materials And Properties, 6020 Ice, 6218 Jovian Satellites

Scientific paper

The infrared detection of evidence for microorganisms on surfaces of icy satellites requires four conditions: (1) the emplacement of microorganisms at the surface, (2) the survival of biotic material in the hostile conditions of space, (3) that the biotic material exhibit diagnostic infrared absorption features and (4) spectra with sufficient resolution and signal-to-noise ratios. This paper will focus on each topic with respect to cryogenic data recently collected on model microorganisms. Several studies suggest that materials from a Europan interior ocean have been emplaced in disrupted regions[1-10]. If the Europan ocean at one time contained Life and its associated biomolecules, then it is possible that surface materials may still harbor some remnant of these structures. Such remnant material must be capable of surviving the low pressure, low temperature and high radiation environment. The terrestrial extremophile Deinococcus radiodurans has been found viable after exposure both to vacuum at temperatures as low as 80 K [11] and to 60 Gy/h of radiation[12]. The chemical degradation of D. radiodurans has also been shown to be dependent on plasma composition (O2 {>>} CO2)[13]. Hence, it is reasonable to assume that some degree of sterilization and degradation would be occurring at the surface of Europa. However, given the sputtering rate at Europa of approximately a few cm every few million years [14], it is possible that fresh material may be continually exposed from depths to which little radiation penetrates. Remote sensing of the surface, therefore, would not be dependent on the survival of the microorganism but on the endurance of the particular biomolecules that give rise to the spectral signature. This endurance is not unreasonable since previous studies have detected hydrated salts, which contain labile bonds to water, on Europa [3,15]. Cryogenic reflectance spectra of hydrated sulfate salts have broad (150-300 nm), asymmetric absorption features due to bound water of hydration, as well as narrow features on the order of 10 to 20 nm. Cryogenic reflectance spectra of D. radiodurans are similarly dominated by asymmetric, water-related absorption features but also have two sharp (5-10 nm) features arising from amide bonds within the cells. These amide bonds are two orders of magnitude stronger than the hydration bonds in the salts [16]. Thus, the features arising from the amides could be exploited for remote-sensing investigations. In comparison, the Europa spectra from Galileo NIMS also contain the broad, asymmetric absorption features attributed to water and several other weaker absorptions. Together, the narrow features are suggestive of a mixture of materials. The NIMS data are consistent with the presence of water ice, with up to 50% sulfuric acid octahydrate, 20-45% hydrated salts, and possibly as much as 0.2 mg /cm3 carbonaceous material which may be of biological origin. However, inherent noise in the observations and limitations of spectral resolution must be taken into account when discussing these findings. References:[1]Greenberg et al.,Icarus 141,1999. [2]Pappalardo et al., JGR 104, 1999. [3]McCord et al., Science 280, 1998. [4]McCord et al., LPSC XXX,1508,1999a.[5]McCord et al., LPSC XXX,1510,1999b.[6]McCord et al., JGR 104,1999c. [7]McCord et al., DPS 31,1171,1999d.[8]McCordet al., JGR 104,1999e.[9]McCord et al., JGR 106,2001.[10]McCord et al.,JGR 107,E1-4,2002.[11]Dalton et al., NAI AstroBiol. Sci. Con. 2,2002.[12]Ventkataswaran et al., Appl Environ Microbiol. 66, 2000.[13]Mogul et al., PNAS, subm., 2002.[14]Cooper et al., Icarus 149, 2000.[15]Dalton, PhD Diss., U. Colorado,Boulder,2000.[16]Darwent, Nat. Bur. Stand., NSRDS-NBS 31,1970.

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