HR: 11:40h
AN: P11C-06 INVITED [PDF]
TI: A Search for Signs of Life and Habitability on Europa
AU: * McKay, C P
EM: cmckay@mail.arc.nasa.gov
AF: NASA Ames Research Center, Space Science Division, Moffett Field, CA 94035 United States
AU: Eicken, H
EM: hajo.eicken@gi.alaska.edu
AF: University of Alaska, 903 Koyukuk Dr., P.O. Box 757320, Fairbanks, AK 99775 United States
AU: Neuer, S
EM: susanne.neuer@asu.edu
AF: Arizona State University, School of Life Sciences, Tempe, AZ 85287 United States
AU: Sogin, M
EM: sogin@mbl.edu
AF: Marine Biology Laboratory, Woods Hole, Wood Hole, MA 02543 United States
AU: Waite, H
EM: hunterw@umich.edu
AF: University of Michigan, Space Research Building, Ann Arbor, MI 48109 United States
AU: Warmflash, D
EM: david.m.warmflash1@jsc.nasa.gov
AF: NASA Johnson Space Center, Space Science Division, Houston, TX 77058 United States
AB:
Europa is a key target in the search for life beyond the Earth because of consistent evidence that below the icy surface
there is liquid water. Future missions to Europa could confirm the presence and nature of the ocean and determine the
thickness of the ice layer. Confirming the presence of an ocean and determining the habitability of Europa are key
astrobiology science objectives. Nevertheless, the highest priority objective for astrobiology will be a search for life.
How could a search for life be accomplished on a near-term mission given the thick ice cover? One answer may lie in the
surface materials. If Europa has an ocean, and if that ocean contains life, and if water from the ocean is carried up to the
surface, then signs of life may be contained in organic material on the surface. Organics that derive from biological
processes (dead organisms) are distinct from organics derived from non-biological processes in several aspects. First,
biology is selective and specific in its use of molecules. For example, Earth life uses 20 left-handed amino acids. Second,
biology can leave characteristic isotopic patterns. Third, biology often produces large complex molecules in high
concentrations, for example lipids. Organic material that has been on the surface of Europa for long periods of time would be
reprocessed by the strong radiation field probably erasing any signature of biological origin. Evidence of life in the ocean
may be found on the surface of Europa if regions of the surface contained relatively recent material carried up from the
ocean through cracks in the icy lithosphere. But organic material that has been on the surface of Europa for long periods of
time would be reprocessed by the strong radiation field probably erasing any signature of biological origin. Thus, the
detailed analysis required may not be possible via remote sensing but direct sampling of the material below the radiation
processed upper meter is probably required.
DE: 5700 PLANETOLOGY: FLUID PLANETS
DE: 5709 Composition
DE: 6040 Origin and evolution
DE: 6218 Jovian satellites
SC: Planetary Sciences [P]
MN: 2003 Fall Meeting