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How does life begin?The general idea for chemical evolution is:Organic matter + Liquid water + Energy
= Life…Maybe
Why Europa?Possible ocean below the icy surfacePossibility of hydrothermal vents (energy)OrganicsConditions on Europa could have fostered
life at one time
Galileo SpacecraftLaunched in 1989 Ended in 2003Jupiter MissionMagnetic data provided evidence that Europa
may have a salt water ocean.
How will we find out?Europa
Hyrdrobot/CryobotNASA-JIMO (Jupiter Icy Moons Orbiter)
TitanCassini-Huygens Mission
What will we look for?Hydrobot/Cryobot (Proposed, not planned)
Drill through ice crustRelease “Hyrdobot” into hypothetical oceanSearch for hydrothermal vents and micro-
organismsNASA-JIMO (Canceled in 2005)
Orbit Europa and map the planetLook for signatures of life
ESA’s Europa Jupiter System Mission?We’ll know in 2013
What will we look for?Cassini-Huygens :
Cassini: Saturn OrbiterHuygens: Titan ProbeObserve the surface
Volcanoes, lakes, seasWaterOrganic profiles
Cassini-HuygensLaunched in 1997Cassini still functioning Huygens probe landed on Titan in 2005Found: Methane and/or Ethane LakesHydrocarbon Sand DunesPossibility of internal liquid water-ammonia
ocean
Methane and/or Ethane LakesTheorized that dark areas were liquidCassini’s radar beams were reflected which
usually indicates liquidsAt 94K, liquids were mostly likely to be
methane and/or ethaneTitan’s atmosphere contains methane