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Europa and Titan Life in the Outer Solar System

Europa and Titan Life in the Outer Solar System

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Europa and Titan Life in the Outer Solar System. How does life begin?. The general idea for chemical evolution is: Organic matter + Liquid water + Energy = Life…Maybe. When looking for life…. Follow the Water. This is Europa. Sixth moon of Jupiter - PowerPoint PPT Presentation

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Page 1: Europa and Titan Life in the Outer Solar System

Europa and TitanLife in the Outer Solar System

Page 2: Europa and Titan Life in the Outer Solar System

How does life begin?The general idea for chemical evolution is:Organic matter + Liquid water + Energy

= Life…Maybe

Page 3: Europa and Titan Life in the Outer Solar System

When looking for life…

Follow the Water

Page 4: Europa and Titan Life in the Outer Solar System

This is Europa• Sixth moon of Jupiter• 3,100 km in diameter (slightly smaller than our moon)

Page 5: Europa and Titan Life in the Outer Solar System

Why Europa?Possible ocean below the icy surfacePossibility of hydrothermal vents (energy)OrganicsConditions on Europa could have fostered

life at one time

Page 6: Europa and Titan Life in the Outer Solar System

Galileo SpacecraftLaunched in 1989 Ended in 2003Jupiter MissionMagnetic data provided evidence that Europa

may have a salt water ocean.

Page 7: Europa and Titan Life in the Outer Solar System

Europa Surface

Page 8: Europa and Titan Life in the Outer Solar System

This is Titan•Largest moon of Saturn•About 80% more massive than our moon

Page 9: Europa and Titan Life in the Outer Solar System

Why Titan?Possibility of liquid waterDense atmosphereOrganicsMethane or Ethane Lakes

Page 10: Europa and Titan Life in the Outer Solar System

How will we find out?Europa

Hyrdrobot/CryobotNASA-JIMO (Jupiter Icy Moons Orbiter)

TitanCassini-Huygens Mission

Page 11: Europa and Titan Life in the Outer Solar System

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

Page 12: Europa and Titan Life in the Outer Solar System

Hydrobot/Cryobot

Page 13: Europa and Titan Life in the Outer Solar System

What will we look for?Cassini-Huygens :

Cassini: Saturn OrbiterHuygens: Titan ProbeObserve the surface

Volcanoes, lakes, seasWaterOrganic profiles

Page 14: Europa and Titan Life in the Outer Solar System

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

Page 15: Europa and Titan Life in the Outer Solar System
Page 16: Europa and Titan Life in the Outer Solar System
Page 17: Europa and Titan Life in the Outer Solar System

Titan Sand Dunes

Earth Sand Dunes

Page 18: Europa and Titan Life in the Outer Solar System

Methane and/or Ethane Lakes

Page 19: Europa and Titan Life in the Outer Solar System

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

Page 20: Europa and Titan Life in the Outer Solar System

Ontario Lacus•Contains Ethane•Determined by Spectroscopy

Page 21: Europa and Titan Life in the Outer Solar System

IssuesOceans on Europa are still theoreticalDirect investigation of ocean’s could lead

to contaminationTitan is very cold (94 K), and unlikely to

support life