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Saturn’s Moons. Lecture 24. Saturn’s Moons. 62 Moons, 53 named (18 above). Mostly icy, some with rocky cores. Titan is the 2 nd largest moon in our Solar System & only one with a “real” atmosphere with N 2 , CH 4 , CO 2 (1.5 bar!) 98% of N 2 : (N 2 =77% at Earth) No appreciable O 2. - PowerPoint PPT Presentation
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Saturn’s Moons
Lecture 24
Saturn’s Moons
62 Moons, 53 named (18 above). Mostly icy, some with rocky cores. Titan is the 2nd largest moon in our Solar System & only one with a “real”
atmosphere with N2, CH4, CO2 (1.5 bar!) 98% of N2 : (N2=77% at Earth) No appreciable O2
Titan, the Masked!Voyager 2 image of Titan
sunlight 1/100 of Earth -180°C
A lot of organic moleculesCH4, C2H2, C2H6, C3H8, …, argon, CO2, etc.
Always covered with thick haze/smog
Cassini/Huygens in 2004+
Cassini + Huygens (2004- )
Titan’s landscape from Huygens descending image…
looks like a dry streambed!Water ice as rocks…
Interior of Titan
Satellite gravity measurement…
Similar to Callisto, Titan’s interior is not differentiated!
It has a subsurface ocean at very low temperature mixture of water and ammonia
Controversial… : some believe that it should have a rocky core + icy mantle…
A lot of NH3 !
Titan’s Atmosphere
Multi-layer of haze Titan once was believed to be the largest moon in the solar system because of its extended
haze layer (~200 km). Titan’s solid surface is only 60km smaller than Ganymede… NH3 + CH4 + solar UV photons organic molecules… Drizzle of methane and ethane. Possible lakes/oceans of methane
Liquid FlowMethane river A feature most likely
formed by a liquid methane flow. Taken by Huygens probe.
Theoretical models predict that a single methane rainstorm can produce several inches of rain…
Methane World
Cassini pictures of Saturn's moon Titan taken in 2004 and 2005 show that a large methane lake suddenly appeared after what looked like a heavy rainstorm
Sea of Methane on Titan
A Cassini radar image juxtaposed with an image of the Lake Superior
Lots of Natural Gases, but no Oxygen to burn with! Temperature range for liquid:
water: 0 to 100C, methane: -182C to -164C, ethane: -183C to -89C
Possible ethane world?
Origin of Atmosphere Image of Titan taken from Cassini orbiter
10 times more extended than Earth’s
Key factor size (gravity)
How does Titan have an atmosphere when even a larger moon Ganymede doesn’t?
1. distance from the Sun2. effect of their host
planets
• Ganymede does not have an atmosphere at Jupiter’s distance, only water ice could condense…, but at Saturn’s distance, ices such as methane and ammonia could condense!
• Due to the stronger gravity of Jupiter, impacts were generally stronger at Jupiter’s moons than Saturn’s moon. Stronger impacts more easily blew away atmospheres…
More surface feature : Sand Dunes
Windblown dunes Namib desert from Space Shuttle
Titan : summary Very similar features with very different composition and temperature!
A lot of liquid hydrocarbons!about 200°C colder than liquid water much slower chemical reaction slower
metabolism A lot of organic material (e.g., organic sand dunes!) Possible life in the upper atmosphere (acetylene [C2H2] based) or in the subsurface
liquid ocean!
Earth Titan
liquid water liquid methane
silicate rocks water ice rocks
molten lava volcano ice/slush volcano
silicate sand dunes organic particulate dunes
Mimas
Enceladus
Active Enceladus Ice geysers subsurface liquid water + ammonia mixture
Although we expect some tidal heating, it is hard to explain all these activities.
possible subsurface habitable zone!
Tiger stripes = fresh ices cracks or grooves
6th largest moon of Saturn
Enceladus
Tethys
Dione
Rhea
Iapetus
Iapetus : An Intelligence Test for Earthlings?
3rd largest moon of Saturn
Strange Surface
Heavily terraformed?
Equatorial bulge (how???)
Iapetus = Alien’s Starship?
?
Iapetus Deathstar!
In summary…
Important ConceptsTitan:• thick atmosphere• origin of the atmosphere• methane world• similarities and dissimilarities
compared to EarthOther moons of Saturn: What’s
special about these?• Enceladus• Iapetus
Important TermsIce geysers
Chapter/sections covered in this lecture : sections 13-8 through 13-10