The Moons of the Gas Giants Astronomy 311 Professor Lee Carkner Lecture 20.
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Transcript of The Moons of the Gas Giants Astronomy 311 Professor Lee Carkner Lecture 20.
The Group of Seven There are seven large (diameter >2000
km) satellites in the solar system
Each is a distinct world of its own
Jupiter’s Lovers
Io, Europa and Callisto were Jupiter’s lovers in Greek mythology
Saturn was the
king of the Titans
The Galilean Moons
Discovered by Galileo in 1610 Studied by Voyager 1 and 2, HST
and Galileo (the spacecraft)
Orbits of the Galilean Moons
All are tidally locked to Jupiter in a 1-to-1 ratio 1
The periods of the orbits of the 3 inner moons are in a 1:2:4 ratio
Formation of the Galilean Moons
The inner parts of the nebula were hotter than the outer
The inner 3 satellites experienced tidal heating and differentiated into a rocky core and an icy crust
Galileo Visits the Galilean Moons
The Galileo spacecraft arrived at Jupiter in 1995 and has been studying the moons from Jupiter orbit ever since
Io Io is the most volcanically active world in the
solar system These changing forces squeeze and flex Io
producing heat The interior heat has also produced a
differentiated interior
Volcanism on Io Io has no impact craters
Volcanoes produce plumes of
material that extend up to 280 km above the surface
Volcanoes can be very long lived
Io’s Plasma Torus Io’s volcanoes put lots of ions into
its orbit
The ions are effected by Jupiter’s magnetic field producing a plasma torus
Europa Europa’s surface is covered with a
layer of ice Water flows up to the top continually
resurfacing Europa
Tidal flex may also crack the surface
Evidence for Warm Oceans on Europa
Europa has ice rafts where the surface has been broken up and reassembled
Europa also has smooth areas where water has
flowed up and re-frozen Galileo magnetometer measurements indicate
that Europa has a variable magnetic field
Ganymede Ganymede is the largest moon in the solar
system
Ganymede should have little tidal heating due to its distance from Jupiter
Ganymede must have had more geological activity in the past
The Surface of Ganymede
Ganymede shows 2 types of surface features Old dark terrain
New bright terrain
Callisto Callisto is the most distant Galilean moon
from Jupiter It has experienced the least tidal heating
Callisto shows few signs of interior or
surface activity Large impact basin Valhalla
Titan The second largest moon in the
solar system
Only moon with an atmosphere Why does Titan have an
atmosphere?
Titan’s Atmosphere Titan has a thicker atmosphere than the
Earth
Titan’s atmosphere may have originally been composed of ammonia (NH3) and methane (CH4)
90% of the atmosphere is N2
Chemicals in Titan’s Atmosphere Titan’s atmosphere also contains hydrocarbons
(composed of H and C) and polymers (long chains of H, N and C)
Titan may have the necessary organic material to form the building blocks of life
Triton Triton is in a decaying, highly inclined (23
degrees), retrograde orbit
Triton shows evidence of geologic activity
When Triton was first captured it was probably in a highly eccentric orbit which resulted in tidal heating
Triton’s Atmosphere
Triton has a very thin nitrogen atmosphere (1.6 X 10-5 atmospheres of pressure)
A little bit of nitrogen evaporates to
produce the atmosphere
Summary The six large moons of the gas giants resemble
the terrestrial planets of the inner solar system They can have volcanoes, atmospheres, and
evidence of resurfacing In general they are cold and have rocky
interiors and icy exteriors Some produce internal energy through tidal
heating Europa and Titan may possibly have the
conditions for life to exist
Summary: Io and Europa
Io Strong tidal heating produces massive volcanism Volcanism produces powerful outgassed plumes,
sulfurous surface and plasma torus of ions Europa
Icy surface shows evidence for water flowing up from interior
May have a warm subsurface ocean due to tidal heating
Summary: Ganymede and Callisto
Ganymede Shows both old dark terrain and bright new
terrain Must have had more internal heat to drive
geologic activity in the past Callisto
No tidal heating results in no differentiation Fairly uniform mixture of icy and rock with
many craters