Chapter 11

 

 

The Jovian Worlds

 

The visitors

Pioneer 10, 11; Voyager 1,2 Galileo [1995]; Cassini [2004]

 

Completely different chemical composition than terrestrials. They are  H and He

 

Interiors

         Core, liquid, deep gas atmosphere

         Rotation rates measured by magnetospheres – interior rotation

         Oblateness (Saturn ~ 10%)

         Internal energy source

                 Jupiter’s 2x solar irradiation contraction

                 Saturn’s 2x  differentiation He

                 Uranus none

                 Neptune  some, but why?

 

Mass vs. radius  Jupiter is about as large as you get

         Saturn is less dense, but Uranus and Neptune are not  Why?

 

Atmospheres

 

H and He

CH4, NH3, H2O and other H compounds

[Jupiter movie]

Jupiter et al. structure  from Galileo probe

Zones and belts circulation pattern

Coriolis gives storms including the Great Red Spot, [movie] storms

Colors from impurities

         Saturn is ‘paler  storms Deeper and cooler atmosphere than Jupiter 

         Uranus and Neptune cold enough for methane ice clouds = blue  [Neptune movie]

         Seasons affects Uranian atmosphere

 

Magnetospheres

 

Jupiter has the largest 

         Aurora

         Io’s influence

 

The others field and magnetosphere

Saturn’s aurora

Source for Jupiter and Saturn is the metallic H layer

For Uranus and Neptune the ‘water’ layer

 

Satellites

 

Some of them  Jupiter  Saturn Uranus Neptune

Lots of small stuff – but who’s counting?

Dividing them by size helps understand them

0-300km; 300-1500km [spherical]; over 1500km [almost planets]

The big seven: Io, Europa, Ganymede, Callisto, Titan, Triton (Moon)

 

Ice geology

Weaker than rock and can melt but less radioactivity

Larger objects: rocky cores with ice mantle

Ice is dirty

The usual: impact, vulcanism, tectonic not much erosion, if any

 

The Galilean Satellites

Io globe, [movie] vulcanism, hot spots

         Tidal heating  orbital resonance

Europa globe tectonic cracks  hot spots subsurface oceans(?) life?

Ganymede  globe  grooves  ice plates  small magnetic field

Callisto  globe  craters not differentiated, black dust?

 

Titan  Huygens probe 2005   landing

Atmosphere cloud covered  layers  model

Surface

Interior under crust liquid ammonia/water mixture

Impact basin  Crater

Methane channels  from methane rain

frozen lakes   

Why does Titan have an atmosphere and Ganymede does not?

 

Triton polar cap,  [movie] cantaloupe terrain, thin atmosphere

 

Some medium sized

Mimas, Enceladus, Thethys, Dione, Rhea, Iapetus

Miranda, Ariel, Umbriel, Titania, Oberon

 

 

Just being average doesn't make you less interesting

Enceladus with geysers of water

Iapetus strange color and shape

 

Small moons

Asteroid-like, or fragments

 

Rocky different than icy

 

Rings

 

Saturn system  

 

The forces that shape rings

         The planet’s gravity (Kepler)

         Planet’s oblateness  causes flatness

Thin rings and shepherd satellites

Gaps due to resonances  and gap moons

ripples  and more ripples due to gravity of gap moons

Smaller yet - evidence of 'propeller' moons

 

Composition

Dust(icy) and larger, seen by how it scatters light  Dust in gaps

 

Other Rings

Jupiter, Uranus, Neptune

 

Origin

         Tidal disruption of large moons and leftovers not popular theories any more

         Best guess: Chipping away of small moons