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Jovian Planets: Composition, Interiors, Atmospheres, and Moons - Prof. Robert O. Wallace, Study notes of Astronomy

The jovian planets, their composition, interiors, atmospheres, and moons. It covers topics such as the differences in planet composition, size, density, and weather patterns. The document also discusses the presence of magnetospheres and the geological activity of moons. Students will gain a better understanding of the unique features of each jovian planet.

Typology: Study notes

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Uploaded on 08/18/2009

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Chapter 11
Jovian Planet Systems
11.1 A Different Kind of Planet
Our goals for learning:
Are jovian planets all alike?
What are jovian planets like on the inside?
What is the weather like on jovian planets?
Do jovian planets have magnetospheres like
Earth’s?
Are jovian planets all alike?
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Chapter 11

Jovian Planet Systems

11.1 A Different Kind of Planet

Our goals for learning:

  • Are jovian planets all alike?
  • What are jovian planets like on the inside?
  • What is the weather like on jovian planets?
  • Do jovian planets have magnetospheres like

Earth’s?

Are jovian planets all alike?

Jovian Planet Composition

  • Jupiter and Saturn
    • Mostly H and He gas
  • Uranus and Neptune
    • Mostly hydrogen compounds: water (H 2 O), methane (CH 4 ), ammonia (NH 3 )
    • Some H, He, and rock

Density Differences

  • Uranus and Neptune are denser than Saturn because they have less (^0) H/He, proportionately

Jupiter^ SaturnUranus Neptune

Density (g/cc)

Density Differences

Jupiter^ SaturnUranus Neptune

Density (g/cc)

  • But that explanation doesn’t work for Jupiter….

What are jovian planets like on

the inside?

Interiors of Jovian Planets

  • No solid surface.
  • Layers under high pressure and

temperatures.

  • Cores (~10 Earth masses) made of hydrogen

compounds, metals & rock

  • The layers are different for the different

planets. WHY?

Inside Jupiter

  • High pressures inside Jupiter cause phase of hydrogen to change with depth
  • Hydrogen acts like a metal at great depths because its electrons move freely

Inside Jupiter

  • Core is thought to be made of rock, metals, and hydrogen compounds
  • Core is about same size as Earth but 10 times as massive

Comparing Jovian Interiors

  • Models suggest cores of jovian planets have similar composition
  • Lower pressures inside Uranus and Neptune mean no metallic hydrogen

Jupiter’s Internal Heat

  • Jupiter radiates twice as much energy it receives from Sun
  • Energy probably comes from slow contraction of interior (releasing potential energy)

Jovian Planet Atmospheres

  • Other jovian planets have cloud layers similar to Jupiter’s
  • Different compounds make clouds of different colors

Jupiter’s

colors

  • Ammonium sulfide clouds (NH 4 SH) reflect red/brown.
  • Ammonia, the highest, coldest layer, reflects white.

Saturn’s

colors

  • Saturn’s layers are similar, but deeper in and farther from the Sun --- more subdued.

Methane on Uranus and Neptune

  • Methane gas of Neptune and Uranus absorb red light but transmit blue light
  • Blue light reflects off methane clouds, making those planes look blue

Jupiter’s Bands

White ammonia clouds form where air rises

Coriolis effect changes N-S flow to E-W winds Between white clouds we see deeper reddish clouds of NH 4 SH

Warmer red bands are brighter in IR

Jupiter’s

Great

Red

Spot

  • A storm twice as wide as Earth
  • Has existed for at least 3 centuries

Other Magnetospheres

  • All the jovian planets have substantial magnetospheres, but Jupiter’s is largest by far

Thought Question

Jupiter does not have a large metal core like the

Earth. How can it have a magnetic field?

a) The magnetic field is left over from when Jupiter accreted b) Its magnetic field comes from the Sun c) It has metallic hydrogen inside, which circulates and makes a magnetic field d) That’s why its magnetic field is weak

What have we learned?

  • Are jovian planets all alike?
    • Jupiter and Saturn are mostly H and He gas
    • Uranus and Nepture are mostly H compounds
  • What are jovian planets like on the inside?
    • Layered interiors with very high pressure and cores made of rock, metals, and hydrogen compounds
    • Very high pressure in Jupiter and Saturn can produce metallic hydrogen

What have we learned?

  • What is the weather like on jovian planets?
    • Multiple cloud layers determine colors of jovian planets
    • All have strong storms and winds
  • Do jovian planets have magnetospheres

like Earth’s?

  • All have substantial magnetospheres
  • Jupiter’s is largest by far

11.2 A Wealth of Worlds: Satellites of

Ice and Rock

Our goals for learning:

  • What kinds of moons orbit jovian planets?
  • Why are Jupiter’s Galilean moons so

geologically active?

  • What is remarkable about Titan and other

major moons of the outer solar system?

  • Why are small icy moons more geologically

active than small rocky planets?

What kinds of moons orbit the

jovian planets?

Small

Moons

  • Captured asteroids or comets, so orbits do

not follow usual patterns.

Why are Jupiter’s Galilean

moons so geologically active?

Io’s Volcanic Activity

  • Io is the most volcanically active body in the

solar system, but why?

Io’s Volcanoes

  • Volcanic eruptions continue to change Io’s surface

Tidal Heating

Io is squished and

stretched as it orbits

Jupiter But why is its

orbit so

elliptical?

Orbital

Resonances

Every 7 days,

these 3 moons

line up.

The tugs add up over

time, making all 3

orbits elliptical.

Ganymede

  • Largest moon in the

solar system

  • Clear evidence of

geological activity

  • Tidal heating plus

heat from radio-

active decay?

Callisto

  • “Classic” cratered

iceball.

  • No tidal heating,

no orbital

resonances.

  • But it has

magnetic field !?

Thought Question

How does Io get heated by Jupiter?

a) Auroras b) Infrared Light c) Jupiter pulls harder on one side than the other d) Volcanoes

What is remarkable about Titan

and other major moons of the

outer solar system?

Titan’s Atmosphere

  • Titan is the only moon in the solar system to have a thick atmosphere
  • It consists mostly of nitrogen with some argon, methane, and ethane

Titan’s Surface

  • Huygens probe provided first look at Titan’s surface in early 2005
  • Liquid methane, “rocks” made of ice

Why are small icy moons more

geologically active than small

rocky planets?

Rocky Planets vs. Icy Moons

  • Rock melts at higher temperatures
  • Only large rocky planets have enough heat for activity - Ice melts at lower temperatures - Tidal heating can melt internal ice, driving activity

What have we learned?

  • What kinds of moons orbit jovian planets?
    • Moons of many sizes
    • Level of geological activity depends on size
  • Why are Jupiter’s Galilean moons so

geologically active?

  • Tidal heating drives activity, leading to Io’s volcanoes and ice geology on other moons

What have we learned?

  • What is special about Titan and other major moons of the solar system? - Titan is only moon with thick atmosphere - Many other major moons show signs of geological activity
  • Why are small icy moons more geologically active than small rocky planets? - Ice melts and deforms at lower temperatures enabling tidal heating to drive activity

11.3 Jovian Planet Rings

Our goals for learning:

  • What are Saturn’s rings like?
  • How do other jovian ring systems compare

to Saturn’s?

  • Why do the jovian planets have rings?

What are Saturn’s rings like?