Jupiter (Galileo)Saturn (Cassini) Uranus (Hubble)Neptune (Voyager)
© 2005 Pearson Education Inc., publishing as Addison-Wesley Giant Planets Jupiter Saturn Uranus...
-
date post
19-Dec-2015 -
Category
Documents
-
view
215 -
download
0
Transcript of © 2005 Pearson Education Inc., publishing as Addison-Wesley Giant Planets Jupiter Saturn Uranus...
![Page 1: © 2005 Pearson Education Inc., publishing as Addison-Wesley Giant Planets Jupiter Saturn Uranus Neptune.](https://reader030.fdocuments.us/reader030/viewer/2022032704/56649d3a5503460f94a14e40/html5/thumbnails/1.jpg)
© 2005 Pearson Education Inc., publishing as Addison-Wesley
Giant PlanetsGiant Planets
Jupiter
QuickTime™ and aTIFF (Uncompressed) decompressor
are needed to see this picture.
Saturn
Uranus
Neptune
![Page 2: © 2005 Pearson Education Inc., publishing as Addison-Wesley Giant Planets Jupiter Saturn Uranus Neptune.](https://reader030.fdocuments.us/reader030/viewer/2022032704/56649d3a5503460f94a14e40/html5/thumbnails/2.jpg)
© 2005 Pearson Education Inc., publishing as Addison-Wesley
Important Notes:Important Notes:
• Read Chapter 11: “Jovian Planet Systems”Read Chapter 11: “Jovian Planet Systems”• Homework #8 due Friday Homework #8 due Friday
(on today’s and Thursday’s lecture)(on today’s and Thursday’s lecture)• MarsMars: Mark mid-semester position!: Mark mid-semester position!
• Midterm #2: Tuesday, April 15Midterm #2: Tuesday, April 15
![Page 3: © 2005 Pearson Education Inc., publishing as Addison-Wesley Giant Planets Jupiter Saturn Uranus Neptune.](https://reader030.fdocuments.us/reader030/viewer/2022032704/56649d3a5503460f94a14e40/html5/thumbnails/3.jpg)
© 2005 Pearson Education Inc., publishing as Addison-Wesley
The Solar SystemThe Solar SystemTerrestrial (Rocky) Outer 4 Planets: Gaseous Giants
![Page 4: © 2005 Pearson Education Inc., publishing as Addison-Wesley Giant Planets Jupiter Saturn Uranus Neptune.](https://reader030.fdocuments.us/reader030/viewer/2022032704/56649d3a5503460f94a14e40/html5/thumbnails/4.jpg)
© 2005 Pearson Education Inc., publishing as Addison-Wesley
The 4 “Giant Planets”The 4 “Giant Planets”“Jovian Planets”:“Jovian Planets”:
QuickTime™ and aTIFF (Uncompressed) decompressor
are needed to see this picture.
Much higher mass & radius than Earth, Venus, Mars.• No solid surfaces !!!
QuickTime™ and aTIFF (Uncompressed) decompressor
are needed to see this picture. H & He
(most common atoms in universe)
(text: “hydrogen compounds” = water, methane, ammonia)
“Ice Giants”
Jupiter Saturn Uranus Neptune
All have Rock Cores: 10-15 Earth-Masses
H & He H2O,
H & He
H2O,
H & He
![Page 5: © 2005 Pearson Education Inc., publishing as Addison-Wesley Giant Planets Jupiter Saturn Uranus Neptune.](https://reader030.fdocuments.us/reader030/viewer/2022032704/56649d3a5503460f94a14e40/html5/thumbnails/5.jpg)
© 2005 Pearson Education Inc., publishing as Addison-Wesley
Jupiter’s Moon: Io
• A volcanic explosion can be seen silhouetted against dark space over Io's brilliant limb. Io more volcanically active than Earth.
QuickTime™ and aTIFF (Uncompressed) decompressor
are needed to see this picture.
Next Lecture:Next Lecture:
Moons orbiting the Giant PlanetsMoons orbiting the Giant Planets
![Page 6: © 2005 Pearson Education Inc., publishing as Addison-Wesley Giant Planets Jupiter Saturn Uranus Neptune.](https://reader030.fdocuments.us/reader030/viewer/2022032704/56649d3a5503460f94a14e40/html5/thumbnails/6.jpg)
© 2005 Pearson Education Inc., publishing as Addison-Wesley
Jupiter – King of the PlanetsJupiter – King of the PlanetsMass = 0.001 solar (318 earths), Radius = 11.2 Earths, Density = 1.3 g/cc (1.3 x water)
Distance: 5.2AUOrbital Period: 11.8 years Rotation period: 9.9 hours.
Flattened Spheroid
![Page 7: © 2005 Pearson Education Inc., publishing as Addison-Wesley Giant Planets Jupiter Saturn Uranus Neptune.](https://reader030.fdocuments.us/reader030/viewer/2022032704/56649d3a5503460f94a14e40/html5/thumbnails/7.jpg)
© 2005 Pearson Education Inc., publishing as Addison-Wesley
SaturnMass = 95 EarthsRadius = 9.4 Earths Density = 0.7 gram/cm3 (floats)Distance: 9.5 AUOrbital Period: 29.4 yearsRotation period: 10.6 hours.
Rings: Composed ofbillions of icy-rocks and icy dust (water and silicates).
![Page 8: © 2005 Pearson Education Inc., publishing as Addison-Wesley Giant Planets Jupiter Saturn Uranus Neptune.](https://reader030.fdocuments.us/reader030/viewer/2022032704/56649d3a5503460f94a14e40/html5/thumbnails/8.jpg)
© 2005 Pearson Education Inc., publishing as Addison-Wesley
UranusUranusMass = 14.5 Earths Orbital Period: 84 years; Radius = 4.0 EarthsDensity = 1.3 gram/cm3 = 1.3 x water Distance: 19.2 AU Rotation period: 17.2 hours.
Visible Light Infrared Light (Thermal Emission)
•Featureless in visible light, because clouds
are below haze layer of methane (colder than Saturn).
![Page 9: © 2005 Pearson Education Inc., publishing as Addison-Wesley Giant Planets Jupiter Saturn Uranus Neptune.](https://reader030.fdocuments.us/reader030/viewer/2022032704/56649d3a5503460f94a14e40/html5/thumbnails/9.jpg)
© 2005 Pearson Education Inc., publishing as Addison-Wesley
NeptuneNeptune
![Page 10: © 2005 Pearson Education Inc., publishing as Addison-Wesley Giant Planets Jupiter Saturn Uranus Neptune.](https://reader030.fdocuments.us/reader030/viewer/2022032704/56649d3a5503460f94a14e40/html5/thumbnails/10.jpg)
© 2005 Pearson Education Inc., publishing as Addison-Wesley
Neptune
Mass = 17 Earths
Radius = 3.9 Earths
Density = 1.76 x water
Distance: 30 AU
Orbital Period: 163 years;
Rotation period: 16.1 hours.
Cyclonic storms.
![Page 11: © 2005 Pearson Education Inc., publishing as Addison-Wesley Giant Planets Jupiter Saturn Uranus Neptune.](https://reader030.fdocuments.us/reader030/viewer/2022032704/56649d3a5503460f94a14e40/html5/thumbnails/11.jpg)
© 2005 Pearson Education Inc., publishing as Addison-Wesley
GIANT PLANETS
![Page 12: © 2005 Pearson Education Inc., publishing as Addison-Wesley Giant Planets Jupiter Saturn Uranus Neptune.](https://reader030.fdocuments.us/reader030/viewer/2022032704/56649d3a5503460f94a14e40/html5/thumbnails/12.jpg)
© 2005 Pearson Education Inc., publishing as Addison-Wesley
Spacecraft Reconnaisance
QuickTime™ and aTIFF (Uncompressed) decompressor
are needed to see this picture.
QuickTime™ and aTIFF (Uncompressed) decompressor
are needed to see this picture.
QuickTime™ and aTIFF (Uncompressed) decompressor
are needed to see this picture.
1980’s: Voyager 1 & 2
Camera
Spectrometer
Visit all 4
giant planets
Measures spectral lines:
Chemical composition
![Page 13: © 2005 Pearson Education Inc., publishing as Addison-Wesley Giant Planets Jupiter Saturn Uranus Neptune.](https://reader030.fdocuments.us/reader030/viewer/2022032704/56649d3a5503460f94a14e40/html5/thumbnails/13.jpg)
© 2005 Pearson Education Inc., publishing as Addison-Wesley
Spacecraft Reconnaisance;
Galileo Spacecraft
QuickTime™ and aTIFF (Uncompressed) decompressorare needed to see this picture.
QuickTime™ and aTIFF (Uncompressed) decompressor
are needed to see this picture.
QuickTime™ and aTIFF (Uncompressed) decompressor
are needed to see this picture.
QuickTime™ and aTIFF (Uncompressed) decompressor
are needed to see this picture.
•Launched from Space Shuttle 1989
![Page 14: © 2005 Pearson Education Inc., publishing as Addison-Wesley Giant Planets Jupiter Saturn Uranus Neptune.](https://reader030.fdocuments.us/reader030/viewer/2022032704/56649d3a5503460f94a14e40/html5/thumbnails/14.jpg)
© 2005 Pearson Education Inc., publishing as Addison-Wesley
Spacecraft Reconnaisance;
Galileo Spacecraft
QuickTime™ and aTIFF (Uncompressed) decompressor
are needed to see this picture.
QuickTime™ and aTIFF (Uncompressed) decompressor
are needed to see this picture.
Arrived: 1995
2003:Dropped into Jupiter’s
Atmosphere:
Measure Chemical
Composition:
97% hydrogen & helium
Plus 3% C, N, O, S, Si …
![Page 15: © 2005 Pearson Education Inc., publishing as Addison-Wesley Giant Planets Jupiter Saturn Uranus Neptune.](https://reader030.fdocuments.us/reader030/viewer/2022032704/56649d3a5503460f94a14e40/html5/thumbnails/15.jpg)
© 2005 Pearson Education Inc., publishing as Addison-Wesley
C, N, O, HChemistry
Giant Planet’s Chemical CompositionGiant Planet’s Chemical Composition
Mostly Hydrogen and HeliumMostly Hydrogen and Helium
•Add H to:
C, N, O
![Page 16: © 2005 Pearson Education Inc., publishing as Addison-Wesley Giant Planets Jupiter Saturn Uranus Neptune.](https://reader030.fdocuments.us/reader030/viewer/2022032704/56649d3a5503460f94a14e40/html5/thumbnails/16.jpg)
© 2005 Pearson Education Inc., publishing as Addison-Wesley
Why are the Jovian Planets Massive and Gaseous (H, He) ?
• Formed beyond the frost line (3 AU): so cold that ice particles exist with silicate dust.
• Ice and Dust collides, sticks grows into icy-rocky core.• Core’s gravity captures H/He gas• Planet attracts ices and dust that orbit• Moons formed out of these disks: A miniature solar system.
Young Solar System:
Gas & Dust
Young Jupiter
![Page 17: © 2005 Pearson Education Inc., publishing as Addison-Wesley Giant Planets Jupiter Saturn Uranus Neptune.](https://reader030.fdocuments.us/reader030/viewer/2022032704/56649d3a5503460f94a14e40/html5/thumbnails/17.jpg)
© 2005 Pearson Education Inc., publishing as Addison-Wesley
Quiz
If Jupiter formed in a protoplanetary disk that had twice as much dust it:
a) Would have a bigger core
b) Might have more hydrogen
c) Might have more metallic hydrogen
d) All of the above
![Page 18: © 2005 Pearson Education Inc., publishing as Addison-Wesley Giant Planets Jupiter Saturn Uranus Neptune.](https://reader030.fdocuments.us/reader030/viewer/2022032704/56649d3a5503460f94a14e40/html5/thumbnails/18.jpg)
© 2005 Pearson Education Inc., publishing as Addison-Wesley
QuickTime™ and aTIFF (Uncompressed) decompressor
are needed to see this picture.
![Page 19: © 2005 Pearson Education Inc., publishing as Addison-Wesley Giant Planets Jupiter Saturn Uranus Neptune.](https://reader030.fdocuments.us/reader030/viewer/2022032704/56649d3a5503460f94a14e40/html5/thumbnails/19.jpg)
© 2005 Pearson Education Inc., publishing as Addison-Wesley
QuickTime™ and aTIFF (Uncompressed) decompressor
are needed to see this picture.
• Color Enhancement
![Page 20: © 2005 Pearson Education Inc., publishing as Addison-Wesley Giant Planets Jupiter Saturn Uranus Neptune.](https://reader030.fdocuments.us/reader030/viewer/2022032704/56649d3a5503460f94a14e40/html5/thumbnails/20.jpg)
© 2005 Pearson Education Inc., publishing as Addison-Wesley
QuickTime™ and aTIFF (Uncompressed) decompressor
are needed to see this picture.
![Page 21: © 2005 Pearson Education Inc., publishing as Addison-Wesley Giant Planets Jupiter Saturn Uranus Neptune.](https://reader030.fdocuments.us/reader030/viewer/2022032704/56649d3a5503460f94a14e40/html5/thumbnails/21.jpg)
© 2005 Pearson Education Inc., publishing as Addison-Wesley
Hydrostatic Equilibrium: Pressure balanceHydrostatic Equilibrium: Pressure balance
“Hydrostatic equilibrium” governs the structure of all planets. The inside has higher pressure and density because of the weight of the overlying material.
Pressure at any depth = gravitational weight of column above
![Page 22: © 2005 Pearson Education Inc., publishing as Addison-Wesley Giant Planets Jupiter Saturn Uranus Neptune.](https://reader030.fdocuments.us/reader030/viewer/2022032704/56649d3a5503460f94a14e40/html5/thumbnails/22.jpg)
© 2005 Pearson Education Inc., publishing as Addison-Wesley
Inside Jupiter• Jupiter emits almost twice as much energy as it absorbs from the Sun.
• accretion, differentiation, radioactivity can not account for it
• Jupiter must still be contracting
• Jupiter has 3 x more mass than Saturn, but is only slightly larger in radius!• the added weight of H & He compresses the core to a higher density
• like stacking pillows• If Jupiter had 10x its mass,
it would have same radius ! Add even more mass, and Jupiter would get smaller !
• Jupiter is about as large as a planet can get.
• Uranus & Neptune have less mass than Saturn, yet
they have higher densities
• They must be made of denser material:
• Rock & Ice !
![Page 23: © 2005 Pearson Education Inc., publishing as Addison-Wesley Giant Planets Jupiter Saturn Uranus Neptune.](https://reader030.fdocuments.us/reader030/viewer/2022032704/56649d3a5503460f94a14e40/html5/thumbnails/23.jpg)
© 2005 Pearson Education Inc., publishing as Addison-Wesley
Quiz
On the moon, a cup of sugar has some pressure, P, at its bottom. You add 50% more sugar to the cup. The new pressure at the bottom is:
a) 0.5 P
b) 1.0 P
c) 1.5 P
d) 2.0 P
![Page 24: © 2005 Pearson Education Inc., publishing as Addison-Wesley Giant Planets Jupiter Saturn Uranus Neptune.](https://reader030.fdocuments.us/reader030/viewer/2022032704/56649d3a5503460f94a14e40/html5/thumbnails/24.jpg)
© 2005 Pearson Education Inc., publishing as Addison-Wesley
Inside Jupiter
• Moving from the surface to the core:• temperature increases• pressure & density increases
• Hydrogen atoms so dense: Electrons not associated with
any one atom: Free- electrons. Metallic Hydrogen!
• Jupiter's core is rock & ice: ~10 times the mass of Earth.
. . . Controversial.
No solid surface and consists mostly of H & He.Distinct interior layers, defined by increasing density inward.
![Page 25: © 2005 Pearson Education Inc., publishing as Addison-Wesley Giant Planets Jupiter Saturn Uranus Neptune.](https://reader030.fdocuments.us/reader030/viewer/2022032704/56649d3a5503460f94a14e40/html5/thumbnails/25.jpg)
© 2005 Pearson Education Inc., publishing as Addison-Wesley
Inside the Jovian Planets• All Jovian cores appear to be similar.
• made of rock, metal, and Hydrogen compounds• 10 x the mass of Earth
• Uranus & Neptune captured less gas from the Solar nebula.• accretion of planetesimals took longer• not much time for gas capture before nebula was cleared out by Solar wind
• Only Jupiter and Saturn have high enough pressure for H & He to exist in liquid and metallic states.
![Page 26: © 2005 Pearson Education Inc., publishing as Addison-Wesley Giant Planets Jupiter Saturn Uranus Neptune.](https://reader030.fdocuments.us/reader030/viewer/2022032704/56649d3a5503460f94a14e40/html5/thumbnails/26.jpg)
© 2005 Pearson Education Inc., publishing as Addison-Wesley
Centrifugal Force:
Flings material at equator outward
Due to Rotation
Rotational Distortionof Planet’s Shape
![Page 27: © 2005 Pearson Education Inc., publishing as Addison-Wesley Giant Planets Jupiter Saturn Uranus Neptune.](https://reader030.fdocuments.us/reader030/viewer/2022032704/56649d3a5503460f94a14e40/html5/thumbnails/27.jpg)
© 2005 Pearson Education Inc., publishing as Addison-Wesley
Rotation flattens shape—> Less pull on satellite at poles
Higher densitytoward center —> Exerts Point-like Grav. Force
Track acceleration ofTrack acceleration ofsatellites accuratelysatellites accurately
—> Density throughout interiorDensity throughout interior
Determining the Density inside a Rotating PlanetUse Motion of Orbiting Satellites
![Page 28: © 2005 Pearson Education Inc., publishing as Addison-Wesley Giant Planets Jupiter Saturn Uranus Neptune.](https://reader030.fdocuments.us/reader030/viewer/2022032704/56649d3a5503460f94a14e40/html5/thumbnails/28.jpg)
© 2005 Pearson Education Inc., publishing as Addison-Wesley
The Great Red Spot
QuickTime™ and aTIFF (Uncompressed) decompressor
are needed to see this picture.
- Another Effect of Planet’s Rotation -
![Page 29: © 2005 Pearson Education Inc., publishing as Addison-Wesley Giant Planets Jupiter Saturn Uranus Neptune.](https://reader030.fdocuments.us/reader030/viewer/2022032704/56649d3a5503460f94a14e40/html5/thumbnails/29.jpg)
© 2005 Pearson Education Inc., publishing as Addison-Wesley
QuickTime™ and aTIFF (Uncompressed) decompressor
are needed to see this picture.
A Hurricane that has
lasted 300 yearsGreat Red SpotGreat Red Spot
![Page 30: © 2005 Pearson Education Inc., publishing as Addison-Wesley Giant Planets Jupiter Saturn Uranus Neptune.](https://reader030.fdocuments.us/reader030/viewer/2022032704/56649d3a5503460f94a14e40/html5/thumbnails/30.jpg)
© 2005 Pearson Education Inc., publishing as Addison-Wesley
Cyclonic MotionsCyclonic Motions
Coriolis effect: Coriolis effect: Motion fromMotion fromHigh PressureHigh Pressure area area
NorthernNorthernHemisphereHemisphere
SouthernSouthernHemisphereHemisphere
![Page 31: © 2005 Pearson Education Inc., publishing as Addison-Wesley Giant Planets Jupiter Saturn Uranus Neptune.](https://reader030.fdocuments.us/reader030/viewer/2022032704/56649d3a5503460f94a14e40/html5/thumbnails/31.jpg)
© 2005 Pearson Education Inc., publishing as Addison-Wesley
Jovian Storms• Red Spot: A High Pressure Storm
• Analogous to hurricanes, but they rotate in the opposite direction
• Jupiter• the Great Red Spot• we are not sure why it is red
• Neptune• the Great Dark Spot
Planet
Rotation
![Page 32: © 2005 Pearson Education Inc., publishing as Addison-Wesley Giant Planets Jupiter Saturn Uranus Neptune.](https://reader030.fdocuments.us/reader030/viewer/2022032704/56649d3a5503460f94a14e40/html5/thumbnails/32.jpg)
© 2005 Pearson Education Inc., publishing as Addison-Wesley
scooter
Neptune’s
Storms
![Page 33: © 2005 Pearson Education Inc., publishing as Addison-Wesley Giant Planets Jupiter Saturn Uranus Neptune.](https://reader030.fdocuments.us/reader030/viewer/2022032704/56649d3a5503460f94a14e40/html5/thumbnails/33.jpg)
© 2005 Pearson Education Inc., publishing as Addison-Wesley
Quiz
You are standing on the equator of the Earth and you throw a ball fast, directly toward the south pole. The ball’s trajectory will
a) Carry it toward the south pole
b) Veer to the right
c) Veer to the left
d) Curl around in a spiral
![Page 34: © 2005 Pearson Education Inc., publishing as Addison-Wesley Giant Planets Jupiter Saturn Uranus Neptune.](https://reader030.fdocuments.us/reader030/viewer/2022032704/56649d3a5503460f94a14e40/html5/thumbnails/34.jpg)
© 2005 Pearson Education Inc., publishing as Addison-Wesley
Jupiter’s Cloud Layers
• Convection in the troposphere causes Jovian weather.
• Warm gas rises to cooler altitudes, where it condenses to form clouds.
• Three gases condense in the Jovian atmosphere:• ammonia (NH3)
• ammonium hydrosulfide (NH4SH)
• water (H2O)
• They condense at different temperatures, so their clouds form at different altitudes.
Alt
itud
e ab
ove
clou
ds to
ps (
km)
Temperature (C )
![Page 35: © 2005 Pearson Education Inc., publishing as Addison-Wesley Giant Planets Jupiter Saturn Uranus Neptune.](https://reader030.fdocuments.us/reader030/viewer/2022032704/56649d3a5503460f94a14e40/html5/thumbnails/35.jpg)
© 2005 Pearson Education Inc., publishing as Addison-Wesley
The Jovian Atmospheres
• The temperature profile of each planet determines the color of its appearance.
• Cloud layers form where a particular gas condenses.
• Saturn has the same cloud layers as Jupiter.• they form deeper since Saturn is
colder overall
• they are spread farther apart since Saturn has lower gravity
• Uranus & Neptune• cold enough to form methane clouds
![Page 36: © 2005 Pearson Education Inc., publishing as Addison-Wesley Giant Planets Jupiter Saturn Uranus Neptune.](https://reader030.fdocuments.us/reader030/viewer/2022032704/56649d3a5503460f94a14e40/html5/thumbnails/36.jpg)
© 2005 Pearson Education Inc., publishing as Addison-Wesley
Bands of JupiterWhat Causes them?
![Page 37: © 2005 Pearson Education Inc., publishing as Addison-Wesley Giant Planets Jupiter Saturn Uranus Neptune.](https://reader030.fdocuments.us/reader030/viewer/2022032704/56649d3a5503460f94a14e40/html5/thumbnails/37.jpg)
© 2005 Pearson Education Inc., publishing as Addison-Wesley
Convection on Jupiter:
•Warm air rises•Coriolis force
diverts path sideways
Coriolis force is due to
rotation of planet
•Jupiter rotates fast:
Period = 10 hours
![Page 38: © 2005 Pearson Education Inc., publishing as Addison-Wesley Giant Planets Jupiter Saturn Uranus Neptune.](https://reader030.fdocuments.us/reader030/viewer/2022032704/56649d3a5503460f94a14e40/html5/thumbnails/38.jpg)
© 2005 Pearson Education Inc., publishing as Addison-Wesley
Wind Speed in Jupiter’s Bands
•1000 km/hr
![Page 39: © 2005 Pearson Education Inc., publishing as Addison-Wesley Giant Planets Jupiter Saturn Uranus Neptune.](https://reader030.fdocuments.us/reader030/viewer/2022032704/56649d3a5503460f94a14e40/html5/thumbnails/39.jpg)
© 2005 Pearson Education Inc., publishing as Addison-Wesley
Red SpotRed Spotin Southernin SouthernHemisphereHemisphere
Winds of Jupiter’s Bands
![Page 40: © 2005 Pearson Education Inc., publishing as Addison-Wesley Giant Planets Jupiter Saturn Uranus Neptune.](https://reader030.fdocuments.us/reader030/viewer/2022032704/56649d3a5503460f94a14e40/html5/thumbnails/40.jpg)
© 2005 Pearson Education Inc., publishing as Addison-Wesley
Magnetic FieldsJupiter Saturn
Uranus Neptune
![Page 41: © 2005 Pearson Education Inc., publishing as Addison-Wesley Giant Planets Jupiter Saturn Uranus Neptune.](https://reader030.fdocuments.us/reader030/viewer/2022032704/56649d3a5503460f94a14e40/html5/thumbnails/41.jpg)
© 2005 Pearson Education Inc., publishing as Addison-Wesley
Jupiter's Magnetosphere
• Ion and neutral mass spectrometer instrument on the Cassini spacecraft, makes the huge magnetosphere surrounding Jupiter visible. The magnetosphere is a bubble of charged particles trapped within the magnetic environment of the planet. In this picture, a magnetic field is sketched over the image to place the energetic neutral atom emissions in perspective.
• Also shown for scale and location are the disk of Jupiter (black circle) and the approximate position (yellow circles) of the doughnut-shaped torus created from material spewed out by volcanoes on Io, one of Jupiter's large moons.
QuickTime™ and aTIFF (Uncompressed) decompressor
are needed to see this picture.
![Page 42: © 2005 Pearson Education Inc., publishing as Addison-Wesley Giant Planets Jupiter Saturn Uranus Neptune.](https://reader030.fdocuments.us/reader030/viewer/2022032704/56649d3a5503460f94a14e40/html5/thumbnails/42.jpg)
© 2005 Pearson Education Inc., publishing as Addison-Wesley
Jupiter’s Magnetosphere – Bigger than the Sun
Solar Wind
protons &
electrons
![Page 43: © 2005 Pearson Education Inc., publishing as Addison-Wesley Giant Planets Jupiter Saturn Uranus Neptune.](https://reader030.fdocuments.us/reader030/viewer/2022032704/56649d3a5503460f94a14e40/html5/thumbnails/43.jpg)
© 2005 Pearson Education Inc., publishing as Addison-Wesley
Jovian Magnetospheres
• Saturn, Uranus, & Neptune have smaller & weaker magnetospheres.• fraction of electrically conducting material in interiors is smaller
• Solar wind is weaker farther out, or else their magnetospheres would be even smaller
• we can not explain the magnetic field tilts of Uranus & Neptune.
![Page 44: © 2005 Pearson Education Inc., publishing as Addison-Wesley Giant Planets Jupiter Saturn Uranus Neptune.](https://reader030.fdocuments.us/reader030/viewer/2022032704/56649d3a5503460f94a14e40/html5/thumbnails/44.jpg)
© 2005 Pearson Education Inc., publishing as Addison-Wesley
Auroral ZonesThe high energy particles come down the field lines and hit the atmosphere near the poles, causing the gases to glow. Just like on the Earth, this makes an “aurora” in a ring-like zone.
![Page 45: © 2005 Pearson Education Inc., publishing as Addison-Wesley Giant Planets Jupiter Saturn Uranus Neptune.](https://reader030.fdocuments.us/reader030/viewer/2022032704/56649d3a5503460f94a14e40/html5/thumbnails/45.jpg)
© 2005 Pearson Education Inc., publishing as Addison-Wesley
The 4 “Jovian” Worlds
• Major features : Massive: 14 - 300 x mass of Earth Gaseous: Hydrogen, Helium & Water Rocky Core (Si, O, Fe, Ni …) Rotating Fast: 10 hours (squashed shape)