The Jovian Planets Saturn Jupiter Uranus Neptune Comparison

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The Jovian Planets Saturn Jupiter Uranus Neptune

The Jovian Planets Saturn Jupiter Uranus Neptune

Comparison • Terrestrial – close to the Sun – closely spaced orbits – small

Comparison • Terrestrial – close to the Sun – closely spaced orbits – small radii – small masses – predominantly rocky – high density – solid surface – few moons – no rings • Jovian – far from the Sun – widely spaced orbits – large radii – large masses – predominantly gaseous – low density – no solid surface – many moons – many rings

History • Jupiter and Saturn known to the ancients – Galileo observed 4 moons

History • Jupiter and Saturn known to the ancients – Galileo observed 4 moons of Jupiter and Saturn’s rings • Uranus – Discovered telescopically by William Herschel in 1781 (actually barely visible to naked eye) • Neptune – Predicted from observed perturbations of Uranus's orbit: Adams (1845) and Leverrier (1846) – Observed by Galle (1846) – Discovery great triumph for computational astronomy/physics

Grand Tour of Voyager 1 & 2 • Used gravitational slingshot to get from

Grand Tour of Voyager 1 & 2 • Used gravitational slingshot to get from planet to planet

Positions in Solar System • Jupiter: 5 A. U. distance from sun, takes 12

Positions in Solar System • Jupiter: 5 A. U. distance from sun, takes 12 years to go around the sun • Saturn: 9. 5 A. U. distance, Saturn year= 29 Earth years • Uranus: 19 A. U. distance, Uranus year= 84 Earth years • Neptune: 30 A. U. distance, Neptune year= 164 Earth years (all numbers approximate)

Rotation • About 10 hours for Jupiter and Saturn; about 17 hours for Uranus

Rotation • About 10 hours for Jupiter and Saturn; about 17 hours for Uranus and Neptune • Differential rotation: rotation speed varies from point to point on the “surfaces” – Gaseous bodies with no solid surfaces! – On Jupiter, the equatorial regions rotate 6 minutes slower than polar regions – On Saturn the equatorial region is about 26 minutes slower • Tilt of rotation axes: – Jupiter: almost none – no seasons! – Saturn, Neptune: about like Earth – Uranus: weird

Uranus’s Strange Seasons

Uranus’s Strange Seasons

Jupiter’s Atmosphere • Cloud bands parallel to equator • Great Red Spot – First

Jupiter’s Atmosphere • Cloud bands parallel to equator • Great Red Spot – First observed in 1664 by Robert Hooke

Jupiter’s Atmosphere • 86% Hydrogen, 14% Helium; some methane, water, ammonia • Several layers

Jupiter’s Atmosphere • 86% Hydrogen, 14% Helium; some methane, water, ammonia • Several layers of clouds: ammonia, ammonium hydrosulfide, water • Colors mostly due to compounds of sulfur and phosphorus

Jupiters’ Bands: Zones and Belts • Belts: cool, dark, sinking • Zones: warm, bright,

Jupiters’ Bands: Zones and Belts • Belts: cool, dark, sinking • Zones: warm, bright, rising • Jovian weather mostly circles the planet due to high rotation rate • Bands exhibit east–west flow Great Red Spot lies between regions of opposite wind flow

Great Red Spot • About twice the diameter of the Earth • A hurricane

Great Red Spot • About twice the diameter of the Earth • A hurricane that is hundreds of years old!

Saturn’s Atmosphere • 92% Hydrogen 7% Helium; some methane, water, ammonia • Belt structure

Saturn’s Atmosphere • 92% Hydrogen 7% Helium; some methane, water, ammonia • Belt structure similar to Jupiter’s, but fainter • Storms are rarer • White spot seen, 1990 (Voyager)

Uranus’ and Neptune’s Atmospheres Neptune’s Dark Spot • Ammonia frozen out; more methane –

Uranus’ and Neptune’s Atmospheres Neptune’s Dark Spot • Ammonia frozen out; more methane – Methane absorbs red light, leads to bluish color • Almost no band structure on Uranus

Magnetospheres • Very strong – Jupiter's extends past the orbit of Saturn! • Indicate

Magnetospheres • Very strong – Jupiter's extends past the orbit of Saturn! • Indicate the presence of conducting cores

Rings Saturn Uranus Jupiter Neptune

Rings Saturn Uranus Jupiter Neptune

Saturn • Rings composed of small, icy fragments, orbiting in concentric circles • Orbits

Saturn • Rings composed of small, icy fragments, orbiting in concentric circles • Orbits obey Kepler’s laws (of course!) – Inner rings move faster than outer ones

Visibility of Saturn’s Rings 2009

Visibility of Saturn’s Rings 2009

How Do They Form? • Miscellaneous debris • Moons or other small bodies torn

How Do They Form? • Miscellaneous debris • Moons or other small bodies torn apart by tidal forces • Roche limit – distance inside of which an object held together by gravity will be pulled apart

Ring Formation • Rings may be short lived (on the time scale of solar

Ring Formation • Rings may be short lived (on the time scale of solar system) • Means that they must form fairly frequently • A moon may pass too close to a planet (within the Roche limit) and be destroyed by tidal forces – This will probably happen to Triton (a moon of Neptune) within 100 million years!

Moons • Big moons: Earth’s moon, Jupiter’s Galilean Moons (Io, Europa, Ganymede, Callisto), Saturn’s

Moons • Big moons: Earth’s moon, Jupiter’s Galilean Moons (Io, Europa, Ganymede, Callisto), Saturn’s Titan, Neptune’s Triton diameters >2500 km, largest: 5260 km • Medium moons: diameter 400 -1600 km e. g. all of Uranus’ major moons • Small moons: diameter down to 20 km

Jupiter’s Galilean Moons

Jupiter’s Galilean Moons

Io • Jupiter’s innermost moon • Size and mass similar to our moon •

Io • Jupiter’s innermost moon • Size and mass similar to our moon • Zips around Jupiter in just 2 days

 • 2 day orbit around Jupiter (Moon: 28 days) • The most volcanically

• 2 day orbit around Jupiter (Moon: 28 days) • The most volcanically active object in the solar system – Heated by tidal friction • Eruptions as high as 200 miles Io

Europa might have liquid water oceans under the surface Life?

Europa might have liquid water oceans under the surface Life?

Saturn’s Moons Two-faced 0000 rooftop looks like Star Wars’ Death Star

Saturn’s Moons Two-faced 0000 rooftop looks like Star Wars’ Death Star

Titan • Titan is the only moon in the solar system known to have

Titan • Titan is the only moon in the solar system known to have an atmosphere Infrared picture shows surface details