Download Jovian Planets

Survey
yes no Was this document useful for you?
   Thank you for your participation!

* Your assessment is very important for improving the workof artificial intelligence, which forms the content of this project

Document related concepts
no text concepts found
Transcript
Jupiter
Radius
Mass
Surf. Gravity
Density
Semi-major axis
Orbital Period
Rotation Period
142,984 km
1.90 x 1027 kg
23.1 m/s2
1.33 g /cm3
778.6 x 106 km
11.86 years
9.925 hrs
Largest of all the planets (size & mass)
Hosts ~ 60 moons, most of which are captured asteroids
MPP©2004
Structure
Composition: 90% H2, 10% He, 0.2% CH4, 0.02% NH3
Upper Atmosphere (1000 km)
Band appearance caused by high speed
winds (640 km/hr) & differential rotation
MPP©2004
Belts & Zones
MPP©2004
Great Red Spot
High pressure storm in S. Hemisphere
D = 25,000 km
8 km above upper atmosphere
6 day rotation period
MPP©2004
Persisted for 400 years!
Interior
Pressure and Temperature increase at greater depths
Pressure gets so intense, the hydrogen forms a liquid-metallic state
Core is still expending energy left over from initial formation
MPP©2004
Magnetic Field
Metallic hydrogen is highly conductive to electricity; coupled with
FAST rotation ! source of Jupiter’s strong magnetic field
Aurora
Io Torus
MPP©2004
Ring System
Found by Voyager 1 in 1979
Low reflectivity = dust grains
MPP©2004
Within Jupiter’s Roche Limit
Roche Limit
Boundary around a massive planet where tidal forces become so
strong that any object (moon, asteroid, comet) will be torn apart.
MPP©2004
Comet Shoemaker-Levy 9
Only comet impact of another planet ever observed (July 1994)
K fragment impact
MPP©2004
T ~ 7500 K
Galilean Moons
Io - most volcanically active object in S.S.
Surface regularly renewed by lava flows
MPP©2004
Galilean Moons
Io’s volcanism is driven by tidal heating as it orbits Jupiter
Quick revolution (1.88 days) & slightly eccentric orbit creates tidal
forces that squeeze Io; keeps interior molten.
MPP©2004
Galilean Moons
Europa – surface is highly reflective and very smooth
- Subsurface ocean
Surface cracks from H2O volcanoes
Very thin oxygen atmosphere?
MPP©2004
Galilean Moons
Ganymede – largest satellite in the Solar System
Crust made of ice 500 km thick floating on slushy mantle
Evidence of past tectonic activity
Very thin oxygen atmosphere?
MPP©2004
Galilean Moons
Callisto – most heavily cratered object in the Solar System
• 200 km thick ice layer
• 10 km salt water ocean under crust
VERY thin CO2 atmosphere
Gipul Catena – crater chain
MPP©2004
Saturn
Radius
120,536 km
5.69 x 1027 kg
Mass
Surf. Gravity
Density
9.02 m/s2
0.69 g /cm3
Semi-major axis
1.43 x 109 km
Orbital Period
29.46 years
Rotation Period
10.66 hours
Similar to Jupiter in terms of:
• Composition
• Belt/zone circulation
• Interior
MPP©2004
Ring System
1st observed by Galileo in 1610 as “protrusions” which “vanished” by 1612
Viewing angle changes
MPP©2004
Ring System
Composed of dust/ice particles (1 cm – 1 m)
Cassini Division
D = 265,000 km
Thickness = 2 km (transparent)
MPP©2004
Ring System
Three main rings (A, B, C) composed of thousands of thinner rings
Cassini
Voyager 1
Gaps result from orbital resonance with Saturn’s moons
MPP©2004
Shepherd Satellites
Moons that keep material confined to the rings.
Prometheus
F ring
MPP©2004
Ring Effects
Ring Spokes – charged dust trapped
in Saturn’s magnetic field
Gravitational influence of Pan
MPP©2004
Ring Effects
Prometheus
Braided F Ring
MPP©2004
Titan
Largest moon of Saturn
CH4 haze
Surface
Possible source of organic molecules (life?) and fuel
Cassini mission sent Huygens probe to surface: January 5, 2005
MPP©2004
Uranus
MPP©2004
Neptune
51,118 km
Radius
49,528 km
8.66 x 1025 kg
Mass
1.02 x 1026 kg
9.60 m/s2
Surf. Gravity
11.0 m/s2
1.27 g /cm3
Density
1.64 g /cm3
2.87 x 109 km
Semi-major axis
4.50 x 109 km
84.1 years
Orbital Period
164.8 years
17.24 hours
Rotation Period
16.11 hours
Uranus
Neptune
Excess methane causes blue appearance
MPP©2004
Magnetic fields are greatly tilted and off-center
Uranus
• 1st planet discovered not known to ancients
• found by William Herschel during
stellar parallax studies (1781)
• plotted as a star over 20 times
MPP©2004
Uranus
Rotational axis is tilted 97.3°
Atmosphere circulates heat to keep temperature uniform
MPP©2004
Uranus
Rings: 1st observed during a 1977 occultation
As Uranus passes in front the star, the star’s brightness will drop
MPP©2004
Neptune
• 1st planet predicted to exist by theory (Adams & Leverrier)
• discovered by Johanne Galle (1846)
• plotted by Galileo on two occasions while observing Jupiter
Methane cirrus clouds
Great Dark Spot
Small Dark Spot
MPP©2004
Pluto
Radius:
Charon
Mass:
Surf. Gravity:
Pluto
Density:
Semi-major axis
Orbital Period
Rotation Period
MPP©2004
1,195 km
1.19 x 1022 kg
0.59 m/s2
1.75 g /cm3
5.87 x 109 km
247.7 years
6.39 days
iorb
17.1º
Eccentricity
0.244
New Moons?
MPP©2004
Pluto
Percival Lowell predicted planet w/ M = 7 MEarth was beyond Neptune
Searched for planet for 10 years, but to no avail
Lowell
Lowell Observatory
Flagstaff, AZ
Tombaugh, 1922
Clyde Tombaugh hired to look for predicted planet
MPP©2004
Pluto
Searched star fields for ~ 1 year; discovered February 18, 1930
• Comes closer than Neptune
• Tidally locked Charon
• Only ~ twice the size of Charon
MPP©2004
• Comet-like
• In Kuiper Belt
• Found serendipitously