Planets, Dwarf Planets and moons of our Solar System Terrestrial Planets Jovian Planets.
Moons, Rings, & Dwarf Planets Solar System Astronomy Chapter 11.
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Transcript of Moons, Rings, & Dwarf Planets Solar System Astronomy Chapter 11.
Moons, Rings, & Dwarf Planets
Solar System AstronomyChapter 11
In the Solar System: Dozens of worlds
Rock & ice Diverse properties, only partially understood Offers insight into our ideas/theories of planet
formation
Moons Most larger moons formed with planets
Regular moons Some are captured objects
Usually in retrograde orbits Irregular moons
Major Moons Four gas giants Earth
Some are geologically active Others show evidence of past activity
Many Moons
Formation of Large Moons The largest moons formed the same way
the terrestrial planets did Major processes: accretion and differentiation Biggest difference with the terrestrials:
composition more ices (frozen water, methane, &c) less rock (silicates)
Rings All four gas giants have ring systems
Swarms of tiny moons Saturn’s are the largest and brightest Particles orbit according to Kepler’s laws
orbits are circular collisions or ring gravity keep them that way
Saturn’s Rings Very complicated system
thousands of ringlets bright and dark rings, and “gaps” gaps are not empty brightness/darkness indicates amount of
material in each ring system is extremely thin
Rings Rings don’t contain much material
mass of all the ring particles is about the same as a small, icy moon
Can be distorted by the gravity of nearby moons
Origin of Rings Ring material is from disrupted moons
Large moons are broken up within Roche limit Tidal forces
Other sources of ring material Volcanoes Impacts
Saturn’s rings formed from an icy moon Uranus’ and Neptune’s are very dark
Body rich in carbon
Moons & Rings Rings don’t last forever
Collisions and sunlight would destroy them Small, nearby shepherd moons can help
stabilize Moons also create gaps
orbital resonance: orbital period is in a ratio with the moon period
Titan Saturn’s largest moon
deep, nitrogen-rich atmosphere Currently being explored by the Cassini
spacecraft Huygens lander revealed icy “rocks” and a soil
rich with organic compounds
Titan Saturn’s largest moon
deep, nitrogen-rich atmosphere methane and ethane can condense and lead to rain
of methane and ethane Methane is gradually converted to ethane in the
atmosphere Renewed in active geology
Then there’s poor Pluto… Very small
1/6 the mass of Moon Binary planet: moon Charon
properties like comets eccentric orbit icy composition (probably) member of the Kuiper Belt Objects (KBO)
Probably not even the largest
Discovery of Pluto 1930 Clyde Tombaugh
Existence predicted from disturbances of Neptune
Though it’s too small…
Discovery of Pluto
Discovery of Pluto Venetia Burney
1930 2007
Venetia Burney Phair died April 30, 2009
Pluto Orbit
2:3 resonance with Neptune Comes closer to Uranus than Neptune
Dwarf Planets Small numbers, but increasing
Pluto Charon, Nix, Hydra
Eris Dysnomia
Ceres Haumea
Hi’iaka, Namaka Makemake