Chapter 8 โ Jovian Planet Systems
Jupiter
Size โ 11 Earths.
Rotation โ about 10 hours.
Revolution โ 12 years.
Mass โ 318 Earths.
Great Red Spot โ hurricane over 300 years old.
Zones โ whitish bands; warmer.
Belts โ dark bands; colder.
Ganymede โ largest moon in the solar system.
Callisto โ 3rd largest moon, most heavily cratered.
Io โ active sulfur volcanoes due to tidal heating.
Europa โ ice-covered cracked surface (subsurface ocean).
Saturn
Size โ 9 Earths.
Rotation โ about 10 hours.
Revolution โ 29.5 years.
Mass โ 95 Earths.
Titan โ thick nitrogen atmosphere.
Roche Limit โ area around a planet that will break up a moon.
Cassini Division โ gap in Saturn's rings due to tides from shepherding moons.
Ringlets โ Saturn's rings are in small ringlets, again due to shepherding moons.
Uranus
Size โ 4 Earths.
Rotation โ about 17 hours.
Revolution โ 84 years.
Tilt โ 98ยฐ on its side.
Neptune
Size โ 4 Earths.
Rotation โ about 16 hours.
Revolution โ 165 years.
Great Dark Spot โ hurricane found by Voyager.
Triton โ Neptune moon with active nitrogen geysers (orbits retrograde โ captured KBO).
Chapter 9 โ Asteroids, Comets, Dwarf Planets
Asteroid โ between Mars and Jupiter belt; rocks.
Trojan โ Jupiter's family of asteroids.
Earth Crossers โ Apollo class; can hit Earth โ NEO (Near-Earth Objects).
Comet diagram from class โ know nucleus + coma + plasma tail + dust tail (tails point AWAY from Sun).
Oort cloud โ spherical cloud surrounding the solar system out to ~50,000 AU.
Kuiper belt โ outside Neptune; leftover planetesimals (30โ100 AU, disk plane).
Meteoroid โ small piece in space.
Meteor โ burning up in our atmosphere.
Meteorite โ rock on the ground.
Chapter 10 โ Other Planetary Systems (Exoplanets)
Doppler Method โ radial velocity and astrometry.
Transit Method โ star eclipses as planet crosses (dimming).
Direct Detection Method โ taking a picture of the planet directly.
Properties known about exoplanets:
- Orbital period
- Distance from star
- Mass
- Size
- Density
- Atmosphere
Planetary Migration โ gas-giants formed far out, migrated inward โ "hot Jupiters."
Planetary Encounters โ gravitational interactions that change orbits.
Chapter 11 โ Our Star (the Sun)
Photosphere โ part of Sun we see; about 500 miles thick; 5800 K.
Chromosphere โ pink; ~10,000 miles above photosphere; 15,000 K.
Corona and Holes โ outer atmosphere; 1,000,000 K+. Areas with no corona are called holes.
Luminosity โ how much energy Sun gives off; Sun is the standard unit of 1 solar luminosity.
Convection Zone โ area just below surface where energy moves and undulates the Sun's surface.
Radiation Zone โ area around core of Sun that moves the energy outward.
Core โ 15,000,000 K; dense; all fusion takes place here.
Helioseismology โ study of convection undulations below the surface.
Granulation โ salt-and-pepper texture on surface due to convection.
Sunspots โ magnetic storms cooler by 2000 K on Sun's surface.
Cycle โ 11 years if you look at numbers; 22 years if you look at total polarity switch.
Prominences โ loops of gases that connect paired sunspots.
Flares โ hot storms that last 5โ20 minutes; 5 million degrees; sends out a lot of X-rays and solar radiation.
Fusion โ combining hydrogen into helium, which releases energy; only in the core.
p-p reaction โ proton-proton reaction in the Sun's core: 4 hydrogen โ 1 helium.
E = mcยฒ โ E = energy, m = mass, c = speed of light.
Neutrinos โ essentially massless particles created at the Sun's core; may let us study the core.
Study workflow
For Test 3, memorize the planet number table (size/rotation/revolution/mass). Drill in Flashcards filtered to U3 โ Practice Exam โ take Test 3.