Test 3 ยท Sun Jul 5 โ†’ Wed Jul 8 (11:59 PM) ยท Ch 8โ€“11 ยท 50 Qs (45 from this sheet)

Test 3 Review โ€” Jovians, Small Bodies, Exoplanets, the Sun

Verbatim review-sheet terminology from Kriegler's Test 3 sheet. Memorize the numbers (size, rotation, revolution, mass).

Review sheets: Test 1 ยท Ch 1โ€“4 Test 2 ยท Ch 5โ€“7 Test 3 ยท Ch 8โ€“11 Test 4 ยท Ch 12โ€“15 Test 5 ยท Ch 16โ€“19

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 (30โ€“100 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:
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 5โ€“20 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.