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CH 25.4 Outer Planets Gas Giants • Jupiter, Saturn, Uranus, & Neptune • Large, “gaseous” planets with small solid cores of metal & rock. • Made mostly of Hydrogen & Helium – under great pressures H & He existing as liquids w/in planet 5.2 AUs from sun Orbit time (Rev.) = 12 yrs Rotation = 9.8 hours GASEOUS, LARGEST & MOST MASSIVE PLANET (mass = 318 x Earth) Features: Cloud Bands, Giant Red Spot storm system, single faint ring Atmosphere = Hydrogen, Helium Temps = -144C (but hot core) Lg. Magnetosphere – currents of metallic liquid Hydrogen moons: 50+ Exploration: Voyager & Galileo Spacecraft Flybys http://www.youtube.com/watch?v=92PdqOA7VE Y&feature=relmfu Io - volcanic Ganymede – icy (Large) Callisto - icy Europa – icy (salt water ocean underneath) The History Channel’s “The Universe – Jupiter” http://www.youtube.com/watch?v=rLeKE8hfP8M Most volcanically active location in the solar system. Europa may have life under its salt water ocean under its frozen surface. http://www.youtube.com/watch?v=rVDE14tFyEM&feature=PlayList&p=10F85C2BC16A885E&index=0 http://www.youtube.com/user/Knowledge2Truth#p/c/28A94D2A4AEC778C/15/-tsamka8gHU http://www.youtube.com/watch?v=4D8Y9J3aL3I GASEOUS- 2nd Largest, Least dense (could float) Moons: 30+ Atmosphere: Hydrogen, Helium, + Features: Large ring system (icy (Rains helium) rock/dust) Cloud Temps: -176C (hot bands core) 9.5 AUs from sun Orbit time (Rev) = 29.5 yrs Rotation = 10.67 hrs Titan: Saturn’s Moon •Has an THICK ATMOSPHERE •Nitrogen & Methane •Liquid lakes of ethane & methane. • Cassini-Huygen’s Mission recently explored Titan with a probe • Cassini continues to explore Saturn The Universe: Saturn 1/3 http://www.youtube.com/watch?v=GfDQeZxPsgw 19.2 AUs Orbit Time (Rev): 84 years Rotation: 17.24 hrs. GASEOUS & RINGS Atmosphere: Hydrogen, Helium Methane, Ammonia Tilted on side 90 degrees and rotates backwards (retrograde) Temps: - 215 C (hot core) moon: 20+ The History Chanel’s Outer Planets: http://www.youtube.com/watch?v=YIrhTXRROgo 30 AUs Orbit time (Rev) = 165 yrs. •GASEOUS & RINGS Rotation = 17.24 hrs. •Atmosphere: Methane, Hydrogen, Ammonia •Temps: -355 F •Features Dark Spot storm system (vanished 1994) Moons: 8+ (Triton is largest) Windiest Planet (1200 mph winds) •Clouds of Methane Ice Crystals http://www.youtube.com/watch?v=woBY6CiIfTg&feature=PlayList&p=DD2B 509749D92C27&playnext=1&playnext_from=PL&index=13 http://www.youtube.com/watch?v=ZgKpinHLY-Q Common Features of Outer Planets • • • • • • Large in size Gaseous surfaces of H & He Many Moons Rings Cold temperatures Long revolutions Dwarf Planet Probably a Kuiper Belt Object 40 AUs Trace Atmosphere (methane) Temps. - 223 C/ -400F SOLID – icy rock w/ frozen methane New Horizons Dense Spacecraft – left Moon: Charon (almost same size; in 2006; will they chase each other arrive in 2015 Eccentric &Tilted Orbit (17 degrees) http://www.youtube.com/watch?v=ZgKpinHLY-Q Discovery: http://www.youtube.com/watch?v=u1RU6P-fUr4 http://www.cnn.com/videos/us/2015/01 /26/orig-new-horizons-probe-nearspluto-nasa.cnn http://www.nasa.gov/mission_pages/n ewhorizons/main/index.html Reasons Pluto was Reclassified 1. Too small & solid(Outer planets are large & gaseous) 2. No rings 3. Only 1 moon (and it chases it). 4. Orbit is very elliptical & tilted 5. More in common with K.B.O.s Kuiper Belt K.B.O.s Round icy rock bodies like Pluto continue to be found & classified. Sedna Short term comets are also in K. Belt (~ 200 yr.orbits) http://www.solarviews.com/eng/kuiper.htm Starts at Neptune’s orbit and extends for 30 – 50 AU out. In the ecliptic plane w. planets www.astro.rug.nl http://discovermagazine.com/2004/nov/cover/outer-oort.jpg The Universe: The Outer Planets (& Pluto & KBO) http://www.youtube.com/watch?v=osWm8QygoH4 library.thinkquest.org Found in Kuiper Belt (region that starts @ Neptune’s orbit and extends past Pluto & is in the ECLIPITC Dirty Snowballs with a rocky core PLANE) & Oort Cloud (SPHERE OF Comets Vapor tail forms as it approaches surrounding S. sun (Solar wind evaporates frozen system as a shell) gases) •Tail faces away from sun •Short Range – 200 yrs (K.Belt) • Long Range – millions or years (Oort Cloud) http://abyss.uoregon.edu/~js/ast121/lectures/lec24.html Check Up 1. 2. 3. 4. List 3 reasons why Pluto is an “odd-ball” What is Pluto now considered? What 2 places can you find comets? Describe a KBO – where do you find them? • • Birth of the Solar System (National Geographic) http://www.youtube.com/watch?v=B1AXbpYndGc Planets form (Condensation Temps): http://www.youtube.com/watch?v=p5nCMCZSVxg • • Massive Solar Storms (National Geographic) http://www.youtube.com/watch?v=DU4hpsistDk&feature=relmfu • Massive Solar Storms http://www.youtube.com/watch?v=DU4hpsistDk&feature=list_related&playnext=1&list=SL