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WOU ES 104 - Outer Planets

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1 Arrow h t shows entry point of Galileo probe, Dec. 1995http://www.solarviews.com/raw/jup/vjupitr5.mpg• http://www2.jpl.nasa.gov/galileo/hstimages.htmlLink to rotating view of Jupiter• http://photojournal.jpl.nasa.gov/catalog/PIA00743 True color on top Enhanced color on bottomSurface covered with Surface covered with calderas (like Crater Lake…without the water!)• http://www.nineplanets.org/io.html• http://photojournal.jpl.nasa.gov/catalog/PIA007462• http://www.solarviews.com/cap/jup/callist1.htm Metis, Adrastea, Amalthea, Thebe Amalthea is 247 km across Photos by Galileo probe, 1996-97• http://www2.jpl.nasa.gov/galileo/ganymede/PIA01076.html Discovered by Voyager I This photo by Galileo space probe--November 9, 1996• http://www2.jpl.nasa.gov/galileo/callisto/p48188.html Voyager I, II went there in 1980, 81 This photo by Cassini in 2004• http://www.nineplanets.org/saturn.html• http://saturn.jpl.nasa.gov/overview/index.cfm• http://saturn.jpl.nasa.gov/multimedia/images/image-details.cfm?path=../multimedia/images/rings/images/PIA05421.jpg&type=image• http://ciclops.lpl.arizona.edu/view.php?id=575• http://www.esa.int/SPECIALS/Cassini-Huygens/SEMHB881Y3E_1.html3• http://pds.jpl.nasa.gov/planets/captions/saturn/encelads.htm• http://hubblesite.org/newscenter/newsdesk/archive/releases/1996/15/image/a Asteroids Meteoroids CometsKuiper Belt ObjectsKuiper Belt Objects Dwarf Planets Orbits Sun Not a satellite Dominates its orbital path is in orbit around Sun  has sufficient mass for its self-gravity to pull itself into near-spherical shape has not cleared the neighborhood around has not cleared the neighborhood around its orbit  is not a satellite HST image• http://www.solarviews.com/cap/pluto/pluto3.htm Pluto does not dominate its orbit Pluto is the first discovered Kuiper Belt Object“Plutonian objects” of which it “Plutonian objects” of which it is the original example Pluto’s moon is Charon4 Notice Pluto is sometimes closer to Sun than Neptune • http://www.nineplanets.org/plutodyn.html Notice Pluto’s large inclination to Sun’s equator• http://www.nineplanets.org/plutodyn.html Donut shaped area containing numerous icy bodies of various sizes Eris is the largest discovered Pluto and Charon are some Titan, moon of Saturn, is likely one that was captured by Saturn’s gravity Origin of numerous comets that orbit Sun in periods less than 200 years A division of Trans-Neptunian Objects Kuiper Belt Object Larger than Pluto Discovered in 2003http://en.wikipedia.org/wiki/Eris_(dwarf_planet)http://www.gps.caltech.edu/~mbrown/planetlila/#sizeIn redCompare to Pluto in black• http://www.gps.caltech.edu/%7Echad/2004dw/ Pluto in red Neptune in gray Orcus in blue wikipedia, Orcus-transNeptunian object, 2008-1013 Earth for scale wikipedia, Orcus-transNeptunian object, 2008-1013 More Info: http://solarsystem.nasa.gov/planets/profile.cfm?Object=KBOs&Display=OverviewLongOrbits of Makemake (blue), Haumea (green), contrasted with the orbit of Pluto (red) and the ecliptic (grey). The perihelia(q)[3]and the aphelia (Q) are marked with the dates of passage. The positions on April 2006 are marked with the spheres illustrating relative sizes and differences in albedoand colour.5 Large Kuiper Belt Objects Pluto Eris Makemake Haumea The asteroid Ceres Other KBOs likely to be discovered that are also dwarf planets• http://www.space.com/scienceastronomy/050907_ceres_planet.htmlIda, Gaspra, Deimos, Phobos• http://www.nineplanets.org/asteroids.html• http://www.jplnet.com/img2002/meteor.jpg• http://www.dmsweb.org/6• http://www.xtec.es/recursos/astronom/craters/METEOR.jpg• http://www.nineplanets.org/sl9.html•


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WOU ES 104 - Outer Planets

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