Transcription of OURSOLARSYSTEM - NASA
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National Aeronautics and Space AdministrationNational Aeronautics and Space Solar SystemOur Star The SunMercuryVenusEarthEarth s MoonMarsAsteroidsMeteors and Meteorites Moons of the Solar SystemJupiterGalilean Moons of JupiterSaturnMoons of SaturnUranusNeptunePluto and CharonCometsKuiper Belt and Oort CloudWhat Is a Planet?Educational ProductEducatorsGrades K 12+LS-2013-07-003-HQ JPL 400-1489 07/13 NASA EDUCATIONAL RESOURCESThe NASA portal ( ) is the gateway for information about content, programs, and services offered for the general public and the education community. NASA s goal is to improve interactions for students, educators, and families with NASA and its education resources. NASA s education home page ( ; click on For Educators ) serves as the portal for information about edu-cational programs and services offered by NASA. A directory of information provides details and points of contact for all of NASA s educational efforts, NASA field center offices, and points of presence within each state.
mostly of hydrogen and helium, while Uranus and Neptune are composed mostly of water, ammonia, and methane, with icy mantles around their cores. The Voyager 1 and 2 spacecraft visited the gas giants, and Voyager 2 flew by and imaged the ice giants. Ceres and the outer dwarf planets — Pluto, Eris, Hau-
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