PPT-Probing the Depths of Jupiter’s Atmosphere using Juno’s

MultiWavelength Eyes Glenn Orton Background Observations of Jupiter from various instruments on board the Juno spacecraft reveal a 3Dimensional view of the planet Data amp Results. TOTALLY different planets than our familiar next door neighbors . They formed beyond the frost line – so . ices. could form and . seed. the early stages of agglomeration. There’s a lot more ice-type raw material than rock-type raw material, so you get bigger planets!. Queen of the Gods and Goddess of Marriage . . Juno enjoys wearing a diadem. . Facts . Lives on Mt. Olympus . . After Juno’s mother gave birth to her. She was then swallowed by . Saturn . .. . Jupiter. 11.1 Orbital and Physical Properties. 11.2 The Atmosphere of Jupiter. A . Cometary. Impact. 11.3 Internal Structure. Almost a Star?. 11.4 Jupiter’s Magnetosphere. 11.5 The Moons of Jupiter. P. ropagation . T. ool. Chihiro Tao. 1,2. ,. . Nicolas Andre. 1. , Vincent Génot. 1. , Alexis P. Rouillard. 1. , Elena Budnik. 1. , Arnaud Biegun. 1. , Andrei Fedorov. 1. 1. IRAP, Univ. de Toulouse/UPS-OMP/CNRS. Chapter . 7 The . Jovian Planets. Observations of Jupiter and Saturn. The Discoveries of Uranus and Neptune. Bulk Properties of the Jovian Planets. Jupiter’s Atmosphere. The Atmospheres of the Outer Jovian Worlds. Configuration. Juno Spacecraft. en route to. Jupiter. (Arrives July 4. th. 2016). . National Aeronautics and. Space Administration. Goddard Space Flight Center. Jet Propulsion Laboratory. PI: Scott Bolton SWRI . Jupiter can be imaged well from Earth, even with a small telescope.. Here: Jupiter with its Galilean moons. Observations of Jupiter and Saturn. Natural color image. Jupiter: King of Gods. Observations of Jupiter . To the Student. What You Will Do and Learn. In this activity, you will use specific website pages and this presentation to compare and contrast the aurora of Earth to the aurora of Jupiter. . You will learn: . TOTALLY different planets than our familiar next door neighbors . They formed beyond the frost line – so . ices. could form and . seed. the early stages of agglomeration. There’s a lot more ice-type raw material than rock-type raw material, so you get bigger planets!. TOTALLY different planets than our familiar next door neighbors!. They formed beyond the frost line – so ices could form and seed the early stages of agglomeration. There’s a lot more ice-type raw material than rock-type raw material, so you get bigger planets!. for the . Juno Mission to Jupiter. FSW-17. Authors. Patrick H. . Stakem. , Johns Hopkins University, Capitol Technology University.. (pstakem1@jhu.edu). Rodrigo Santos Valente Da Costa, . Universidade. TOTALLY different planets than our familiar next door neighbors!. They formed beyond the frost line – so ices could form and seed the early stages of agglomeration. There’s a lot more ice-type raw material than rock-type raw material, so you get bigger planets!. Shun Zhou. IHEP, CAS, Beijing. on . behalf of the JUNO Collaboration. The 8. th. Workshop of France-China Particle Physics Laboratory. USTC, Hefei, April 8 - 10, 2015. T. he JUNO Experiment. 20 . kton. PRESS KIT/AUGUST 2011Press KitMedia ContactsDwayne BrownPolicy/Program202-358-1726dwaynecbrownnasagov WashingtonDC Agle Juno Mission818-393-9011Jet PropulsionLaboratoryPasadena CalifMaria Martinez Sci