Moog Hardware in Space

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MOOG IN SPACE OH, THE WONDERS WE WILL SEE WILD 2 & BRAILLE & 67P CHURYUMOV- HEO TEMPEL 1 BORRELLY GERASIMENKO COMET Magnetospheric Stardust Deep Space-1 Rosetta Multiscale SUN TESS› Parker Solar Probe› EARTH/SUN EARTH/SUN JUPITER Spitzer Space LAGRANGE L1 1999 JU3 25143 ITOKAWA BENNU LAGRANGE L2 TROJANS Telescope DSCOVR Hayabusa-2 Hayabusa-1 OSIRIS-Rex James Webb Space Telescope* Lucy* Solar Orbiter* ACE Herschel LISA Pathfinder Planck Genesis GAIA PLUTO New Horizons VESTA MERCURY VENUS MOON MARS & CERES 16 PSYCHE JUPITER SATURN URANUS NEPTUNE MESSENGER Magellan LCROSS Mars Science Laboratory DAWN Psyche* Juno Cassini Voyager 2 Voyager 2 BepiColombo* Pioneer 12 LRO Mars 2020* Galileo Pioneer 11 Pioneer 13 GRAIL Exo Mars* Pioneer 10 Voyager 1 Akatsuki Clementine (DSPSE) MRO Voyager 1 LADEE MGS Europa Clipper* Apollo Program Mars Odyssey JUICE* SMART-1 Viking-1 Orion MPCV* Viking-2 Google Lunar MAVEN DID YOU KNOW THAT MOOG HAS TRAVELED TO EVERY PLANET? X-Prize Landers* Phoenix Moog designs and manufactures components industry for over 60 years. For future space Mars Climate Orbiter and systems to survive the harsh environments missions, Moog is investing significant resources InSight of space travel. An industry leader in space into propulsion test facilities, metal additive Hope* avionics, actuation and mechanisms, propulsion, manufacturing, rad-hardened avionics, and power, structures, and shock and vibration innovative orbital maneuvering vehicles. control, Moog has been committed to the space › In Transit * Yet To Be Launched Moog Inc. 500 Jamison Road, Plant 20 East Aurora, New York 14052 ©2019 Moog, Inc. All rights reserved. 500-1191 0119 Product and company names listed are trademarks or trade names of their respective companies. www.moog.com/space.

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Volcanic History of the Imbrium Basin: a Close-Up View from the Lunar Rover Yutu
Volcanic history of the Imbrium basin: A close-up view from the lunar rover Yutu Jinhai Zhanga, Wei Yanga, Sen Hua, Yangting Lina,1, Guangyou Fangb, Chunlai Lic, Wenxi Pengd, Sanyuan Zhue, Zhiping Hef, Bin Zhoub, Hongyu Ling, Jianfeng Yangh, Enhai Liui, Yuchen Xua, Jianyu Wangf, Zhenxing Yaoa, Yongliao Zouc, Jun Yanc, and Ziyuan Ouyangj aKey Laboratory of Earth and Planetary Physics, Institute of Geology and Geophysics, Chinese Academy of Sciences, Beijing 100029, China; bInstitute of Electronics, Chinese Academy of Sciences, Beijing 100190, China; cNational Astronomical Observatories, Chinese Academy of Sciences, Beijing 100012, China; dInstitute of High Energy Physics, Chinese Academy of Sciences, Beijing 100049, China; eKey Laboratory of Mineralogy and Metallogeny, Guangzhou Institute of Geochemistry, Chinese Academy of Sciences, Guangzhou 510640, China; fKey Laboratory of Space Active Opto-Electronics Technology, Shanghai Institute of Technical Physics, Chinese Academy of Sciences, Shanghai 200083, China; gThe Fifth Laboratory, Beijing Institute of Space Mechanics & Electricity, Beijing 100076, China; hXi’an Institute of Optics and Precision Mechanics, Chinese Academy of Sciences, Xi’an 710119, China; iInstitute of Optics and Electronics, Chinese Academy of Sciences, Chengdu 610209, China; and jInstitute of Geochemistry, Chinese Academy of Science, Guiyang 550002, China Edited by Mark H. Thiemens, University of California, San Diego, La Jolla, CA, and approved March 24, 2015 (received for review February 13, 2015) We report the surface exploration by the lunar rover Yutu that flows in Mare Imbrium was obtained only by remote sensing from landed on the young lava flow in the northeastern part of the orbit. On December 14, 2013, Chang’e-3 successfully landed on the Mare Imbrium, which is the largest basin on the nearside of the young and high-Ti lava flow in the northeastern Mare Imbrium, Moon and is filled with several basalt units estimated to date from about 10 km south from the old low-Ti basalt unit (Fig.
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Appendix 1: Venus Missions
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