Please find below the latest Mission Status Reports from the Sentinel-1 Team. These reports provide information on the status of the satellite and the instrument, the associated ground segment, and any mission milestones.
The mission uses technological innovations already demonstrated successfully, especially for entry, descent, and landing (EDL). Like NASA's Curiosity rover (, the Mars 2020 spacecraft uses a guided entry, descent, and landing system. The landing system on Mars 2020 mission includes a parachute, descent vehicle, and an approach called a "skycrane maneuver" for lowering the rover on a tether to the surface during the final seconds before landing.
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The Perseverance rover design minimizes costs and risks because it is largely based on the engineering design for the previous Curiosity rover. The Perseverance long-range mobility system allows it to travel on the surface of Mars over 3 to 12 miles (5 to 20 kilometers). Improvements on Perseverance include a new, more capable wheel design. And for the first time, the rover carries a drill for coring samples from Martian rocks and soil. It gathers and stores the cores in tubes on the Martian surface, using "depot caching." Caching demonstrates a new rover capability of gathering, storing, and preserving samples. This could potentially pave the way for future missions to retrieve the samples and ferry them to Earth for intensive laboratory analysis.
Perseverance tests a technology for extracting oxygen from the Martian atmosphere, which is 96% carbon dioxide. This demonstration helps mission planners test ways of using Mars' natural resources to support human explorers and improve designs for life support, transportation, and other important systems for living and working on Mars. The rover also monitors weather and dust in the Martian atmosphere. Such studies are important for understanding daily and seasonal changes on Mars, and will help future human explorers better predict Martian weather.
This website replays the Apollo 11 mission as it happened, 51 years ago. It consistsentirely of historical material, all timed to Ground Elapsed Time--the mastermission clock. Footage of Mission Control, film shot by the astronauts, andtelevision broadcasts transmitted from space and the surface of the Moon, have beenpainstakingly placed to the very moments they were shot during the mission, as hasevery photograph taken, and every word spoken.
Navigate to any moment of the mission using the time navigator at the top of thescreen. The top bar is the entire mission with two bars below it providingmagnification. Selecting transcript items, photos, commentary items, or guided tourmoments, also jumps the mission time to the moment they occurred.
Main mission audio consists of space-to-ground (left ear), capcom loop (right ear),and on-board recorder (center, when available). Selecting a Mission Control audiochannel mutes the main audio, opens the Mission Control audio panel, and plays the"live" audio of that Mission Control position. Change channels by selecting theseats in mission control. Closing the Mission Control audio panel will unmute themain audio and continue mission playback.
Ben Feist Concept, research, mission data restoration,audio restoration, video, software architecture and programming. Follow@BenFeistfor updates.Stephen Slater Archive Producer, historical audio/footagesynchronizationChris Bennett Visual design, interface styling andprogrammingDavid Charney Visual designArnfinn Holderer Audio restoration programmingRobin Wheeler Photography timing, transcript corrections
Todd Miller Director,Apollo 11 filmTom Petersen Producer,Apollo 11 filmDr. John Hansen and the National Science Foundation30-track Mission Controlaudio digitization. More info atexploreapollo.orgLunar and Planetary InstituteJamie Shumbera Operations ManagerNASA HeadquartersDr. Bill Barry Chief Historian, NASA HQDr. Jacob Bleacher Chief Exploration Scientist, NASA HQNASA Johnson Space CenterDr. Cindy Evans Division Chief, Astromaterials Researchand Exploration Science (ARES) Division, NASA JSCDan Garrison Jacobs Technology, NASA JSCDr. Ryan Zeigler Manager, Apollo Curator, ARES, NASA JSCDr. Paul Niles Assistant Chief Scientist, ARES NASA JSCSandra Tetley Real Property Officer, Historic PreservationOfficer, NASA JSCGreg Wiseman 30-track Mission Controlaudio digitization, NASA JSCNASA Goddard Space Flight CenterDr. Noah Petro Project Scientist, Lunar Reconnaissance Orbiter. Planetary Geology, Geochemistry and Geophysics Lab, NASA GoddardWeb hosting byDavid Woods Author,How Apollo Flew to the MoonKipp TeagueApollo mission photographyPaul Vanezis EVA footageNASA Apollo Flight JournalNASA Apollo Lunar Surface JournalInternet ArchiveThe crew of Apollo 11The men and women of Mission ControlBeta TestersMike Dinn Jacqueline PooleTodd Green Ian HouseJoey Schwartz David CharneySammy Goldberg Robin WheelerJoe Davenport Linden SimsSuzanne Molina Kevin SpencerTHIS WEBSITE IS THE COPYRIGHT OF BEN FEIST 2019.THE ARCHIVE MATERIAL ON THIS WEBSITE COMPRISES NASA AUDIO RESTORED BY BEN FEIST ANDNASA SYNCHRONISED AUDIO/VISUAL MATERIAL PROVIDED BY STEPHEN SLATER.ANY SYNCHRONISED FOOTAGE MAY ONLY BE REPRODUCED AND UTILISED WITH THE PRIOR WRITTENPERMISSION OF STEPHEN SLATER. ALL RIGHTS IN THE SYNCHRONISED FOOTAGE ARE EXPRESSLYRESERVED TO STEPHEN SLATER.
Geologic samples returned from the Moon by the six Apollo lunar surface exploration missions (1969-1972), along with associated data records, are physically protected, environmentally preserved, and scientifically processed by NASA's Astromaterials Research and Exploration Science Division in building 31N, a special building dedicated for that purpose, at Johnson Space Center in Houston, Texas. A total of 382 kilograms of lunar material, comprising 2200 individual specimens returned from the Moon, has been processed to meet scientific requirements into more than 110,000 individually cataloged samples.
The Deputy Assistant Secretary (Installations, Energy and Facilities) is focused on providing assured energy whenever and wherever it is required to enable mission accomplishment. Our purpose is to align the DON leadership on the objective of achieving assured energy and energy-related cyber controls at our installations, in the quantity and the quality we require to accomplish required missions.
Theology and Mission in World Christianity is a new peer-reviewed series which treats theology, mission, and the interface between them in view of the development of world Christianity. It is edited by Kirsteen Kim, Stephen B. Bevans and Miikka Ruokanen. The series is published by Brill Publishers and also functions as a supplement series for the IAMS journal Mission Studies. The editors welcome scholarly monographs, edited volumes, and outstanding dissertations on contextual and inter-cultural theologies, mission theology, and historical and practical questions relating to mission and Christianity worldwide. For further information, click here.
Our mission is to administer the permanent fund dividend program assuring that all eligible Alaskans receive timely dividends, fraud is prosecuted, and all internal and external stakeholders are treated with respect. 2ff7e9595c
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