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|    BAMA    |    Science Research Echo    |    1,586 messages    |
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|    Message 468 of 1,586    |
|    Roger Nelson to All    |
|    Asteroid Moon Movie    |
|    07 Jun 13 17:13:58    |
      Asteroid Moon Movie               June 7, 2013: Scientists working with NASA's 230-foot-wide (70-meter) Deep       Space Network antenna at Goldstone, Calif., have released a new and improved       movie clip of near-Earth asteroid 1998 QE2 and its moon. The 55 individual       images used in the movie were generated from data collected at Goldstone on       June 1, 2013.               http://www.youtube.com/watch?v=ssYnC90U0mM               In this movie, each of the individual images required about five minutes of       data collection by the Goldstone radar. At the time of the observations on       June 1st, asteroid 1998 QE2 was about 3.75 million miles (6 million       kilometers) from Earth. The resolution is about 125 feet (38 meters) per       pixel. Play the movie!               The asteroid's satellite, or moon, is approximately 2,000 feet (600 meters)       wide, has an elongated appearance, and completes a revolution around its host       body about once every 32 hours. At any point during its orbit, the maximum       distance between the primary body and moon is about 4 miles (6.4 kilometers).       Similar to our moon, which always points the same "face" at Earth, the       asteroid's satellite appears to always show the same portion of its surface to       the primary asteroid. This is called "synchronous rotation."               The radar data indicate the main, or primary body, is approximately 1.9 miles       (3 kilometers) in diameter and has a rotation period of about five hours. This       makes 1998 QE2 one of the slowest (with respect to its rotation) and largest       binaries that have been observed by planetary radar. In the near-Earth       population, about 16 percent of asteroids that are about 655 feet (200 meters)       or larger are binary or triple systems.               Each of the individual images obtained on June 1, 2013, required about five       minutes of data collection by the Goldstone radar. At the time of the       observations that day, asteroid 1998 QE2 was about 3.75 million miles (6       million kilometers) from Earth. The resolution is about 125 feet (38 meters)       per pixel.               The trajectory of asteroid 1998 QE2 is well understood. The closest approach       of the asteroid occurred on May 31 at 1:59 p.m. PDT (4:59 p.m. EDT / 20:59       UTC), when the asteroid got no closer than about 3.6 million miles (5.8       million kilometers), or about 15 times the distance between Earth and the       moon. This was the closest approach the asteroid will make to Earth for at       least the next two centuries.               For more information about the near-Earth flyby of 1998 QE2 watch the       ScienceCast video Big Asteroid Flyby               Credits:               Production editor: Dr. Tony Phillips | Credit: Science@NASA               More information and web links:               Asteroid 1998 QE2 was discovered on Aug. 19, 1998, by the Massachusetts       Institute of Technology Lincoln Near Earth Asteroid Research (LINEAR) program       near Socorro, N.M.               NASA places a high priority on tracking asteroids and protecting our home       planet from them. In fact, the United States has the most robust and       productive survey and detection program for discovering near-Earth objects. To       date, U.S. assets have discovered more than 98 percent of the known Near-Earth       Objects.               In 2012, the Near-Earth Object budget was increased from $6 million to $20       million. Literally dozens of people are involved with some aspect of       near-Earth object research across NASA and its centers. Moreover, there are       many more people involved in researching and understanding the nature of       asteroids and comets, including those objects that come close to Earth, plus       those who are trying to find and track them in the first place.               In addition to the resources NASA puts into understanding asteroids, it also       partners with other U.S. government agencies, university-based astronomers,       and space science institutes across the country that are working to track and       better understand these objects, often with grants, interagency transfers and       other contracts from NASA.               NASA's Near-Earth Object Program at NASA Headquarters, Washington, manages and       funds the search, study, and monitoring of asteroids and comets whose orbits       periodically bring them close to Earth. JPL manages the Near-Earth Object       Program Office for NASA's Science Mission Directorate in Washington. JPL is a       division of the California Institute of Technology in Pasadena.                       Regards,               Roger              --- D'Bridge 3.94        * Origin: NCS BBS - Houma, LoUiSiAna (1:3828/7)    |
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