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|    BAMA    |    Science Research Echo    |    1,586 messages    |
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|    Message 171 of 1,586    |
|    Roger Nelson to All    |
|    Weekend Meteor Shower    |
|    21 Oct 11 08:29:23    |
      Weekend Meteor Shower               Oct. 20, 2011: Earth is about to pass through a stream of debris from Halley's       comet, source of the annual Orionid meteor shower. Forecasters expect more       than 15 meteors per hour to fly across the sky on Saturday morning, Oct. 22nd,       when the shower peaks.               http://science.nasa.gov/media/medialibrary/2008/08/10/19oct_magicalmorning_re       sources/meteor.jpg               Orionids are most easily seen during the dark hours before sunrise. Twilight       Orionids, however, are the most beautiful of all. "Although this isn't the       biggest meteor shower of the year, it's definitely worth waking up for," says       Bill Cooke of the NASA Meteoroid Environment Office. "The setting is dynamite."               Orionids are framed by some of the brightest and most beautiful constellations       in the night sky. The meteors emerge from mighty Orion, the shower's       glittering namesake. From there they streak through Taurus the Bull, the       twins of Gemini, Leo the Lion, and Canis Major--home to Sirius, the most       brilliant star of all.               This year, the Moon and Mars are part of the show. They'll form two vertices       of a celestial triangle in the eastern sky on Saturday morning while the       shower is most active; Regulus is the third vertex. Blue Regulus and red Mars       are both approximately of 1st magnitude, so they are easy to see alongside the       35% crescent Moon. Many Orionids will be diving through the triangle in the       hours before dawn.               Cooke's team at the Meteoroid Environment Office will be watching for Orionids       that actually hit the Moon.               Cometary debris streams like Halley's are so wide, the whole Earth-Moon system       fits inside. So when there is a meteor shower on Earth, there's usually one on       the Moon, too. Unlike Earth, however, the Moon has no atmosphere to intercept       meteoroids. Pieces of debris fall all the way to the surface and explode       where they hit. Flashes of light caused by thermal heating of lunar rocks and       moondust are so bright, they can sometimes be seen through backyard-class       telescopes.               http://science.nasa.gov/media/medialibrary/2011/10/20/skymap_north.gif               A map of the morning sky on Saturday, Oct. 22nd at 5:30 a.m. local time,       viewed facing southeast. Click to view a larger, more complete map.       "Since we began our monitoring program in 2005, our group has detected more       than 250 lunar meteors," says Cooke. "Some explode with energies exceeding       hundreds of pounds of TNT."               So far, they've seen 15 Orionids hitting the Moon--"two in 2007, four in 2008,       and nine in 2009," recalls Cooke. This year they hope to add to the haul.        About 25% of the Moon's dark terrain will be exposed to Halley's debris       stream, giving the team millions of square miles to scan for explosions.               Watching meteoroids hit the Moon is a good way to learn about the structure of       comet debris streams and the energy of the particles therein. It also allows       Cooke and colleagues to calculate risk factors for astronauts who, someday,       will walk on the lunar surface again.               "Going outside to watch the Orionids might not be a good idea for a       moonwalker," says Cooke.               But it is a good idea for the rest of us. Set your alarm for a few hours       before dawn on Saturday morning and enjoy the show.                       Author: Dr. Tony Phillips | Credit: Science@NASA               More Information       Lunar Impact Monitoring News -- from the NASA Meteoroid Environment Office               International Meteor Organization -- live Orionid meteor counts                       Regards,               Roger              --- D'Bridge 3.64        * Origin: NCS BBS (1:3828/7)    |
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