Hello All!   
      
   Rock Comet Meteor Shower        
      
   Dec. 9, 2012:  Every year in mid-December, astronomers look up in the sky and   
   witness a mystery. It announces itself with a flurry of shooting stars. For   
   several nights in a row, dozens to hundreds of meteors per hour cut across the   
   glistening constellations of winter, each one a little puzzle waiting to be   
   solved.    
      
   "It's the Geminid meteor shower--set to peak on Dec. 13th and 14th," says Bill   
   Cooke of NASA's Meteoroid Environment Office. "Although the Geminids come   
   every year, we still don't fully understand them."    
      
   http://www.youtube.com/watch?v=fEPPGF3KrMQ   
      
   A ScienceCast video explores how a "rock comet" can produce a meteor shower   
   like the Geminids. Play it   
      
   Most meteor showers are caused by icy comets, which spew jets of meteoroids   
   when they are heated by sunlight. The Geminids are different. The parent is   
   not a comet but a weird rocky object named 3200 Phaethon.    
      
   When 3200 Phaethon was discovered in 1983 by NASA's IRAS satellite,   
   astronomers quickly realized that they had found the source of the Geminids.   
   The orbit of 3200 Phaethon was such a close match to that of the Geminid   
   debris stream, no other conclusion was possible. Yet here was a puzzler:   
   Everything about 3200 Phaethon suggests it is an asteroid.    
      
   In fact, 3200 Phaethon resembles main belt asteroid Pallas so much, it could   
   well be a 5-kilometer chip off that 544 km block. "If 3200 Phaethon broke   
   apart from asteroid Pallas, as some researchers believe, then Geminid   
   meteoroids might be debris from the breakup," speculates Cooke.    
      
   There is, however, another possibility: Perhaps 3200 Phaethon is a "rock   
   comet."    
      
   A "rock comet" is a new kind of object being discussed by some astronomers. It   
   is, essentially, an asteroid that comes very close to the sun--so close that   
   solar heating scorches dusty debris right off its rocky surface. Rock comets   
   could thus grow comet-like tails made of gravely debris that produce meteor   
   showers on Earth.    
      
   Could this be the answer?    
      
   http://www2.ess.ucla.edu/~jewitt/papers/2010/JL10.pdf   
      
   The path of 3200 Phaethon through STEREO's HI-1A coronagraph camera.   
   False-color green and blue streamers come from the sun. [more] To test the   
   idea, researchers turned to NASA's twin STEREO spacecraft, which are designed   
   to study solar activity. In June 2009, STEREO watched 3200 Phaethon passing   
   only 15 solar diameters from the sun's surface. What happened next surprised   
   UCLA planetary scientists David Jewitt and Jing Li, who analyzed the data. "    
      
   3200 Phaethon unexpectedly brightened by a factor of two," they wrote. "The   
   most likely explanation is that Phaethon ejected dust, perhaps in response to   
   a break-down of surface rocks (through thermal fracture and decomposition   
   cracking of hydrated minerals) in the intense heat of the Sun."    
      
   So, according to the STEREO observations, 3200 Phaethon does behave like a   
   rock comet.    
      
   The "rock comet" hypothesis is compelling, but Jewett and Li point out a   
   problem: The amount of dust 3200 Phaethon ejected during its sun-encounter   
   added a paltry 0.01% to the mass of the Geminid debris stream, not enough to   
   keep the debris stream stocked up with meteoroids for the annual display of   
   shooting stars.  3200 Phaethon is not spewing enough dust to account for the   
   Geminids.    
      
   Could the rock comet have been more active in the past....? "We just don't   
   know," says Cooke.    
      
   Forecasters expect Geminid meteor rates to top 100 per hour when the shower   
   peaks on the moonless nights of Dec. 13th and 14th, 2012.  Cooke encourages   
   sky watchers to go out, look up, and savor the mystery.    
      
      
   Author: Dr. Tony Phillips| Production editor: Dr. Tony Phillips | Credit:   
   Science@NASA   
      
      
   Regards,   
      
   Roger    
   --- timEd/386 1.10.y2k+   
    * Origin: NCS BBS - Houma, LoUiSiAna - (1:3828/7)