A comet has been spotted disintegrating in the atmosphere of the sun for the first time.
   Such sun-diving comets  are common but none have been seen surviving entry into the sun's  atmosphere until now. They could help reveal what comets are made of and  also uncover hidden properties of the sun's atmosphere, researchers  said today (Jan. 19) as they announced the discovery.
   A group of comets known as the Kreutz family regularly flies perilously close to the sun.
   In the past 15 years, more than 1,400 of these dirty snowballs have  been detected, likely originating from a giant parent comet 20 to 100  kilometers wide (12 to 62 miles) that broke apart as recently as 2,500  years ago. However, until now, none of the telescopes trained on the sun  was sensitive enough to follow any of these comets to their demise in  the sun's atmosphere.
  Using NASA's Solar Dynamics Observatory (SDO), Solar Heliospheric Observatory  (SOHO) and Solar-Terrestrial Relations Observatory (STEREO), scientists  followed the Kreutz comet C/2011 N3 in its mad dash to the sun.
   "It was very surprising to see this comet at all," Karel Schrijver, an astrophysicist at Lockheed Martin Advanced Technology Center  in Palo Alto, Calif., told SPACE.com. "We may think that an object of  some 60,000 metric tons and some 50 meters [164 feet] across is large  and heavy, but if you compare it to the sun, which can easily hold a  million Earths, it is astonishing that such a small object glows  brightly enough to be seen."
   Schrijver is the lead author of the study of the disintegrating comet.  The scientists detail their findings in the Jan. 20 issue of the journal  Science.
  Doomed comet's death dive
   Researchers first detected the comet last July 4, two days before its  destruction. It initially had a tail more than 6,200 miles (10,000  kilometers) long and was diving at the sun at about 1.3 million mph (2.1  million kilometers per hour). During the final 10 minutes of  observations, the comet lost about 1.5 million to 150 million pounds  (700,000 to 70 million kilograms).
   "We've been able to bracket its size as between 30 and 150 feet (9 and  45 meters) long, with a greater likelihood that it lies at the upper end  of that range," Schrijver  said. "And it most likely weighed in at as much as 70,000 tons, giving  it about the weight of an aircraft carrier when it first became  visible."
   On July 6, the comet managed to reach deep into the sun's atmosphere,  about 62,000 miles (100,000 km) from the surface. As it approached that  point, it broke up into many large pieces ranging in size from dust up  to about 150 feet (45 meters) wide. Then it completely vaporized.
  A glimpse inside comets
   As sun-diving comets disintegrate, they could reveal much about how  comets in general are put together and what their components are  scientists say. Since comets date back to the origins of the solar system,  such details about their death throes could lead to a better  understanding of how the planets evolved from protoplanetary gas and  dust.
   The behavior of these comets as they graze the sun also could shed  light on the sun's mysterious high-altitude atmosphere. Scientists  normally are unable to see this part of the sun because its glow is not  bright enough for telescopes, while it is still too close to the sun to  observe with instruments that block out the bright disk of the sun,  Schrijver said.
   Understanding how the sun's atmosphere works could in turn reveal more  about the operations of the sun's roiling surface, which can often burst  with solar flares that affect Earth.
 
