1 00:00:00,020 --> 00:00:04,060 Bell Tone 2 00:00:04,080 --> 00:00:08,190 Bell Tone 3 00:00:08,210 --> 00:00:12,340 Narrator: All the comets that we can see from Earth are orbiting the sun, but some belong to 4 00:00:12,360 --> 00:00:16,520 a special group called sungrazing comets. Sungrazers are comets that 5 00:00:16,540 --> 00:00:20,560 come very close to the sun at their nearest approach, a point called perihelion. 6 00:00:20,580 --> 00:00:24,690 To be considered a sungrazer, a comet needs to get within about 850,000 7 00:00:24,710 --> 00:00:28,860 miles from the sun at perihelion. Many come even closer, 8 00:00:28,880 --> 00:00:32,940 even to within a few thousand miles. Being so close to the sun is very hard 9 00:00:32,960 --> 00:00:37,100 on comets for many reasons. They are subjected to a lot of solar radiation 10 00:00:37,120 --> 00:00:41,280 which boils off their water or other volatiles. The physical push 11 00:00:41,300 --> 00:00:45,450 of the radiation and the solar wind also helps form the tails. And as they get closer 12 00:00:45,470 --> 00:00:49,620 to the sun, the comets experience extremely strong tidal forces, or 13 00:00:49,640 --> 00:00:53,710 gravitational stress. In this hostile environment, many 14 00:00:53,730 --> 00:00:57,870 sungrazers do not survive their trip around the sun. They don't actually crash into the solar 15 00:00:57,890 --> 00:01:01,890 surface, but the sun destroys them anyway. Many sungrazing 16 00:01:01,910 --> 00:01:05,970 comets follow a similar orbit, called the Kreutz Path, and collectively belong to 17 00:01:05,990 --> 00:01:10,000 a population called the Kreutz Group. In fact, close to 18 00:01:10,020 --> 00:01:14,030 85% of the sungrazers seen by the SOHO satellite are on this orbital highway. 19 00:01:14,050 --> 00:01:18,140 Scientists think one extremely large sungrazing comet broke up 20 00:01:18,160 --> 00:01:22,250 hundreds, or even thousands, of years ago, and the current comets on the Kreutz Path 21 00:01:22,270 --> 00:01:26,370 are the leftover fragments of it. As clumps of remnants make their way back around 22 00:01:26,390 --> 00:01:30,560 the sun, we experience a sharp increase in sungrazing comets, which appears 23 00:01:30,580 --> 00:01:34,590 to be going on now. Comet Lovejoy, which reached 24 00:01:34,610 --> 00:01:38,630 perihelion on December 15, 2011 is the best known recent 25 00:01:38,650 --> 00:01:42,820 Kreutz-group sungrazer. And so far, it is the only one that NASA's 26 00:01:42,840 --> 00:01:46,870 solar-observing fleet has seen survive its trip around the sun. Comet 27 00:01:46,890 --> 00:01:50,990 ISON, an upcoming sungrazer with perihelion on November 28, 2013, 28 00:01:51,010 --> 00:01:55,180 is not on the Kreutz Path. In fact, ISON's orbit 29 00:01:55,200 --> 00:01:59,220 suggests that it may gain enough momentum to escape the solar system entirely, and never 30 00:01:59,240 --> 00:02:03,370 return. Before it does so, it will pass within about 40 31 00:02:03,390 --> 00:02:07,400 million miles from Earth on December 26th. Assuming it survives its trip 32 00:02:07,420 --> 00:02:11,460 around the sun. All comets are great laboratories for 33 00:02:11,480 --> 00:02:15,580 scientists to learn more about our solar system, but sungrazing comets can also help us learn 34 00:02:15,600 --> 00:02:19,620 about the sun. Their tails of ionized gas illuminate invisible 35 00:02:19,640 --> 00:02:23,690 magnetic fields, so they can act as a tracer, helping scientists observe these normally 36 00:02:23,710 --> 00:02:27,890 unseeable features. Such fields have even ripped off comet tails, 37 00:02:27,910 --> 00:02:32,030 allowing astronomers to watch them blowing in the solar wind. A wind that 38 00:02:32,050 --> 00:02:36,210 abruptly accelerates between one and five million miles from the sun. 39 00:02:36,230 --> 00:02:40,270 Because of this, researchers will be watching ISON, and other sungrazing comets 40 00:02:40,290 --> 00:02:44,360 very closely. And since we are in a period of high sungrazing comet activity, 41 00:02:44,380 --> 00:02:48,400 scientists can expect many more chances to watch these beautiful, 42 00:02:48,420 --> 00:02:52,510 natural research satellites in the coming years. 43 00:02:52,530 --> 00:02:56,720 Beeping 44 00:02:56,740 --> 00:03:05,832 Beeping