1 00:00:00,000 --> 00:00:04,100 Music 2 00:00:04,120 --> 00:00:08,200 People have been 3 00:00:08,220 --> 00:00:12,320 hunting for sungrazing comets for hundreds of years, but as of 4 00:00:12,340 --> 00:00:16,390 1979 we only knew of less than a dozen. Today, 5 00:00:16,410 --> 00:00:20,500 we have seen about 2,500. Why did the number increase? 6 00:00:20,520 --> 00:00:24,550 Understanding this starts with the Kreutz path. In the 7 00:00:24,570 --> 00:00:28,580 late 1800s, Heinrich Kreutz observed that many recent comets 8 00:00:28,600 --> 00:00:32,760 traveling near the sun appeared to follow the same orbit. On this Kreutz 9 00:00:32,780 --> 00:00:36,820 path, as we've come to call it, it takes the comet about 800 years 10 00:00:36,840 --> 00:00:40,930 to complete one loop around the sun. While there are other orbits of 11 00:00:40,950 --> 00:00:45,040 sungrazers, Kreutz comets are the most common. All of the comets 12 00:00:45,060 --> 00:00:49,120 in this orbit came from a single comet, observed thousands of years ago. 13 00:00:49,140 --> 00:00:53,180 As the comet moved closer to the sun, the ice binding it 14 00:00:53,200 --> 00:00:57,240 together evaporated, breaking it into smaller pieces that the sun's gravity 15 00:00:57,260 --> 00:01:01,309 pulled apart. Every time the comet comes around the Kreutz path, this can 16 00:01:01,330 --> 00:01:05,420 happened again, resulting in a new generation of comets. It might 17 00:01:05,440 --> 00:01:09,530 sound like this would clutter the solar system full of comets, but that is not the case. 18 00:01:09,550 --> 00:01:13,580 Some of the new comets are small enough that they become completely vaporized 19 00:01:13,600 --> 00:01:17,649 as they approach the sun. There are more comets observed, not because 20 00:01:17,670 --> 00:01:21,680 there are more in the solar system but because we have better ways to see them. 21 00:01:21,700 --> 00:01:25,890 Spotting a sungrazer from the ground is difficult because of the blinding sunlight. 22 00:01:25,910 --> 00:01:29,920 Now, spacecraft designed to observe the sun make the job a lot 23 00:01:29,940 --> 00:01:34,120 easier. Since the joint ESA/NASA mission SOHO launched in 1995, 24 00:01:34,140 --> 00:01:38,180 it has shown us thousands more comets than any tool before. 25 00:01:38,200 --> 00:01:42,270 To date, it has found 2,387 comets. 26 00:01:42,290 --> 00:01:46,370 With SOHO we can now see the smaller, fainter comets 27 00:01:46,390 --> 00:01:50,480 close to the sun, just long enough to ad them to our list of sungrazers 28 00:01:50,500 --> 00:01:54,670 before they vaporize. The spacecraft's data is available online, 29 00:01:54,690 --> 00:01:58,700 so now, anyone can discover a comet. Roughly 75% 30 00:01:58,720 --> 00:02:02,789 of these comets have been found by amateur astronomers. 31 00:02:02,810 --> 00:02:06,880 Other solar observatories, such as NASA's SDO, weren't expected to provide 32 00:02:06,900 --> 00:02:10,910 good comet observations, but they captured some beautiful images, creating 33 00:02:10,930 --> 00:02:14,960 more possibilities for comet research using unexpected tools. Now 34 00:02:14,980 --> 00:02:19,019 that we can observe comets better than ever - who knows? - maybe you 35 00:02:19,040 --> 00:02:23,060 will spot the next sungrazer. 36 00:02:23,080 --> 00:02:27,130 beeping 37 00:02:27,150 --> 00:02:31,190 beeping 38 00:02:31,210 --> 00:02:35,220 39 00:02:35,240 --> 00:02:36,480