WEBVTT 00:01.266 --> 00:06.066 position:40% line:84.67% size:50% (MUSIC) 00:06.066 --> 00:07.366 position:17.5% line:84.67% size:72.5% JOAN CARTAN-HANSEN, HOST: 00:07.366 --> 00:08.700 position:12.5% line:84.67% size:77.5% The first astronomers observed 00:08.700 --> 00:09.966 position:15% line:84.67% size:75% comets by watching the night 00:09.966 --> 00:10.900 position:45% line:84.67% size:45% sky. 00:10.900 --> 00:12.233 position:10% line:84.67% size:80% From the ground, they identified 00:12.233 --> 00:14.166 position:12.5% line:84.67% size:77.5% about 900 comets from 1761 to 00:14.166 --> 00:16.233 position:42.5% line:84.67% size:47.5% 1995. 00:16.233 --> 00:17.633 position:17.5% line:84.67% size:72.5% But as it turns out, human 00:17.633 --> 00:19.133 position:10% line:84.67% size:80% scientists are no match for the 00:19.133 --> 00:21.000 position:15% line:84.67% size:75% best comet hunter in space. 00:21.000 --> 00:22.233 position:25% line:84.67% size:65% That's the Solar and 00:22.233 --> 00:24.600 position:10% line:84.67% size:80% Heliospheric Observatory, better 00:24.600 --> 00:25.633 position:30% line:84.67% size:60% known as "SOHO." 00:25.633 --> 00:26.933 position:12.5% line:84.67% size:77.5% It was originally designed to 00:26.933 --> 00:28.300 position:12.5% line:84.67% size:77.5% study the sun, but scientists 00:28.300 --> 00:29.800 position:10% line:84.67% size:80% soon realized it was really good 00:29.800 --> 00:31.066 position:27.5% line:84.67% size:62.5% at finding comets. 00:31.066 --> 00:32.400 position:15% line:84.67% size:75% So far, it's found more than 00:32.400 --> 00:33.500 position:42.5% line:84.67% size:47.5% 3000. 00:33.500 --> 00:35.000 position:10% line:84.67% size:80% But most of the comets its finds 00:35.000 --> 00:36.300 position:32.5% line:84.67% size:57.5% disintegrate. 00:36.300 --> 00:37.666 position:10% line:84.67% size:80% SOHO finds comets that pass very 00:37.666 --> 00:38.866 position:27.5% line:84.67% size:62.5% close to the sun. 00:38.866 --> 00:40.366 position:15% line:84.67% size:75% And those comets just can't 00:40.366 --> 00:41.833 position:15% line:84.67% size:75% handle the intense sunlight. 00:41.833 --> 00:42.866 position:22.5% line:84.67% size:67.5% So, they're destroyed. 00:42.866 --> 00:44.400 position:10% line:84.67% size:80% Astronomers think most of these 00:44.400 --> 00:45.833 position:12.5% line:84.67% size:77.5% comets are fragments of a much 00:45.833 --> 00:47.366 position:12.5% line:84.67% size:77.5% bigger comet that broke apart 00:47.366 --> 00:48.733 position:20% line:84.67% size:70% thousands of years ago. 00:48.733 --> 00:50.000 position:10% line:84.67% size:80% Scientists can learn a lot from 00:50.000 --> 00:51.200 position:27.5% line:84.67% size:62.5% these dying comets. 00:51.200 --> 00:52.566 position:10% line:84.67% size:80% Their tails are pushed around by 00:52.566 --> 00:54.233 position:17.5% line:84.67% size:72.5% the sun's magnetic fields. 00:54.233 --> 00:55.666 position:12.5% line:84.67% size:77.5% So, watching these tails move 00:55.666 --> 00:57.066 position:10% line:84.67% size:80% can tell researchers more about 00:57.066 --> 00:58.933 position:27.5% line:84.67% size:62.5% how the sun works. 00:58.933 --> 01:00.466 position:17.5% line:84.67% size:72.5% For more information about 01:00.466 --> 01:01.800 position:10% line:84.67% size:80% asteroids and comets, check out 01:01.800 --> 01:02.833 position:17.5% line:84.67% size:72.5% the Science Trek website. 01:02.833 --> 01:03.766 position:27.5% line:84.67% size:62.5% You'll find it at 01:03.766 --> 01:04.866 position:30% line:84.67% size:60% ScienceTrek.org