1 00:00:07,882 --> 00:00:08,174 We are 2 00:00:08,174 --> 00:00:12,053 looking at a picture of the planet Jupiter taken with the Hubble Space Telescope 3 00:00:12,053 --> 00:00:18,226 in 1994, at a time when the fragments of shattered comet Shoemaker-Levy 9 4 00:00:18,226 --> 00:00:22,897 were pummeling into the planet, leaving huge black impact 5 00:00:22,897 --> 00:00:24,607 sites on the planet. 6 00:00:25,233 --> 00:00:27,193 A bunch of them going in kind of like this. 7 00:00:29,696 --> 00:00:31,614 Prior to Shoemaker-Levy 9, 8 00:00:31,698 --> 00:00:36,077 We had never had the opportunity to prepare 9 00:00:36,077 --> 00:00:39,122 to watch an interplanetary impact 10 00:00:39,122 --> 00:00:40,415 in our solar system. 11 00:00:40,540 --> 00:00:46,046 Isn’t that incredible? That’s amazing. That’s what we all say. 12 00:00:48,840 --> 00:00:50,258 Shoemaker-Levy 9 13 00:00:50,258 --> 00:00:54,637 was a comet that was discovered by Gene and Carolyn 14 00:00:54,637 --> 00:00:56,347 Shoemaker and David Levy, 15 00:01:00,727 --> 00:01:03,813 Which is why it's called Shoemaker-Levy 9. 16 00:01:03,813 --> 00:01:06,107 It was the ninth Comet that team had found. 17 00:01:13,073 --> 00:01:15,492 And what was unusual about Shoemaker-Levy 9 18 00:01:15,492 --> 00:01:19,621 was that it was in orbit around Jupiter. 19 00:01:19,954 --> 00:01:26,294 We believe was captured probably about 70 years earlier, 20 00:01:26,294 --> 00:01:27,921 the late 1920s. 21 00:01:30,006 --> 00:01:32,926 It wasn't just flying through the solar system. 22 00:01:32,926 --> 00:01:35,678 It had, at some point in the past, been captured 23 00:01:35,678 --> 00:01:38,098 by the gravitational field of Jupiter. 24 00:01:38,098 --> 00:01:43,186 And more importantly than that, when the orbit of the comet 25 00:01:43,186 --> 00:01:47,398 was computed, it was discovered that within 26 00:01:47,398 --> 00:01:52,028 about six months this comet was going to hit Jupiter. 27 00:01:52,403 --> 00:01:55,657 We think the reason that Shoemaker-Levy 9 was shattered 28 00:01:55,657 --> 00:02:00,662 into so many fragments was that on its last close pass 29 00:02:00,662 --> 00:02:04,290 while it was orbiting Jupiter, the gravitation was so strong, 30 00:02:04,290 --> 00:02:08,294 the gravity field that it actually caused it to fragment and break up. 31 00:02:15,552 --> 00:02:17,762 I was asked to take all 32 00:02:17,762 --> 00:02:21,432 of the proposals that had been accepted to look at Jupiter 33 00:02:21,432 --> 00:02:24,769 as the comet was hitting it and put them together into one large 34 00:02:24,769 --> 00:02:28,273 observing program, with Hubble so that it could capture 35 00:02:28,356 --> 00:02:31,609 all the full range of what may happen on Jupiter. 36 00:02:31,860 --> 00:02:35,572 Everybody who predicted that we would see something 37 00:02:35,572 --> 00:02:37,323 dramatic was right. 38 00:02:41,369 --> 00:02:44,289 And the Hubble observations were fantastic. 39 00:02:44,539 --> 00:02:50,295 We saw massive explosions, we saw ripples in the atmosphere of Jupiter. 40 00:02:50,461 --> 00:02:54,132 We saw dark material that was processed 41 00:02:54,132 --> 00:02:56,718 by the intense heat of these explosions. 42 00:02:58,636 --> 00:03:02,015 This image of Jupiter, taken by the Hubble Space Telescope, 43 00:03:02,015 --> 00:03:06,352 was one of the most dramatic images from the Shoemaker-Levy 9 week. 44 00:03:06,561 --> 00:03:08,813 It was a week long event. 45 00:03:08,813 --> 00:03:13,818 It took that long for all the fragments of this shattered comet to hit Jupiter. 46 00:03:14,194 --> 00:03:19,532 This particular image is of a particularly large fragment. 47 00:03:19,616 --> 00:03:23,620 It created a massive plume of material 48 00:03:23,703 --> 00:03:27,790 that shot out for thousands of miles above Jupiter's cloud tops. 49 00:03:27,874 --> 00:03:30,835 It took about 20 minutes to rise and then collapsed. 50 00:03:31,044 --> 00:03:34,505 And so the arc that we see in the bottom of this image 51 00:03:34,505 --> 00:03:38,176 is the collapsed material from this gigantic plume. 52 00:03:40,470 --> 00:03:43,223 It was just an amazing 53 00:03:43,223 --> 00:03:48,102 example of the power of collisions in our solar system.