1 00:00:00,010 --> 00:00:06,020 Engine Sound 2 00:00:06,040 --> 00:00:08,040 Engine 3 00:00:12,170 --> 00:00:08,070 Leia: You don't have to do this to impress me. C-3PO: Sir the 4 00:00:12,190 --> 00:00:16,190 asteroid field is approximately 3, 720 to 1. Han: Never tell me the odds. 5 00:00:16,210 --> 00:00:20,230 Narrator: Asteroids collide all the time. 6 00:00:20,250 --> 00:00:24,250 At least, we think they do. Close-up views from spacecraft show asteroids 7 00:00:24,270 --> 00:00:28,310 to be pockmarked with impact craters. But until recently, astronomers 8 00:00:28,330 --> 00:00:32,450 never expected they'd see the recent aftermath of a collision. 9 00:00:32,470 --> 00:00:36,510 Now, thanks to Hubble and Swift, they have. In 10 00:00:36,530 --> 00:00:40,540 early 2010, Hubble took a close look at the tail of what astronomers thought was an unusual 11 00:00:40,560 --> 00:00:44,700 comet. The curious tail turned out to be wreckage from a collision between two 12 00:00:44,720 --> 00:00:48,730 small asteroids. On December 11, 2010, 13 00:00:48,750 --> 00:00:52,770 astronomers saw that another asteroid, (596) Scheila, had also grown a tail. 14 00:00:52,790 --> 00:00:56,830 Swifts ability to see ultraviolet light helped astronomers rule 15 00:00:56,850 --> 00:01:00,870 out the possibility that they were looking at a comet. None of the gasses characteristic 16 00:01:00,890 --> 00:01:04,930 of a comet were detected. These plumes are clouds of dust, 17 00:01:04,950 --> 00:01:08,980 debris from the impact of a smaller asteroid, less than 100 feet across. 18 00:01:09,000 --> 00:01:13,000 The shape, evolution, and content of the plumes let astronomers reconstruct 19 00:01:13,020 --> 00:01:17,080 what happened. 20 00:01:17,100 --> 00:01:21,110 The smaller asteroid would have been heading towards Scheila at about 11,000 miles per 21 00:01:21,130 --> 00:01:22,170 hour. 22 00:01:22,190 --> 00:01:24,210 Music 23 00:01:24,230 --> 00:01:28,290 It hit at a low angle with the force of at least a 100 kiloton nuclear 24 00:01:28,310 --> 00:01:32,470 bomb. Yet much of the debris fell back onto the asteroid. 25 00:01:32,490 --> 00:01:36,500 The particles that escaped were the smallest ones. Easily 26 00:01:36,520 --> 00:01:40,570 pushed around by sunlight, this fine dust formed wispy plumes. 27 00:01:40,590 --> 00:01:44,590 When Hubble observed Scheila two weeks later, the 28 00:01:44,610 --> 00:01:48,620 plumes were barely visible. Within two months of the outburst, 29 00:01:48,640 --> 00:01:52,690 the plumes were completely gone--and with them went any sign from Earth that Scheila even had 30 00:01:52,710 --> 00:01:56,710 a collision. Astronomers estimate that, somewhere in the asteroid 31 00:01:56,730 --> 00:02:00,750 belt, events like this may happen as often as every year. Thanks to Hubble and