1 00:00:10,400 --> 00:00:16,550 hmm 2 00:00:21,189 --> 00:00:18,470 are we alone 3 00:00:24,070 --> 00:00:21,199 that's a question likely asked by anyone 4 00:00:25,429 --> 00:00:24,080 who's ever stared in awe at the bright 5 00:00:28,150 --> 00:00:25,439 night sky 6 00:00:30,710 --> 00:00:28,160 until recently astronomers knew only of 7 00:00:34,549 --> 00:00:30,720 the planets in our solar system 8 00:00:37,350 --> 00:00:34,559 then in 1995 came the discovery of the 9 00:00:38,549 --> 00:00:37,360 first planets orbiting stars other than 10 00:00:41,750 --> 00:00:38,559 our sun 11 00:00:44,389 --> 00:00:41,760 could they like earth harbor life we now 12 00:00:46,709 --> 00:00:44,399 know of over 300 exoplanets planets 13 00:00:49,190 --> 00:00:46,719 around other stars but the ones that 14 00:00:51,590 --> 00:00:49,200 have been found to date fall into 15 00:00:54,069 --> 00:00:51,600 categories that are not very similar to 16 00:00:56,869 --> 00:00:54,079 the solar system with its sophisticated 17 00:00:59,670 --> 00:00:56,879 array of high resolution cameras the 18 00:01:02,630 --> 00:00:59,680 kepler spacecraft is designed to stare 19 00:01:05,590 --> 00:01:02,640 at one region of our milky way galaxy 20 00:01:08,789 --> 00:01:05,600 and capture images of any transits it 21 00:01:11,590 --> 00:01:08,799 sees a transit happens when a planet is 22 00:01:13,590 --> 00:01:11,600 passing in front of the face of its star 23 00:01:16,630 --> 00:01:13,600 it's basically the same idea as when you 24 00:01:18,550 --> 00:01:16,640 see a solar eclipse when that happens 25 00:01:21,030 --> 00:01:18,560 that's the moon passing in from the sun 26 00:01:23,030 --> 00:01:21,040 and having a dramatic decrease on the 27 00:01:25,429 --> 00:01:23,040 brightness that we see of the sun how 28 00:01:28,230 --> 00:01:25,439 much starlight is blocked by a planet's 29 00:01:30,630 --> 00:01:28,240 transit and how often that happens can 30 00:01:33,030 --> 00:01:30,640 tell astronomers the planet's size and 31 00:01:36,870 --> 00:01:33,040 orbit and whether it's in the habitable 32 00:01:39,749 --> 00:01:36,880 zone not too close nor too far away from 33 00:01:42,230 --> 00:01:39,759 its star what we want to determine is 34 00:01:44,550 --> 00:01:42,240 how rare or common is a system like the 35 00:01:46,310 --> 00:01:44,560 earth with a planet like earth in a zone 36 00:01:48,550 --> 00:01:46,320 where you could have liquid water and 37 00:01:50,950 --> 00:01:48,560 potentially life kepler will look 38 00:01:52,950 --> 00:01:50,960 continuously at well over one hundred 39 00:01:56,069 --> 00:01:52,960 thousand stars for at least three and a 40 00:01:58,389 --> 00:01:56,079 half years the data it produces should 41 00:02:01,429 --> 00:01:58,399 be a significant step in learning 42 00:02:04,149 --> 00:02:01,439 whether we've got company in our galaxy 43 00:02:06,469 --> 00:02:04,159 and tell astronomers where best to focus 44 00:02:08,869 --> 00:02:06,479 the search for neighbors it's like when 45 00:02:11,029 --> 00:02:08,879 galileo first turned his telescope to 46 00:02:12,630 --> 00:02:11,039 the heavens and everything changed the 47 00:02:14,229 --> 00:02:12,640 way we thought of ourselves and the 48 00:02:16,229 --> 00:02:14,239 universe changed and the same thing 49 00:02:17,910 --> 00:02:16,239 happened when the apollo astronauts took 50 00:02:19,190 --> 00:02:17,920 that picture of the earth when they were 51 00:02:20,630 --> 00:02:19,200 around the moon you know everyone on 52 00:02:22,309 --> 00:02:20,640 earth could see the earth differently 53 00:02:24,150 --> 00:02:22,319 from that moment on i think we'll have 54 00:02:25,750 --> 00:02:24,160 the same kind of revolution in the way 55 00:02:27,430 --> 00:02:25,760 we think of 56 00:02:29,910 --> 00:02:27,440 our solar system and our existence when 57 00:02:31,830 --> 00:02:29,920 we know how special or how common we 58 00:02:35,110 --> 00:02:31,840 really are for more on the kepler