1 00:00:00,120 --> 00:00:18,950 [Music] 2 00:00:24,070 --> 00:00:21,830 the trojan asteroids are small bodies in 3 00:00:27,189 --> 00:00:24,080 our solar system they share it in orbit 4 00:00:29,830 --> 00:00:27,199 with jupiter there's two swarms of them 5 00:00:31,910 --> 00:00:29,840 one located 60 degrees ahead of jupiter 6 00:00:34,630 --> 00:00:31,920 in its orbit and the other swarm is 7 00:00:37,590 --> 00:00:34,640 located 60 degrees behind jupiter in its 8 00:00:39,910 --> 00:00:37,600 orbit and these trojan asteroids are 9 00:00:42,069 --> 00:00:39,920 remnants from planetary formation so 10 00:00:44,630 --> 00:00:42,079 sometimes we'll call them the fossils of 11 00:00:46,790 --> 00:00:44,640 solar system formation their near 12 00:00:49,670 --> 00:00:46,800 neighbors might have gone into forming 13 00:00:52,389 --> 00:00:49,680 the giant planets and so these objects 14 00:00:55,029 --> 00:00:52,399 then became captured in their locations 15 00:00:58,229 --> 00:00:55,039 today and so in that way we can look and 16 00:01:00,229 --> 00:00:58,239 see what went into forming the planets 17 00:01:02,790 --> 00:01:00,239 in our solar system the main goal of the 18 00:01:05,590 --> 00:01:02,800 lucy mission is to explore the trojan 19 00:01:08,710 --> 00:01:05,600 asteroids we want to understand where 20 00:01:10,789 --> 00:01:08,720 these asteroids came from and why 21 00:01:13,510 --> 00:01:10,799 they're so diverse this is going to be 22 00:01:15,830 --> 00:01:13,520 our first ever exploration of these 23 00:01:18,230 --> 00:01:15,840 objects from the earth 24 00:01:20,390 --> 00:01:18,240 we can see certain features on the 25 00:01:23,190 --> 00:01:20,400 trojan asteroids we can see where 26 00:01:25,429 --> 00:01:23,200 they're located we can see their colors 27 00:01:27,830 --> 00:01:25,439 and we can get spectra 28 00:01:31,270 --> 00:01:27,840 spectra can tell you about the surface 29 00:01:33,270 --> 00:01:31,280 composition a spectrum is when you take 30 00:01:34,950 --> 00:01:33,280 light and spread it out into all its 31 00:01:36,710 --> 00:01:34,960 different wavelengths and so you have 32 00:01:39,109 --> 00:01:36,720 the brightness of the light as a 33 00:01:41,109 --> 00:01:39,119 function of wavelength so think of it 34 00:01:44,310 --> 00:01:41,119 like a rainbow but you're going to 35 00:01:47,590 --> 00:01:44,320 divide up the colors even more finely 36 00:01:49,429 --> 00:01:47,600 than just roy g biv from earth the 37 00:01:51,270 --> 00:01:49,439 trojan asteroids are just a point of 38 00:01:53,429 --> 00:01:51,280 light and you can't 39 00:01:56,789 --> 00:01:53,439 tell one part of the trojan asteroid 40 00:01:58,950 --> 00:01:56,799 composition versus another part and lucy 41 00:02:01,429 --> 00:01:58,960 is going to be able to get that detail 42 00:02:03,749 --> 00:02:01,439 close up but we'll be able to do that by 43 00:02:05,670 --> 00:02:03,759 taking this spacecraft and these 44 00:02:07,749 --> 00:02:05,680 instruments to the trojan asteroids and 45 00:02:10,070 --> 00:02:07,759 we'll be able to see how the surface 46 00:02:11,190 --> 00:02:10,080 composition varies across the trojan 47 00:02:14,470 --> 00:02:11,200 asteroids 48 00:02:17,350 --> 00:02:14,480 additionally we have really large solar 49 00:02:19,670 --> 00:02:17,360 arrays because we are solar-powered 50 00:02:21,750 --> 00:02:19,680 spacecraft the spacecraft gets its power 51 00:02:23,830 --> 00:02:21,760 from the sun at the trojan asteroids 52 00:02:26,470 --> 00:02:23,840 we're more than five times further from 53 00:02:29,030 --> 00:02:26,480 the sun than earth is so there's much 54 00:02:31,589 --> 00:02:29,040 less light we need large solar arrays to 55 00:02:32,309 --> 00:02:31,599 power our spacecraft and in fact we will 56 00:02:35,589 --> 00:02:32,319 be 57 00:02:37,670 --> 00:02:35,599 the furthest operating spacecraft