1 00:00:19,990 --> 00:00:17,510 exoplanets are very difficult to detect 2 00:00:25,349 --> 00:00:20,000 because they are tiny little objects 3 00:00:32,389 --> 00:00:28,550 other telescopes are designed to be 4 00:00:35,510 --> 00:00:32,399 better detectors of exoplanets 5 00:00:37,750 --> 00:00:35,520 but what hubble is used for is to find 6 00:00:40,260 --> 00:00:37,760 for some of them the atmospheric 7 00:00:41,510 --> 00:00:40,270 composition of these exoplanets 8 00:00:43,510 --> 00:00:41,520 [Music] 9 00:00:45,830 --> 00:00:43,520 it has to be a system that just by 10 00:00:48,470 --> 00:00:45,840 chance has to be aligned so that the 11 00:00:50,869 --> 00:00:48,480 planet is orbiting its star 12 00:00:56,510 --> 00:00:50,879 along the line of sight of the hubble 13 00:00:59,270 --> 00:00:57,670 [Music] 14 00:01:00,709 --> 00:00:59,280 for doing a lot of the exoplanet 15 00:01:03,189 --> 00:01:00,719 observations you have to catch what's 16 00:01:05,590 --> 00:01:03,199 known as a transit one the orbit of the 17 00:01:07,670 --> 00:01:05,600 exoplanet has to be such that it's going 18 00:01:10,789 --> 00:01:07,680 to go between you and the star it's 19 00:01:14,469 --> 00:01:12,469 and then you have to do the timing we 20 00:01:15,990 --> 00:01:14,479 can't just do an exoplanet observation 21 00:01:18,070 --> 00:01:16,000 whenever we want or whenever it's 22 00:01:20,230 --> 00:01:18,080 convenient we have to do an exoplanet 23 00:01:21,830 --> 00:01:20,240 observation when it's first starting to 24 00:01:23,990 --> 00:01:21,840 go into the star 25 00:01:25,749 --> 00:01:24,000 so they have to know very accurately the 26 00:01:27,270 --> 00:01:25,759 timing of that we have to schedule it 27 00:01:28,870 --> 00:01:27,280 ahead of time this is not something that 28 00:01:31,350 --> 00:01:28,880 you know hubble can get around to when 29 00:01:33,350 --> 00:01:31,360 it wants to we have to say no at this 30 00:01:34,550 --> 00:01:33,360 point in time on this date you have to 31 00:01:38,630 --> 00:01:34,560 be pointed here and you have to be 32 00:01:43,030 --> 00:01:40,550 when that planet passes in front of its 33 00:01:45,270 --> 00:01:43,040 star the starlight some of it is blocked 34 00:01:46,789 --> 00:01:45,280 by the planet but some of it comes 35 00:01:49,270 --> 00:01:46,799 through the outer 36 00:01:51,670 --> 00:01:49,280 ridge the outer rims of the atmosphere 37 00:01:53,190 --> 00:01:51,680 of that planet on its way to the hubble 38 00:01:55,429 --> 00:01:53,200 telescope 39 00:01:57,749 --> 00:01:55,439 some of that light is absorbed by 40 00:02:00,709 --> 00:01:57,759 whatever is in that atmosphere 41 00:02:03,270 --> 00:02:00,719 and it is absorbed at very particular 42 00:02:05,429 --> 00:02:03,280 frequencies that correspond to the atoms 43 00:02:07,590 --> 00:02:05,439 and molecules that are in the atmosphere 44 00:02:09,589 --> 00:02:07,600 of that exoplanet then when the hubble 45 00:02:12,070 --> 00:02:09,599 telescope receives that light and we 46 00:02:13,910 --> 00:02:12,080 take it in usually with a spectrograph 47 00:02:16,229 --> 00:02:13,920 we get the light we spread it out into 48 00:02:18,070 --> 00:02:16,239 its constituent colors or wavelengths of 49 00:02:21,110 --> 00:02:18,080 light and we can tell which of those 50 00:02:24,150 --> 00:02:21,120 wavelengths have been absorbed and that 51 00:02:26,550 --> 00:02:24,160 tells us by the pattern of spectroscopy 52 00:02:28,150 --> 00:02:26,560 what are the elements and molecules that 53 00:02:30,630 --> 00:02:28,160 are found in the atmosphere of that 54 00:02:33,830 --> 00:02:30,640 planet hubble has detected things like 55 00:02:37,190 --> 00:02:33,840 sodium and hydrogen and even evidence of 56 00:02:39,830 --> 00:02:37,200 methane and water vapor by using transit 57 00:02:41,910 --> 00:02:39,840 observations of exoplanets and measuring 58 00:02:43,990 --> 00:02:41,920 not only that composition but also the 59 00:02:45,990 --> 00:02:44,000 height of the atmosphere which can tell 60 00:02:47,430 --> 00:02:46,000 us something about how heavy the 61 00:02:51,270 --> 00:02:47,440 atmosphere is and that tells us 62 00:02:53,509 --> 00:02:51,280 something about its composition as well 63 00:02:55,589 --> 00:02:53,519 hubble was the pioneer in doing that and 64 00:02:57,670 --> 00:02:55,599 now other observatories are also using