1 00:00:06,230 --> 00:00:03,990 to observe with hubble we actually have 2 00:00:08,310 --> 00:00:06,240 to plan out pretty far in advance and 3 00:00:10,390 --> 00:00:08,320 for the outer planets what we do is we 4 00:00:12,390 --> 00:00:10,400 pick the time when they're at opposition 5 00:00:14,150 --> 00:00:12,400 and that means that it's opposite from 6 00:00:15,669 --> 00:00:14,160 the sun from the earth's point of view 7 00:00:17,670 --> 00:00:15,679 and that basically gives us the highest 8 00:00:19,429 --> 00:00:17,680 resolution view that's when hubble is 9 00:00:21,670 --> 00:00:19,439 the closest to each planet even though 10 00:00:22,790 --> 00:00:21,680 that doesn't vary much over a year and 11 00:00:25,109 --> 00:00:22,800 the planets are a little bit more 12 00:00:27,349 --> 00:00:25,119 challenging because they move and so 13 00:00:28,790 --> 00:00:27,359 hubble has to find guide stars first 14 00:00:30,790 --> 00:00:28,800 that tell it where it's pointing in the 15 00:00:32,630 --> 00:00:30,800 sky but then it has to track those 16 00:00:34,630 --> 00:00:32,640 planets so it has to move following the 17 00:00:36,229 --> 00:00:34,640 planet across the sky and so that has to 18 00:00:37,830 --> 00:00:36,239 be interleaved with all the other 19 00:00:39,750 --> 00:00:37,840 science program hubble's doing every 20 00:00:41,750 --> 00:00:39,760 single day and so it's very carefully 21 00:00:43,590 --> 00:00:41,760 coordinated to fit in as hubble then 22 00:00:45,190 --> 00:00:43,600 orbits around the earth and so it gets 23 00:00:47,670 --> 00:00:45,200 planned out down to the minutes of 24 00:00:49,510 --> 00:00:47,680 exactly which image we're going to take 25 00:00:52,790 --> 00:00:49,520 in which filter for each of those 26 00:00:56,709 --> 00:00:54,950 so it's a cosmic dance of getting hubble 27 00:00:58,549 --> 00:00:56,719 pointed in the right place moving in the 28 00:01:01,610 --> 00:00:58,559 right direction and tracking all at the 29 00:01:06,230 --> 00:01:03,590 [Applause] 30 00:01:08,630 --> 00:01:06,240 the opal project or the outer planet's 31 00:01:10,469 --> 00:01:08,640 atmosphere's legacy program is an 32 00:01:12,950 --> 00:01:10,479 observational program using the hubble 33 00:01:14,310 --> 00:01:12,960 space telescope and what we're doing is 34 00:01:16,390 --> 00:01:14,320 we're looking at each of the outer 35 00:01:18,550 --> 00:01:16,400 planets every year so that we can build 36 00:01:20,390 --> 00:01:18,560 up a time base using the exact same 37 00:01:22,390 --> 00:01:20,400 facility and the same instruments so we 38 00:01:30,789 --> 00:01:22,400 can actually track what's changing over 39 00:01:35,670 --> 00:01:34,230 it started really with jupiter 40 00:01:37,670 --> 00:01:35,680 in essence we were trying to look at the 41 00:01:38,950 --> 00:01:37,680 weather on jupiter 42 00:01:40,789 --> 00:01:38,960 and as we're trying to understand 43 00:01:42,630 --> 00:01:40,799 whether we know even here on earth it 44 00:01:43,590 --> 00:01:42,640 changes every minute every hour every 45 00:01:44,950 --> 00:01:43,600 day 46 00:01:46,789 --> 00:01:44,960 and we didn't have that kind of time 47 00:01:48,550 --> 00:01:46,799 coverage but we also didn't even have 48 00:01:50,469 --> 00:01:48,560 long time coverage to look at things 49 00:01:52,149 --> 00:01:50,479 that changed over seasons and so we had 50 00:01:53,749 --> 00:01:52,159 this big gap in our knowledge where we 51 00:01:55,670 --> 00:01:53,759 just weren't getting frequent enough 52 00:01:58,630 --> 00:01:55,680 data to be able to trend any of these 53 00:02:00,870 --> 00:01:58,640 things and the idea kind of came about 54 00:02:03,510 --> 00:02:00,880 to look at a legacy program where we 55 00:02:05,990 --> 00:02:03,520 built up a legacy for hubble within the 56 00:02:07,510 --> 00:02:06,000 planetary community and in 2014 we 57 00:02:08,790 --> 00:02:07,520 started with our first observations of 58 00:02:10,710 --> 00:02:08,800 uranus 59 00:02:12,949 --> 00:02:10,720 and the first thing i think we noticed 60 00:02:15,270 --> 00:02:12,959 was uranus had a very prominent polar 61 00:02:17,270 --> 00:02:15,280 cap it was very much brighter and 62 00:02:18,470 --> 00:02:17,280 getting brighter over time we've watched 63 00:02:19,670 --> 00:02:18,480 it over the last few years get much 64 00:02:21,350 --> 00:02:19,680 brighter 65 00:02:23,190 --> 00:02:21,360 neptune on the other hand has been 66 00:02:24,869 --> 00:02:23,200 really quite interesting the first thing 67 00:02:26,550 --> 00:02:24,879 we noted was it had a lot of bright 68 00:02:28,229 --> 00:02:26,560 white clouds and they were coming and 69 00:02:29,300 --> 00:02:28,239 going pretty rapidly at a lot of 70 00:02:31,910 --> 00:02:29,310 different latitudes 71 00:02:34,229 --> 00:02:31,920 [Music] 72 00:02:36,390 --> 00:02:34,239 and so when we start looking at neptune 73 00:02:38,390 --> 00:02:36,400 and uranus as dynamic planets with 74 00:02:40,550 --> 00:02:38,400 changing atmospheres weather like we 75 00:02:42,150 --> 00:02:40,560 know now for jupiter and saturn 76 00:02:46,710 --> 00:02:42,160 we realize that we have a lot of gaps in 77 00:02:50,869 --> 00:02:48,869 and so we've been able to use the opel 78 00:02:52,550 --> 00:02:50,879 program to track how much cloud cover we 79 00:02:53,830 --> 00:02:52,560 have from year to year but the other 80 00:02:55,750 --> 00:02:53,840 thing we can do with hubble that we 81 00:02:57,190 --> 00:02:55,760 can't really do any other way is look 82 00:02:59,830 --> 00:02:57,200 for dark spots 83 00:03:01,910 --> 00:02:59,840 and so the great dark spot was this big 84 00:03:03,670 --> 00:03:01,920 iconic feature we saw with voyager and 85 00:03:05,190 --> 00:03:03,680 when we looked again a few years later 86 00:03:06,949 --> 00:03:05,200 finally when hubble was online it was 87 00:03:08,869 --> 00:03:06,959 gone 88 00:03:10,550 --> 00:03:08,879 and that kind of surprised us because we 89 00:03:12,869 --> 00:03:10,560 were used to the great red spot which 90 00:03:14,230 --> 00:03:12,879 doesn't go away it's changed over time 91 00:03:15,830 --> 00:03:14,240 but it's still there 92 00:03:17,430 --> 00:03:15,840 [Music] 93 00:03:19,110 --> 00:03:17,440 and so these storms are not quite the 94 00:03:21,190 --> 00:03:19,120 same as what we see on jupiter because 95 00:03:23,750 --> 00:03:21,200 they form and go away on much more rapid 96 00:03:25,509 --> 00:03:23,760 time scales 97 00:03:27,589 --> 00:03:25,519 the latest image of neptune is really 98 00:03:29,030 --> 00:03:27,599 interesting to me because we don't see 99 00:03:30,789 --> 00:03:29,040 those bright weight clouds we've been 100 00:03:32,390 --> 00:03:30,799 seeing the last few years as a matter of 101 00:03:34,630 --> 00:03:32,400 fact the only thing we see in that 102 00:03:36,710 --> 00:03:34,640 particular image is this great dark spot 103 00:03:38,630 --> 00:03:36,720 and so in a lot of ways it brings us 104 00:03:41,430 --> 00:03:38,640 around full circle because this looks so 105 00:03:43,670 --> 00:03:41,440 much like the voyager image from 1989 106 00:03:45,350 --> 00:03:43,680 and that was pretty surprising to me not 107 00:03:48,470 --> 00:03:45,360 to see as much cloud activity as we've 108 00:03:50,149 --> 00:03:48,480 been seeing in previous years 109 00:03:52,550 --> 00:03:50,159 the opal team's actually a fairly small 110 00:03:54,149 --> 00:03:52,560 team there's only three of us but our 111 00:03:55,589 --> 00:03:54,159 data is immediately available to the 112 00:03:57,910 --> 00:03:55,599 public and any other scientist that 113 00:04:01,110 --> 00:03:57,920 wants to use them and so we do that as 114 00:04:03,270 --> 00:04:01,120 well as our own scientific analysis 115 00:04:05,270 --> 00:04:03,280 i think having so much hubble data now 116 00:04:06,949 --> 00:04:05,280 there's just so much in there to study 117 00:04:09,030 --> 00:04:06,959 and you know as a scientist that's what 118 00:04:11,270 --> 00:04:09,040 drives us is trying to solve mysteries 119 00:04:13,509 --> 00:04:11,280 trying to look for new mysteries and so 120 00:04:15,429 --> 00:04:13,519 having these long-term data sets with 121 00:04:17,030 --> 00:04:15,439 just such rich numbers of features in 122 00:04:18,789 --> 00:04:17,040 there there's always something to go 123 00:04:20,469 --> 00:04:18,799 look at and it's certainly going to keep 124 00:04:24,310 --> 00:04:20,479 us busy for years to come even when