1 00:00:15,160 --> 00:00:20,270 From the John Hopkins Applied Physics Laboratory in Laurel Maryland, welcome to NASA's New 2 00:00:20,270 --> 00:00:21,930 Horizons countdown to Pluto. 3 00:00:21,930 --> 00:00:26,220 I'm Mike Buckley from APL Communications and Public Affairs, with the latest update from 4 00:00:26,220 --> 00:00:27,520 Pluto's doorstep. 5 00:00:27,520 --> 00:00:33,410 As we countdown to New Horizons historic flyby of the Pluto system on July 14th, we're 14 6 00:00:33,410 --> 00:00:38,900 days away from the Pluto flyby, just two weeks and only 10 million miles from Pluto. 7 00:00:38,900 --> 00:00:42,680 All the activities the team has practiced for years are happening for real. 8 00:00:42,680 --> 00:00:47,560 Now let's check in on some of those activities with an operations update. 9 00:00:47,560 --> 00:00:57,710 Now we get to say hello again to Alice Bowman, the New Horizons Mission operations manager. 10 00:00:57,710 --> 00:01:01,890 Alice, thank you for stepping away from the console for a few minutes to join us in the 11 00:01:01,890 --> 00:01:02,890 show. 12 00:01:02,890 --> 00:01:03,890 Sure. 13 00:01:03,890 --> 00:01:04,890 It's nice to be here. 14 00:01:04,890 --> 00:01:06,020 We know that activity is picking up. 15 00:01:06,020 --> 00:01:07,020 Right? 16 00:01:07,020 --> 00:01:11,220 Can you give us an idea from the operations team, what's happening that indicates that 17 00:01:11,220 --> 00:01:13,200 we're really close to the flyby? 18 00:01:13,200 --> 00:01:14,200 Right. 19 00:01:14,200 --> 00:01:19,490 So, if you've been looking at the pictures on the Web site, you can see that Pluto and 20 00:01:19,490 --> 00:01:25,440 Charon are becoming more distinct, and their surface features, it's getting pretty exciting. 21 00:01:25,440 --> 00:01:29,190 And every day is bringing new features into light. 22 00:01:29,190 --> 00:01:34,030 From the missions operations point of view we've just transitioned to a set of commands 23 00:01:34,030 --> 00:01:37,580 that we actually started planning in 2011. 24 00:01:37,580 --> 00:01:40,970 This is called the approach phase 3. 25 00:01:40,970 --> 00:01:45,170 And this current command set will get us to July 3rd. 26 00:01:45,170 --> 00:01:48,850 So, these are commands that are sent to the spacecraft's computer that essentially tells 27 00:01:48,850 --> 00:01:51,290 it what to do for a set period of time? 28 00:01:53,290 --> 00:01:52,290 Yes. 29 00:01:53,290 --> 00:01:57,280 You mentioned planning something for years in advance, again, in this case 2011 for the 30 00:01:57,280 --> 00:01:59,090 load that's up on the computers now. 31 00:01:59,090 --> 00:02:03,789 I guess it really indicates this is not as simple as just writing a few lines of code 32 00:02:03,789 --> 00:02:05,110 and hitting a send button? 33 00:02:05,110 --> 00:02:09,479 I mean especially for something like, you know, this is a one shot deal, if things have 34 00:02:09,479 --> 00:02:10,479 to work. 35 00:02:10,479 --> 00:02:14,530 Take us through how you actually plan and design commands that go to the spacecraft? 36 00:02:14,530 --> 00:02:15,530 Sure. 37 00:02:15,530 --> 00:02:22,000 So, the science team has a set of observations that they want to accomplish. 38 00:02:22,000 --> 00:02:27,590 There's many of those that happen at closest approach, which is of course July 14th, but 39 00:02:27,590 --> 00:02:32,200 there are also many that happen on this approach phase. 40 00:02:32,200 --> 00:02:36,540 And the most intense observations are starting right now. 41 00:02:36,540 --> 00:02:41,230 Not that it hasn’t been intense but, you know, a lot of the group one and two observations 42 00:02:41,230 --> 00:02:43,380 are really gearing up right now. 43 00:02:43,380 --> 00:02:50,390 So, to build a command set that goes to the spacecraft involves the science team, the 44 00:02:50,390 --> 00:02:55,450 guidance and control team, the mission design team, the navigation team, the mission operations 45 00:02:55,450 --> 00:02:59,400 team, the instrument analysis, all those people. 46 00:02:59,400 --> 00:03:05,680 And so, it starts with the science team really defining what kind of observations they want. 47 00:03:05,680 --> 00:03:12,880 And then they--mission operations knows how to operate the spacecraft, what kind of constraints 48 00:03:12,880 --> 00:03:14,910 you have to take into account. 49 00:03:14,910 --> 00:03:19,080 We'll talk with the guidance and control, and so this is really like a dance. 50 00:03:19,080 --> 00:03:25,370 You have to have all those observations intertwined with the spacecraft commands. 51 00:03:25,370 --> 00:03:31,030 And again, we can't just take science, we have to turn and look to Earth, and communicate 52 00:03:31,030 --> 00:03:34,690 with Earth, and bring back that science data. 53 00:03:34,690 --> 00:03:41,380 So, it's kind of a push and pull, like where you take science and where you turn back and 54 00:03:41,380 --> 00:03:42,640 communicate with Earth. 55 00:03:42,640 --> 00:03:47,250 And then of course, you mentioned communications, and communications are critical, you know, 56 00:03:47,250 --> 00:03:48,450 for these operations. 57 00:03:48,450 --> 00:03:52,910 And that's the connection between New Horizons and NASA's deep space network. 58 00:03:52,910 --> 00:03:58,300 So, maybe remind us a bit, how long is the one way time for a signal to reach Earth from 59 00:03:58,300 --> 00:03:59,300 the spacecraft? 60 00:03:59,300 --> 00:04:03,420 One way time is about four and a half hours. 61 00:04:03,420 --> 00:04:08,270 Explain how you stay in touch with the spacecraft over such long periods of time? 62 00:04:08,270 --> 00:04:16,959 So, there are three DSM complexes; Madrid Spain, Canberra Australia, and Goldstone California. 63 00:04:16,959 --> 00:04:23,770 And so if you think of the path our spacecraft New Horizons is travelling, it's going straight 64 00:04:23,770 --> 00:04:26,479 out to Earth, right toward Pluto. 65 00:04:26,479 --> 00:04:32,740 And the Earth on the other hand is rotating, you know, once every 24 hours. 66 00:04:32,740 --> 00:04:38,660 And as those different complexes come into view, you can use those antennas, those spots 67 00:04:38,660 --> 00:04:43,880 on Earth to communicate with the one that's in view of the spacecraft. 68 00:04:43,880 --> 00:04:48,950 Now I point out that people can follow that coverage online through DSN Now, the NASA 69 00:04:48,950 --> 00:04:53,970 Web site that allows people to see when each deep space network antenna is either talking 70 00:04:53,970 --> 00:04:57,830 to or listening to any spacecraft anywhere. 71 00:04:57,830 --> 00:05:02,680 If I went to that Web site and checked New Horizons I might see one or two of those antenna 72 00:05:02,680 --> 00:05:05,040 stations talking to the spacecraft? 73 00:05:05,040 --> 00:05:06,040 Yes. 74 00:05:06,040 --> 00:05:10,419 You'll see us communicating with the spacecraft when the spacecraft's not taking science. 75 00:05:10,419 --> 00:05:17,340 And so, there's usually about three or four hours there in a period of maybe 12 hours 76 00:05:17,340 --> 00:05:20,010 where we aren’t in communication with the spacecraft. 77 00:05:20,010 --> 00:05:22,410 But there are also some busier periods too. 78 00:05:22,410 --> 00:05:23,410 Right? 79 00:05:23,410 --> 00:05:26,540 During the flyby I think much of the deep space network is going to be focused on New 80 00:05:26,540 --> 00:05:27,540 Horizons. 81 00:05:27,540 --> 00:05:28,540 Tell us about that. 82 00:05:28,540 --> 00:05:29,540 Yeah. 83 00:05:29,540 --> 00:05:30,540 It's going to be pretty interesting. 84 00:05:30,540 --> 00:05:35,600 We have the radio science experiment and what we do there is we uplink signal to the radio 85 00:05:35,600 --> 00:05:42,210 science experiment and it will collect data, like form scan or occultation data. 86 00:05:42,210 --> 00:05:48,111 So, when you--if you were to go to that DSN site and look at those antennas, there's a 87 00:05:48,111 --> 00:05:50,900 total of 13 antennas. 88 00:05:50,900 --> 00:05:56,230 And four and a half hours before closest approach you'll see that New Horizons will be using 89 00:05:56,230 --> 00:05:58,550 seven of those 13 antennas. 90 00:05:58,550 --> 00:06:00,210 A busy day, a busy morning. 91 00:06:00,210 --> 00:06:01,210 Yes. 92 00:06:01,210 --> 00:06:02,210 Definitely. 93 00:06:02,210 --> 00:06:05,490 And I'm not even sure there's been any other spacecraft that has actually used that many 94 00:06:05,490 --> 00:06:06,610 at one time. 95 00:06:06,610 --> 00:06:10,729 Well then speaking of busy, what's next for the operations team over the next week or 96 00:06:10,729 --> 00:06:11,729 so? 97 00:06:11,729 --> 00:06:16,650 Well we're going to be putting up the flyby sequence on board the spacecraft in the next 98 00:06:16,650 --> 00:06:21,290 couple of days, to both the primary and the backup computers. 99 00:06:21,290 --> 00:06:25,880 There's a possibility that we will be doing a trajectory correction maneuver, and of course, 100 00:06:25,880 --> 00:06:33,190 getting down lots of science data, optical navigation data, so it's going to be great. 101 00:06:33,190 --> 00:06:35,110 Well thanks Alice. 102 00:06:35,110 --> 00:06:45,070 All right, now let's get a science update. 103 00:06:45,070 --> 00:06:49,020 We managed to pull Deputy Project Scientist Cathy Olkin away from the images just long 104 00:06:49,020 --> 00:06:53,430 enough to tell us about some of the amazing views New Horizons is getting of Pluto and 105 00:06:53,430 --> 00:06:54,430 its moons. 106 00:06:54,430 --> 00:06:55,699 So, Cathy thanks for joining us again. 107 00:06:55,699 --> 00:06:57,630 Happy to be here. 108 00:06:57,630 --> 00:06:59,680 Our view of Pluto is changing dramatically. 109 00:06:59,680 --> 00:07:00,680 Right? 110 00:07:00,680 --> 00:07:04,110 So, kind of--what are we seeing now that we weren’t able to see a week or even two weeks 111 00:07:04,110 --> 00:07:05,110 ago? 112 00:07:05,110 --> 00:07:06,110 Yeah. 113 00:07:06,110 --> 00:07:09,850 There's features on Pluto that we were starting to see before, and they're coming in to sharper 114 00:07:09,850 --> 00:07:11,540 and sharper focus. 115 00:07:11,540 --> 00:07:14,820 We see a bright region on Pluto's North Pole. 116 00:07:14,820 --> 00:07:16,960 So, it might be a polar cap. 117 00:07:16,960 --> 00:07:20,360 We're looking to get closer and investigate that further. 118 00:07:20,360 --> 00:07:26,680 We're seeing detailed images of the closest approach hemisphere we can look every time 119 00:07:26,680 --> 00:07:30,570 it comes into view is Pluto rotates every six point four days. 120 00:07:30,570 --> 00:07:35,270 And you can see it getting larger and larger and there's dark regions and bright regions, 121 00:07:35,270 --> 00:07:37,290 and it's going to be really exciting. 122 00:07:37,290 --> 00:07:39,340 I mean--and that's the one we're going to see close up to. 123 00:07:39,340 --> 00:07:43,340 So, it's just enough of a tease to get a preview of what you're going to see when you get close 124 00:07:43,340 --> 00:07:44,340 enough. 125 00:07:44,340 --> 00:07:45,340 That's right. 126 00:07:45,340 --> 00:07:49,259 The science team spent a lot of time looking at when to flyby Pluto, which involved, which 127 00:07:49,259 --> 00:07:51,920 hemisphere we would be seeing at closest approach. 128 00:07:51,920 --> 00:07:55,710 And we're all really excited that we choose this hemisphere, because it ends up being 129 00:07:55,710 --> 00:07:57,009 really exciting. 130 00:07:57,009 --> 00:08:01,020 Now, also starting to see details on Charon for the first time. 131 00:08:01,020 --> 00:08:02,020 That's right. 132 00:08:02,020 --> 00:08:03,020 It's very exciting. 133 00:08:03,020 --> 00:08:09,169 We're seeing details on Charon we see a dark region and Charon pole, which is surprising 134 00:08:09,169 --> 00:08:11,520 to me. 135 00:08:11,520 --> 00:08:17,650 A lot of times on Polar Regions you see bright features like we do on Pluto, and Mars, and 136 00:08:17,650 --> 00:08:22,800 Earth, where you have a bright polar cap, but this region is dark compared to the rest 137 00:08:22,800 --> 00:08:23,800 of the surface. 138 00:08:23,800 --> 00:08:25,380 And so it's very tantalizing. 139 00:08:25,380 --> 00:08:28,509 And just waiting to get closer and see more about it. 140 00:08:28,509 --> 00:08:29,509 Right. 141 00:08:29,509 --> 00:08:30,509 Another mystery to solve. 142 00:08:30,509 --> 00:08:31,509 That's right. 143 00:08:31,509 --> 00:08:33,509 It's happening here too, something a little closer to your heart, because you work on 144 00:08:33,509 --> 00:08:34,599 this instrument. 145 00:08:34,599 --> 00:08:39,700 The Ralph Camera actually got some color readings of Pluto and Charon recently. 146 00:08:39,700 --> 00:08:42,339 And from those we got our first New Horizons color movie. 147 00:08:42,339 --> 00:08:43,339 Yeah. 148 00:08:43,339 --> 00:08:47,050 Tell us a little bit about what was in those that we learned about Pluto and Charon that 149 00:08:47,050 --> 00:08:48,560 we had some color views. 150 00:08:48,560 --> 00:08:49,560 That's right. 151 00:08:49,560 --> 00:08:54,740 So, there's a--we have a color movie of Pluto and Charon, and in it you can see that Pluto 152 00:08:54,740 --> 00:08:56,800 is distinctly red compared to Charon. 153 00:08:56,800 --> 00:08:59,009 Charon is more of a gray color. 154 00:08:59,009 --> 00:09:04,931 And you can see as Pluto and Charon are both rotating that Pluto is more red on all the 155 00:09:04,931 --> 00:09:07,850 faces compared to Charon being gray. 156 00:09:07,850 --> 00:09:13,769 And so, this confirms what we knew from ground based observing, but it's giving us more and 157 00:09:13,769 --> 00:09:15,720 more detail as we get closer and closer. 158 00:09:15,720 --> 00:09:17,720 And plus it's just cool to see color. 159 00:09:17,720 --> 00:09:19,379 It's really exciting to see color. 160 00:09:21,379 --> 00:09:20,379 Yeah. 161 00:09:21,379 --> 00:09:22,379 Are they true colors? 162 00:09:22,379 --> 00:09:23,379 In what we saw. 163 00:09:23,379 --> 00:09:24,379 They are true colors. 164 00:09:24,379 --> 00:09:27,939 We worked really hard to try and make them as close to true color that the eye would 165 00:09:27,939 --> 00:09:28,939 see. 166 00:09:28,939 --> 00:09:31,379 So, that is a true color movie. 167 00:09:31,379 --> 00:09:33,230 So it's defiantly a busy time. 168 00:09:33,230 --> 00:09:35,629 The science team getting closer to Pluto. 169 00:09:35,629 --> 00:09:39,230 What activities are on tap for the next week or two, leading up to flyby? 170 00:09:39,230 --> 00:09:42,819 There are so many different activities coming up this week. 171 00:09:42,819 --> 00:09:48,389 We have observation of Pluto and Charon continuing as they get larger and larger, we get closer 172 00:09:48,389 --> 00:09:49,490 and closer. 173 00:09:49,490 --> 00:09:55,240 We've got photometry of the small satellites of Pluto, we've got color images. 174 00:09:55,240 --> 00:09:57,050 We've got infrared images. 175 00:09:57,050 --> 00:09:59,649 The plasma sweep is busy doing its thing. 176 00:09:59,649 --> 00:10:01,149 It's a very exciting time. 177 00:10:01,149 --> 00:10:02,149 It sounds like it. 178 00:10:02,149 --> 00:10:03,300 Well, Cathy thanks again for joining us. 179 00:10:03,300 --> 00:10:04,300 Thank you. 180 00:10:04,300 --> 00:10:09,269 You know, it's probably safe to say that every member of the New Horizons science team loves 181 00:10:09,269 --> 00:10:11,100 Pluto, but probably for different reasons. 182 00:10:11,100 --> 00:10:32,189 So, let's hear from another one, the real Plutophile. 183 00:10:32,189 --> 00:10:36,119 I'm Fran Bagenal I'm at the University of Colorado in Boulder. 184 00:10:36,119 --> 00:10:43,199 Back in oh, about late 1989 or so, there was a bunch of us who were really keen to go to 185 00:10:43,199 --> 00:10:44,199 Pluto. 186 00:10:44,199 --> 00:10:47,810 We wanted to have a mission that would get out there and make observations of this object 187 00:10:47,810 --> 00:10:49,929 right on the edge of the solar system. 188 00:10:49,929 --> 00:10:55,209 So, we realized to make this happen we had to get together and campaign hard to make 189 00:10:55,209 --> 00:10:57,181 the case, to go there and explore. 190 00:10:57,181 --> 00:11:02,209 So, it was a bit of an opportunity for young people to come in and say, hey where are we 191 00:11:02,209 --> 00:11:03,230 going to go next. 192 00:11:03,230 --> 00:11:06,980 What's the next great frontier that we should go explore? 193 00:11:06,980 --> 00:11:08,119 And it was clear. 194 00:11:08,119 --> 00:11:10,069 Out to the Kuiper Belt. 195 00:11:10,069 --> 00:11:14,149 Pluto is a very exciting place, it's right at the edge of the solar system. 196 00:11:14,149 --> 00:11:19,079 We've got a bunch of junk out there, and we don’t know why it is there. 197 00:11:19,079 --> 00:11:23,559 And current ideas are that it got there through the formation of the solar system. 198 00:11:23,559 --> 00:11:27,259 And there's Pluto out there representing that junk. 199 00:11:27,259 --> 00:11:29,470 Remnants of the formation of the solar system. 200 00:11:29,470 --> 00:11:33,559 When I started is a professional scientist, planetary scientist. 201 00:11:33,559 --> 00:11:38,250 Why does Pluto have this big exciting moon called Charon? 202 00:11:38,250 --> 00:11:40,230 And then we found another one and another one. 203 00:11:40,230 --> 00:11:44,249 We keep finding these moons, totally unexpected. 204 00:11:44,249 --> 00:11:48,899 And a great surprise, so it will be very interesting to see what we find when we get there. 205 00:11:48,899 --> 00:11:51,839 How many more are there? 206 00:11:51,839 --> 00:11:58,351 I actually think we have no idea what we're going to find. 207 00:11:58,351 --> 00:12:00,369 It could be completely different. 208 00:12:00,369 --> 00:12:05,970 You see these fabulous paintings that people have drawn of icy surfaces, and clouds and 209 00:12:05,970 --> 00:12:08,639 mist, and rocks and mountains. 210 00:12:08,639 --> 00:12:11,420 It could be completely different. 211 00:12:11,420 --> 00:12:16,610 Oh the satisfaction of the whole mission will come when we see those first pictures and 212 00:12:16,610 --> 00:12:20,910 we actually get a glimpse of what that icy surface looks like. 213 00:12:20,910 --> 00:12:25,720 It really tells us about our world, our solar system formed, and how it got to the way it 214 00:12:25,720 --> 00:12:26,720 is. 215 00:12:26,720 --> 00:12:31,639 So, it's cool, let's go there. 216 00:12:31,639 --> 00:12:35,019 Let's go explore it. 217 00:12:35,019 --> 00:12:41,850 I'm really hoping that we can conserve enough fuel on the New Horizons spacecraft that we 218 00:12:41,850 --> 00:12:46,629 can then use a little bit of extra power to change this spacecraft, deflect it a little 219 00:12:46,629 --> 00:12:50,040 bit and then send it off to another object. 220 00:12:50,040 --> 00:12:55,410 Because I'm pretty sure that Pluto is one of a whole family of very different types 221 00:12:55,410 --> 00:12:56,410 of objects. 222 00:12:56,410 --> 00:13:01,540 Different colors, different ices, different histories, different gases, and it would be 223 00:13:01,540 --> 00:13:04,120 fun to go and see two, not just one. 224 00:13:04,120 --> 00:13:07,269 I'm Fran Bagenal, and I'm a Pluto file. 225 00:13:07,269 --> 00:13:13,259 And the reason is because Pluto is cool. 226 00:13:13,259 --> 00:13:17,220 As we're just two weeks away from the Pluto flyby, we thought it was a great time to cover 227 00:13:17,220 --> 00:13:19,089 the reason for the mission. 228 00:13:19,089 --> 00:13:21,360 Why is New Horizons exploring Pluto? 229 00:13:21,360 --> 00:13:23,649 And what's specifically is New Horizons going to learn? 230 00:13:23,649 --> 00:13:28,070 And to answer that is Bill McKinnon a New Horizons co-investigator from Washington University 231 00:13:28,070 --> 00:13:29,480 in St. Louis. 232 00:13:29,480 --> 00:13:31,489 Bill thanks for joining us. 233 00:13:31,489 --> 00:13:32,489 Thanks for having me. 234 00:13:32,489 --> 00:13:34,820 It's fantastic to be right here, right now. 235 00:13:34,820 --> 00:13:38,570 I just can't even believe it's happening. 236 00:13:38,570 --> 00:13:43,899 When Clyde Tombaugh first discovered Pluto, it was considered an odd ball, but we've learned 237 00:13:43,899 --> 00:13:49,019 then and since over the decades that it was actually a harbinger of an entirely new class 238 00:13:49,019 --> 00:13:51,319 of planets, in a new realm of the solar system. 239 00:13:51,319 --> 00:13:56,040 Kind of show us how the evolution of Pluto--how we got to where--how we think of Pluto today? 240 00:13:56,040 --> 00:14:00,440 Well as you know, Clyde Tombaugh discovered Pluto in 1930. 241 00:14:00,440 --> 00:14:05,239 And at the time, people thought it was the long-sought Planet X, the new world beyond 242 00:14:05,239 --> 00:14:06,239 Neptune. 243 00:14:06,239 --> 00:14:07,759 But, it was odd. 244 00:14:07,759 --> 00:14:10,819 It wasn't as big as Uranus or Neptune. 245 00:14:10,819 --> 00:14:12,589 And in fact, no one could figure out how big it was at all. 246 00:14:12,589 --> 00:14:13,970 And it had this strange orbit. 247 00:14:13,970 --> 00:14:15,300 It wasn't with the rest of the planets. 248 00:14:15,300 --> 00:14:19,389 It had an eccentric loop that even took it inside the orbit of Neptune for a while during 249 00:14:19,389 --> 00:14:21,269 its course around the Sun. 250 00:14:21,269 --> 00:14:26,470 And it really wasn't until the 1990s that we fully grasped where Pluto belonged, in 251 00:14:26,470 --> 00:14:32,579 a sense, what it was trying to tell us back in 1930 because in the early 1990s, we used 252 00:14:32,579 --> 00:14:36,859 CCD technology, the kind of stuff we have in our cell phones now, and finally attached 253 00:14:36,859 --> 00:14:38,230 it to a telescope. 254 00:14:38,230 --> 00:14:42,769 And it's so sensitive that the first new Kuiper Belt object was discovered. 255 00:14:42,769 --> 00:14:47,139 I say new one because, in a sense, we now know that Pluto was the first Kuiper Belt 256 00:14:47,139 --> 00:14:48,930 body to be discovered in human history. 257 00:14:48,930 --> 00:14:51,649 And so, now we know thousands of these bodies. 258 00:14:51,649 --> 00:14:56,540 It's the last, you know, 20 or 30 years of astronomical observations have really filled, 259 00:14:56,540 --> 00:14:57,810 you know, what's going on. 260 00:14:57,810 --> 00:15:01,369 There's a whole new third zone of the solar system beyond Neptune. 261 00:15:01,369 --> 00:15:04,680 It's like we really are then venturing into a new realm, right? 262 00:15:04,680 --> 00:15:06,660 I mean a whole new realm in the Solar System. 263 00:15:06,660 --> 00:15:08,360 Tell us a little bit about that. 264 00:15:08,360 --> 00:15:11,920 Well, if you think about it, in some ways, the Kuiper Belt is like the asteroid belt. 265 00:15:11,920 --> 00:15:14,709 You know, it's--the asteroid belt's a little inside Jupiter. 266 00:15:14,709 --> 00:15:20,110 The Kuiper Belt's outside Neptune, but there's 1,000 times more stuff outside Neptune. 267 00:15:20,110 --> 00:15:24,559 And the best part is that amongst all these hundreds of thousands or millions of bodies 268 00:15:24,559 --> 00:15:29,470 are big worlds, well, big in a relative sense. 269 00:15:29,470 --> 00:15:31,670 They're all--they're small planets. 270 00:15:31,670 --> 00:15:33,920 Pluto is actually the biggest of these, as far as we know. 271 00:15:33,920 --> 00:15:34,949 And there are several others. 272 00:15:34,949 --> 00:15:39,259 So, there's--it's like it's an entirely new Solar System, in a way. 273 00:15:39,259 --> 00:15:40,259 And tell us about that. 274 00:15:40,259 --> 00:15:44,239 I mean you mentioned Pluto is, of all these objects in that region in the Kuiper Belt, 275 00:15:44,239 --> 00:15:47,799 Pluto is the brightest, the biggest that we know about so far. 276 00:15:47,799 --> 00:15:51,919 So, tell us a little bit more about what kind of--like, this new kind of planet that Pluto 277 00:15:51,919 --> 00:15:52,919 represents. 278 00:15:52,919 --> 00:15:53,919 Yeah. 279 00:15:53,919 --> 00:15:57,670 Well, if you look at Pluto, what you'll actually see is an icy world, but on the inside, it 280 00:15:57,670 --> 00:15:59,230 has a rock heart. 281 00:15:59,230 --> 00:16:02,309 And we think it's big enough and warm enough on the inside. 282 00:16:02,309 --> 00:16:04,079 We believe that it could even have an ocean. 283 00:16:04,079 --> 00:16:06,519 And, of course, it's not really alone. 284 00:16:06,519 --> 00:16:07,519 It has a big moon. 285 00:16:07,519 --> 00:16:09,660 In fact, it has five known moons. 286 00:16:09,660 --> 00:16:12,399 So, it's like it's a miniature planetary system. 287 00:16:12,399 --> 00:16:14,339 I mean, and you see those, too. 288 00:16:14,339 --> 00:16:19,019 I think people are amazed that when New Horizons launched, right, there were three moons that 289 00:16:19,019 --> 00:16:20,019 we knew about. 290 00:16:20,019 --> 00:16:21,019 Yeah. 291 00:16:21,019 --> 00:16:24,279 Two more since then, you start to learn a little bit more about what we can learn from 292 00:16:24,279 --> 00:16:25,279 a system like that. 293 00:16:25,279 --> 00:16:26,279 And there's some similarities. 294 00:16:26,279 --> 00:16:30,990 I think we've thought along the way that some similarities between the Earth and Moon, and 295 00:16:30,990 --> 00:16:33,470 Pluto and Charon and its other moons, even how they developed. 296 00:16:33,470 --> 00:16:34,470 Yeah. 297 00:16:34,470 --> 00:16:37,470 You know, if you look in a book, sometimes you'll find the Earth and the Moon described 298 00:16:37,470 --> 00:16:38,529 as a double planet. 299 00:16:38,529 --> 00:16:41,249 But, the Moon's only 1 percent of the Earth's mass. 300 00:16:41,249 --> 00:16:43,309 Pluto's moon is 12 percent of its mass. 301 00:16:43,309 --> 00:16:47,319 So, it's the true binary planet in the Solar System. 302 00:16:47,319 --> 00:16:51,839 And in fact, when we watch it, as we approach with the New Horizons cameras, we actually 303 00:16:51,839 --> 00:16:56,500 see Pluto and Charon both moving, both orbiting their mutual balance point, like a sort of 304 00:16:56,500 --> 00:16:57,839 asymmetric barbell. 305 00:16:57,839 --> 00:17:01,850 So, in fact, that's one of the reasons, of course, we're studying it, because it's going 306 00:17:01,850 --> 00:17:04,919 to help us understand really in a sense how our own Moon formed. 307 00:17:04,919 --> 00:17:09,459 So, I mean that--the Moon formation aspect of it is one. 308 00:17:09,459 --> 00:17:13,439 So, let's--specifically, what is New Horizons going to learn in the Pluto System? 309 00:17:13,439 --> 00:17:14,689 What's it going to teach us about Pluto? 310 00:17:14,689 --> 00:17:17,280 Well, we're going to learn so much. 311 00:17:17,280 --> 00:17:19,800 I could hardly tell you all the things at once. 312 00:17:19,800 --> 00:17:21,130 But, the mission goals, what--? 313 00:17:21,130 --> 00:17:24,440 --Well, you know, there's--we've actually set it up in a sort of hierarchy, where there's 314 00:17:24,440 --> 00:17:28,050 stuff that's absolutely required to do, the stuff that, you know, you don't even have 315 00:17:28,050 --> 00:17:30,010 to be a rocket scientist to understand what we're doing. 316 00:17:30,010 --> 00:17:34,470 We're going to take lots of pictures, understand the global geology, understand what's on the 317 00:17:34,470 --> 00:17:35,790 surface, the composition. 318 00:17:35,790 --> 00:17:38,010 That way we can infer what's underneath. 319 00:17:38,010 --> 00:17:40,740 And of course, Pluto, of course, is a very complicated world. 320 00:17:40,740 --> 00:17:41,890 It has an atmosphere. 321 00:17:41,890 --> 00:17:44,470 It's actually an atmosphere that's slowly leaking off into space. 322 00:17:44,470 --> 00:17:48,400 So, we're going to, you know, probe this atmosphere in every way we can with our instruments and 323 00:17:48,400 --> 00:17:52,950 learn all about it and learn about this fundamental process that affected, actually the early 324 00:17:52,950 --> 00:17:54,470 Earth, atmospheric escape. 325 00:17:54,470 --> 00:17:55,830 So, there's different goals. 326 00:17:55,830 --> 00:18:00,460 As the mission was laid out to see what the science community really wanted New Horizons--any 327 00:18:00,460 --> 00:18:02,670 mission to Pluto and the Kuiper Belt to learn. 328 00:18:02,670 --> 00:18:04,750 You mentioned, there's different levels, different priorities. 329 00:18:04,750 --> 00:18:08,740 So, there is a tops on your list of what we--the mission needs to get. 330 00:18:08,740 --> 00:18:12,830 And then, I guess it goes to another level below, and then levels below that, that--. 331 00:18:12,830 --> 00:18:13,830 Yeah. 332 00:18:13,830 --> 00:18:16,830 So, I talked to you--I talked a little bit about what's absolutely required of the mission. 333 00:18:16,830 --> 00:18:19,510 And then, there's just a lot of important stuff to do. 334 00:18:19,510 --> 00:18:23,350 It's important because we have the cameras and we have the technology that will take 335 00:18:23,350 --> 00:18:25,490 very high resolution pictures. 336 00:18:25,490 --> 00:18:27,190 We'll also take overlapping pictures. 337 00:18:27,190 --> 00:18:29,680 And that way, we can get stereo and really learn the topography. 338 00:18:29,680 --> 00:18:33,870 And we can, of course, measure the temperature, not just in the atmosphere, but on the surface. 339 00:18:33,870 --> 00:18:36,140 In fact, we can do this three separate ways. 340 00:18:36,140 --> 00:18:37,400 That's fantastic. 341 00:18:37,400 --> 00:18:41,620 And if you--and if I--not to interrupt, but if we keep going, there's even stuff that 342 00:18:41,620 --> 00:18:42,620 are--isn't required. 343 00:18:42,620 --> 00:18:45,160 It isn't necessary. 344 00:18:45,160 --> 00:18:46,170 It isn't as important. 345 00:18:46,170 --> 00:18:47,650 But, it's desired. 346 00:18:47,650 --> 00:18:52,860 And that's things like looking for new moons or looking for rings. 347 00:18:52,860 --> 00:18:56,720 And basically, all of the things we want to do, we're going to do them all. 348 00:18:56,720 --> 00:18:58,340 And it's a full slate. 349 00:18:58,340 --> 00:19:02,140 I mean, you have this opportunity, and you have a great spacecraft at your disposal to 350 00:19:02,140 --> 00:19:06,710 get as much as you can possibly get in this one shot in the first time through the Pluto 351 00:19:06,710 --> 00:19:07,710 system. 352 00:19:07,710 --> 00:19:09,140 And so, you're going for the whole list. 353 00:19:11,140 --> 00:19:10,140 Yes. 354 00:19:11,140 --> 00:19:14,840 So, you've been working on a Pluto mission for a long time and really looking forward 355 00:19:14,840 --> 00:19:15,870 to get here. 356 00:19:15,870 --> 00:19:20,120 I just--personally, what are you looking forward to the most of learning at Pluto or just seeing 357 00:19:20,120 --> 00:19:23,750 in that Pluto system as New Horizons goes by? 358 00:19:23,750 --> 00:19:26,470 I've been interested in Pluto my whole life. 359 00:19:26,470 --> 00:19:29,130 I've been working on it scientifically since the early '80s. 360 00:19:29,130 --> 00:19:34,270 But, what I'm most interested in, I suppose, are in fact the details of its geology and 361 00:19:34,270 --> 00:19:37,980 the geology of its big moon because they can both be active worlds. 362 00:19:37,980 --> 00:19:38,980 And who knows? 363 00:19:38,980 --> 00:19:42,360 Maybe there will be clues there for what's on the inside, like an ocean. 364 00:19:42,360 --> 00:19:45,160 And even just in a basic sense, just seeing it up close for the first time, right? 365 00:19:45,160 --> 00:19:50,210 I mean just the ideas of what it might be, but then to really see it, it just has to 366 00:19:50,210 --> 00:19:51,210 be incredible. 367 00:19:51,210 --> 00:19:52,210 Yeah. 368 00:19:52,210 --> 00:19:54,440 I mean day by day, every image is just better than ever taken before. 369 00:19:54,440 --> 00:19:56,200 Well, it's going to be a great ride. 370 00:19:56,200 --> 00:19:57,200 Oh, yeah. 371 00:19:57,200 --> 00:19:58,200 I'm looking forward to it. 372 00:19:58,200 --> 00:19:59,200 Well, thanks, Bill. 373 00:19:59,200 --> 00:20:00,200 Thanks for joining us. 374 00:20:00,200 --> 00:20:01,200 Oh, pleasure to be here. 375 00:20:01,200 --> 00:20:03,860 You know, a misconception of Pluto is that it's so dark. 376 00:20:03,860 --> 00:20:08,720 But, really, for just a moment near dawn and dusk each day, the illumination on Earth actually 377 00:20:08,720 --> 00:20:11,070 matches that of noon on Pluto. 378 00:20:11,070 --> 00:20:12,220 And we call this Pluto time. 379 00:20:12,220 --> 00:20:16,800 And a cool NASA Web program can help you find Pluto time in your area. 380 00:20:16,800 --> 00:20:20,390 It's always Pluto time somewhere, and NASA wants to see your view. 381 00:20:20,390 --> 00:20:22,830 Visit the Pluto time Web site. 382 00:20:22,830 --> 00:20:25,270 Take a picture during your local Pluto time. 383 00:20:25,270 --> 00:20:28,530 And share it to social media with the hashtag #Plutotime. 384 00:20:28,530 --> 00:20:31,990 Then check the Web to see if your view is among the most interesting shots from around 385 00:20:31,990 --> 00:20:33,120 the world. 386 00:20:33,120 --> 00:20:37,480 Of course, for the New Horizons team with just two weeks to go until the flyby, it's 387 00:20:37,480 --> 00:20:38,970 really Pluto time. 388 00:20:38,970 --> 00:20:42,300 Now, this wraps up our weekly updates from Pluto's doorstep. 389 00:20:42,300 --> 00:20:47,350 We'll be back on July 7th to begin our daily live updates that continue through the Pluto 390 00:20:47,350 --> 00:20:48,350 flyby. 391 00:20:48,350 --> 00:20:52,440 So, until then, I'm Mike Buckley from the Johns Hopkins Applied Physics Lab.