1 00:00:01,634 --> 00:00:05,538 In 1958 scientists put a vision that 2 00:00:05,538 --> 00:00:08,675 we need to fly a spacecraft within the atmosphere of the Sun, 3 00:00:08,675 --> 00:00:12,445 but it is so challenging, extremely difficult to realize, 4 00:00:12,445 --> 00:00:16,616 that it took us six decades to build a system that can fly safely 5 00:00:16,616 --> 00:00:18,985 and reliably within the atmosphere of a star. 6 00:00:19,386 --> 00:00:23,323 Three. Two. One. Zero. 7 00:00:23,790 --> 00:00:26,226 Liftoff of the mighty Delta Four Heavy 8 00:00:26,226 --> 00:00:29,229 rocket with NASA's Parker Solar Probe. 9 00:00:29,362 --> 00:00:32,799 A daring mission to shed light on the mysteries of our closest star, 10 00:00:33,066 --> 00:00:35,068 the Sun. 11 00:00:44,177 --> 00:00:48,915 [Chatter and ambient sounds] 12 00:00:48,915 --> 00:00:51,418 It looked like we had a hit there for a second. 13 00:00:52,952 --> 00:00:53,653 Yes, Nick. 14 00:00:53,653 --> 00:00:57,424 I believe we do have detection of beacon tone one. 15 00:00:57,824 --> 00:01:02,695 [Applause] 16 00:01:02,695 --> 00:01:03,596 There it is. 17 00:01:03,596 --> 00:01:04,030 See it? 18 00:01:04,030 --> 00:01:05,198 There it is. 19 00:01:05,198 --> 00:01:08,101 [Applause] 20 00:01:09,135 --> 00:01:10,937 Parker Solar Probe is 3.8 21 00:01:10,937 --> 00:01:12,172 3.8 22 00:01:12,172 --> 00:01:12,972 3.8 23 00:01:12,972 --> 00:01:14,774 million miles from the surface of the Sun. 24 00:01:14,774 --> 00:01:17,877 It is so incredible to just realize 25 00:01:17,877 --> 00:01:21,514 this is the moment that we designed this mission for. 26 00:01:21,514 --> 00:01:24,951 3.8 million miles may not sound that close, 27 00:01:24,951 --> 00:01:28,154 but if I put the Sun and the Earth one meter apart, 28 00:01:28,621 --> 00:01:31,591 Parker Solar Probe would be four centimeters from the Sun. 29 00:01:31,591 --> 00:01:35,061 It's the closest human made object to a star 30 00:01:35,061 --> 00:01:40,967 and also the fastest traveling at 430,000 miles an hour. 31 00:01:41,201 --> 00:01:44,337 I mean, we're flying through the atmosphere of a star. 32 00:01:44,337 --> 00:01:46,506 That's not easy to do. 33 00:01:46,506 --> 00:01:48,608 It's something we've never done before. 34 00:01:49,542 --> 00:01:52,745 This is our first close encounter with a star 35 00:01:52,745 --> 00:01:54,347 and it’s really just amazing. 36 00:01:54,347 --> 00:01:56,382 This area that Parker’s going into 37 00:01:56,382 --> 00:01:59,052 is just so crucial to our understanding of the Sun 38 00:01:59,052 --> 00:02:00,753 and its impact on the Earth. 39 00:02:00,753 --> 00:02:03,289 That solar interaction, that space weather, 40 00:02:03,289 --> 00:02:06,559 those billions of tons of material that the Sun can throw at us, 41 00:02:06,559 --> 00:02:09,963 interacts with our power grids, can interact with our technology, 42 00:02:09,963 --> 00:02:12,599 so it's really important to understand them at their source 43 00:02:12,599 --> 00:02:14,100 and how they get all that energy. 44 00:02:14,334 --> 00:02:17,737 When we were thinking about designing a spacecraft to go to someplace 45 00:02:17,737 --> 00:02:22,775 that had never been before, and it's actually going there to study the Sun, 46 00:02:22,775 --> 00:02:25,211 and so you're kind of saying, what am I designing? 47 00:02:25,211 --> 00:02:27,413 What are the environments we’re designing for? 48 00:02:27,413 --> 00:02:32,318 It has to go from the deepest, coldest, space to a very warm area 49 00:02:32,318 --> 00:02:36,389 and keep everything working at a little bit above room temperature. 50 00:02:36,623 --> 00:02:39,659 It's designed to go to such an extreme environment. 51 00:02:39,659 --> 00:02:43,096 You look at it and it doesn't quite look like most other spacecraft. 52 00:02:43,096 --> 00:02:44,697 The whole thing is designed 53 00:02:44,697 --> 00:02:48,668 such that the heat shield is taking most of the brunt of the heat of the Sun. 54 00:02:48,668 --> 00:02:53,306 The heat shield will be at about 1800 degrees Fahrenheit 55 00:02:53,306 --> 00:02:55,008 and it's protecting the spacecraft. 56 00:02:55,008 --> 00:02:57,677 So the spacecraft's actually basically at room temperature. 57 00:02:57,677 --> 00:03:00,313 This is such a great feat of engineering 58 00:03:00,313 --> 00:03:03,750 and it really shows how capable we are in space. 59 00:03:04,384 --> 00:03:05,585 This is something that 60 00:03:05,585 --> 00:03:10,056 we've been wanting to do since 1958 when it was first mentioned, 61 00:03:10,390 --> 00:03:14,460 and the technical problems that had to be overcome in order to achieve it — 62 00:03:14,794 --> 00:03:17,463 it's just monumental to be able to get a spacecraft 63 00:03:17,463 --> 00:03:18,798 this close to the Sun. 64 00:03:18,798 --> 00:03:21,267 To get close to the Sun 65 00:03:22,135 --> 00:03:24,304 is not easy. 66 00:03:24,304 --> 00:03:27,974 It looks like from Earth to the Sun is not that far, 67 00:03:28,241 --> 00:03:30,743 uh, the key issue is energy. 68 00:03:30,743 --> 00:03:34,047 In order for Parker to get close to the Sun, 69 00:03:34,047 --> 00:03:37,350 we needed to lose lots of Parker’s speed 70 00:03:37,350 --> 00:03:39,686 possessed at earth’s orbit. 71 00:03:39,686 --> 00:03:43,456 Fortunately, I was able to create a 72 00:03:43,923 --> 00:03:47,227 trajectory with seven Venus flyby. 73 00:03:47,560 --> 00:03:49,062 The mission uses Venus 74 00:03:49,062 --> 00:03:51,497 in order to actually change its angular momentum 75 00:03:51,497 --> 00:03:54,834 and slow down to actually go closer and closer to the Sun. 76 00:03:55,668 --> 00:03:59,105 Over the course of about six years and seven flybys, 77 00:03:59,239 --> 00:04:03,476 we were able to move closer to the Sun, and each time unraveling a little bit 78 00:04:03,476 --> 00:04:06,579 more of the mysteries of the Sun as we get data from places 79 00:04:06,579 --> 00:04:08,648 that no spacecraft has ever been before. 80 00:04:09,816 --> 00:04:14,153 It's the only star in our galaxy that we can actually go visit, 81 00:04:14,153 --> 00:04:15,822 and that's what makes it so magical. 82 00:04:15,822 --> 00:04:18,725 By flying within the atmosphere of a star, 83 00:04:18,725 --> 00:04:22,061 we are basically tracing the fingerprints 84 00:04:22,061 --> 00:04:24,230 of the physical mechanisms of the Sun. 85 00:04:24,497 --> 00:04:27,166 We now view the Sun in a different way. 86 00:04:27,500 --> 00:04:30,169 When you look at images from Parker Solar Probe 87 00:04:32,038 --> 00:04:34,474 they are extremely, extremely complex. 88 00:04:34,941 --> 00:04:38,278 And that complexity for us, it’s a new science 89 00:04:38,278 --> 00:04:40,747 that we need to investigate. We need to understand. 90 00:04:41,414 --> 00:04:45,118 The things that we’ve learned over the years that Parker’s been in orbit 91 00:04:45,118 --> 00:04:48,321 have been amazing. They’ve challenged our ideas about 92 00:04:48,321 --> 00:04:50,156 how the solar wind is made, 93 00:04:50,156 --> 00:04:51,958 about how the Sun works, 94 00:04:51,958 --> 00:04:54,961 about some of these fundamental things that are going on. 95 00:04:57,063 --> 00:04:59,299 There's a lot of pride and excitement 96 00:04:59,299 --> 00:05:01,701 for this closest approach. 97 00:05:01,701 --> 00:05:03,369 So much effort 98 00:05:03,369 --> 00:05:05,872 and so many people have worked on this. 99 00:05:05,872 --> 00:05:10,143 I think it really took the teamwork and synergy of engineers and scientists 100 00:05:10,143 --> 00:05:14,714 and administrators and, and a lot of different people to think this mission up. 101 00:05:15,715 --> 00:05:16,883 It makes you think 102 00:05:17,550 --> 00:05:20,853 that you can basically overcome any hurdles, 103 00:05:20,853 --> 00:05:24,857 so dream big and go out there and make them happen.