1 00:00:00,230 --> 00:00:02,730 (light music) 2 00:00:05,870 --> 00:00:07,320 - Hi, I'm Ellen Stofan, 3 00:00:07,320 --> 00:00:08,930 the John and Adrienne Mars Director 4 00:00:08,930 --> 00:00:11,670 of the Smithsonian's National Air and Space Museum. 5 00:00:11,670 --> 00:00:14,540 I'm Doctor E and we're here for another episode 6 00:00:14,540 --> 00:00:16,600 of E.Z. Science. 7 00:00:16,600 --> 00:00:18,040 - Hey, and I'm Thomas Zurbuchen, 8 00:00:18,040 --> 00:00:20,057 the Associate Administrator for Science 9 00:00:20,057 --> 00:00:22,800 at NASA also known as Doctor Z. 10 00:00:22,800 --> 00:00:25,370 - We're here today to talk a little bit about something 11 00:00:25,370 --> 00:00:26,960 that people don't probably think of as being 12 00:00:26,960 --> 00:00:28,340 that important in their lives 13 00:00:28,340 --> 00:00:31,230 but if for example you use some app 14 00:00:31,230 --> 00:00:33,032 to help you get to where you were going today, 15 00:00:33,032 --> 00:00:36,650 you're actually relying on NASA understanding the sun. 16 00:00:36,650 --> 00:00:39,890 - So we're looking at our star, our favorite star, 17 00:00:39,890 --> 00:00:42,900 the sun and we see that the star is a magnetic star. 18 00:00:42,900 --> 00:00:46,240 You see as the sun is boiling at the surface 19 00:00:46,240 --> 00:00:50,010 because it's so hot it's carrying with it magnetic fields. 20 00:00:50,010 --> 00:00:51,930 And like little arcs they're there 21 00:00:51,930 --> 00:00:55,070 and they're interacting with each other liberating energy, 22 00:00:55,070 --> 00:00:58,740 UV energy of the type that of course burns your skin, 23 00:00:58,740 --> 00:01:00,680 an x-ray like you see at the doctor. 24 00:01:00,680 --> 00:01:02,630 That kind of radiation is coming from the sun 25 00:01:02,630 --> 00:01:04,269 and it's spreading around causing 26 00:01:04,269 --> 00:01:06,800 what we call space weather. 27 00:01:06,800 --> 00:01:09,980 Of course, as it's heating up, that atmosphere, the corona, 28 00:01:09,980 --> 00:01:12,120 it's also blowing away it's atmosphere. 29 00:01:12,120 --> 00:01:14,490 It cannot hold on to it and it's filling the space 30 00:01:14,490 --> 00:01:15,760 between the planets. 31 00:01:15,760 --> 00:01:16,770 - Now that space weather 32 00:01:16,770 --> 00:01:19,490 is what can disrupt our communication satellites, 33 00:01:19,490 --> 00:01:20,790 our GPS satellites. 34 00:01:20,790 --> 00:01:22,504 For the astronauts up on the space station, 35 00:01:22,504 --> 00:01:24,820 they even have to worry about what's going on 36 00:01:24,820 --> 00:01:26,090 on the surface of the sun. 37 00:01:26,090 --> 00:01:27,910 - Exactly right and when they're leaving 38 00:01:27,910 --> 00:01:29,553 to go to the moon or to Mars, 39 00:01:29,553 --> 00:01:31,010 that is even more important 40 00:01:31,010 --> 00:01:31,843 because now we're away 41 00:01:31,843 --> 00:01:34,860 from the magnetic protection of our Earth. 42 00:01:34,860 --> 00:01:38,280 - Now NASA has a lot of spacecrafts studying the sun, 43 00:01:38,280 --> 00:01:40,972 and they get as close to the sun as they can, 44 00:01:40,972 --> 00:01:43,110 but right now we have a spacecraft up there 45 00:01:43,110 --> 00:01:45,400 that's doing something pretty special. 46 00:01:45,400 --> 00:01:47,270 Can you tell us about the Parker Solar Probe? 47 00:01:47,270 --> 00:01:50,150 - It's really the first spacecraft to touch the sun, 48 00:01:50,150 --> 00:01:53,470 to fly through that corona, through that atmosphere, 49 00:01:53,470 --> 00:01:56,800 and sample it in a way that we've never seen. 50 00:01:56,800 --> 00:01:59,730 So in fact it just completed its third orbit 51 00:01:59,730 --> 00:02:02,660 by the sun and it's collecting data 52 00:02:02,660 --> 00:02:04,080 and sending it back to Earth. 53 00:02:04,080 --> 00:02:05,770 So we're learning about this atmosphere 54 00:02:05,770 --> 00:02:08,350 in a way we've never seen before just now. 55 00:02:08,350 --> 00:02:09,780 - I think a lot of people don't recognize 56 00:02:09,780 --> 00:02:11,910 that when NASA does things like go to a planet 57 00:02:11,910 --> 00:02:13,542 or get really close to the sun, 58 00:02:13,542 --> 00:02:16,416 we have to push technology in ways 59 00:02:16,416 --> 00:02:18,610 that you just don't normally have to do 60 00:02:18,610 --> 00:02:21,750 which then spins off and benefits us right here on Earth. 61 00:02:21,750 --> 00:02:22,583 - Absolutely. 62 00:02:22,583 --> 00:02:24,840 A lot of these materials that are being developed 63 00:02:24,840 --> 00:02:27,220 right here for Parker Solar Probe and we're developed 64 00:02:27,220 --> 00:02:29,370 in the last decade or so are materials 65 00:02:29,370 --> 00:02:31,790 that are very much applicable in other systems 66 00:02:31,790 --> 00:02:33,110 like energy systems 67 00:02:33,110 --> 00:02:35,291 or even fire fighting type of applications 68 00:02:35,291 --> 00:02:38,580 where those kind of materials matter for example. 69 00:02:38,580 --> 00:02:41,330 - Now we did get a question that someone sent in 70 00:02:41,330 --> 00:02:42,950 to E.Z. Science, so don't forget 71 00:02:42,950 --> 00:02:46,120 about sending your questions in for future episodes. 72 00:02:46,120 --> 00:02:47,830 Parker has gathered some information 73 00:02:47,830 --> 00:02:51,090 about why the sun's corona is hotter than its surface. 74 00:02:51,090 --> 00:02:54,370 Tell us a bit about what it's found in its first year. 75 00:02:54,370 --> 00:02:57,070 - What we're learning about is that the near corona 76 00:02:57,070 --> 00:02:59,730 like right down there by the sun 77 00:02:59,730 --> 00:03:03,580 is a lot more turbulent, a lot more interactive 78 00:03:03,580 --> 00:03:04,870 than we thought before. 79 00:03:04,870 --> 00:03:05,990 - This is a spacecraft 80 00:03:05,990 --> 00:03:07,890 that was named for a living scientist 81 00:03:07,890 --> 00:03:09,710 and can you tell us why we did that? 82 00:03:09,710 --> 00:03:12,980 - Eugene Parker is so important for that entire field. 83 00:03:12,980 --> 00:03:15,760 He's the guy who predicted that the solar atmosphere 84 00:03:15,760 --> 00:03:18,070 would be blown off into super sonic stream, 85 00:03:18,070 --> 00:03:19,230 the solar wind. 86 00:03:19,230 --> 00:03:21,600 Highly controversial and of course he was right. 87 00:03:21,600 --> 00:03:25,090 In fact, there is something like 35 spacecraft 88 00:03:25,090 --> 00:03:27,940 in all of NASA's inventory that are dealing with things 89 00:03:27,940 --> 00:03:30,739 that Parker predicted and I will never forget 90 00:03:30,739 --> 00:03:32,930 how Parker looked and his family 91 00:03:32,930 --> 00:03:35,450 when the rocket went into the sky with him 92 00:03:35,450 --> 00:03:38,163 seeing his spacecraft leave the Earth. 93 00:03:41,640 --> 00:03:43,130 I'm going to ask you the second question 94 00:03:43,130 --> 00:03:46,970 that is how does the research in space help prepare humans 95 00:03:46,970 --> 00:03:49,410 on a journey to future Artemis missions 96 00:03:49,410 --> 00:03:51,290 to the moon, Mars, and beyond? 97 00:03:51,290 --> 00:03:53,020 - So the more that we can monitor the sun, 98 00:03:53,020 --> 00:03:54,470 the more that we can understand 99 00:03:54,470 --> 00:03:56,050 and predict what's happening at the sun, 100 00:03:56,050 --> 00:03:58,900 the better we can do with protecting the astronauts. 101 00:03:58,900 --> 00:04:00,810 Now if we know there's a solar flares 102 00:04:00,810 --> 00:04:03,880 of particles coming towards them, they can go into areas 103 00:04:03,880 --> 00:04:04,800 that are shielded. 104 00:04:04,800 --> 00:04:06,940 And those are some of the technologies we work on 105 00:04:06,940 --> 00:04:10,530 is how do we protect astronauts from this space radiation 106 00:04:10,530 --> 00:04:13,960 both from the sun but also from galactic cosmic rays. 107 00:04:13,960 --> 00:04:15,470 We're gonna be able to do that research 108 00:04:15,470 --> 00:04:17,240 even better on the surface of the moon 109 00:04:17,240 --> 00:04:18,807 outside of our magnetic field 110 00:04:18,807 --> 00:04:20,760 where as Thomas said the astronauts 111 00:04:20,760 --> 00:04:22,150 are much more vulnerable. 112 00:04:22,150 --> 00:04:24,560 Now Thomas, some of the surface science from Artemis 113 00:04:24,560 --> 00:04:26,646 is also gonna help us eventually get to Mars. 114 00:04:26,646 --> 00:04:27,510 - Of course. 115 00:04:27,510 --> 00:04:30,340 As we're sampling the surface of the moon, 116 00:04:30,340 --> 00:04:32,040 what we also will be able to do 117 00:04:32,040 --> 00:04:34,040 is look at the components that are in there, 118 00:04:34,040 --> 00:04:36,770 especially water, that we may be able to use 119 00:04:36,770 --> 00:04:39,370 both on the moon and Mars over time 120 00:04:39,370 --> 00:04:42,350 to live off but also make fuel out of it. 121 00:04:42,350 --> 00:04:43,820 So it's really exciting. 122 00:04:43,820 --> 00:04:45,330 - Well I'm afraid we're out of time 123 00:04:45,330 --> 00:04:47,410 and thank you, this has been incredibly fun 124 00:04:47,410 --> 00:04:49,290 to talk about our favorite star. 125 00:04:49,290 --> 00:04:51,730 - And I really want to encourage everybody 126 00:04:51,730 --> 00:04:53,080 to send questions again, 127 00:04:53,080 --> 00:04:54,160 questions that we'll answer