1 00:00:11,136 --> 00:00:11,594 That's right. 2 00:00:11,594 --> 00:00:15,473 So NASA's Parker Solar Probe, which launched in 2018, 3 00:00:15,724 --> 00:00:20,061 has been using Venus gravity assist to get closer and closer to the sun. 4 00:00:20,437 --> 00:00:23,023 And most recently, it had a Venus gravity assist. 5 00:00:23,023 --> 00:00:27,736 And so now it's going to fly within 3.83 million miles of the surface of the sun, 6 00:00:27,736 --> 00:00:30,822 which is closer than any human made object has ever gone 7 00:00:30,822 --> 00:00:33,825 before. 8 00:00:41,833 --> 00:00:42,375 That's right. 9 00:00:42,375 --> 00:00:42,709 Even though 10 00:00:42,709 --> 00:00:46,421 the sun is a constant in our sky, the sun is not constant at all. 11 00:00:46,421 --> 00:00:50,925 The sun constantly has magnetic explosions and little bursts of energy 12 00:00:50,925 --> 00:00:54,471 that come out, and sometimes big burst of energy like the solar storms. 13 00:00:54,888 --> 00:00:58,516 And by measuring that process, as it happens, 14 00:00:58,516 --> 00:01:02,979 so close to where its original energy source was, we can really understand 15 00:01:03,271 --> 00:01:06,691 more about the energization and the 16 00:01:06,691 --> 00:01:09,819 the structures as they evolve through the solar system. 17 00:01:19,746 --> 00:01:21,498 I am so excited about 18 00:01:21,498 --> 00:01:24,501 Parker touching the top edges of the, 19 00:01:25,043 --> 00:01:28,296 corona, the solar corona, the outer atmosphere of the sun, 20 00:01:28,671 --> 00:01:32,383 and by measuring it in such detail so close, 21 00:01:32,634 --> 00:01:35,929 we can combine that with what we already know about the sun 22 00:01:36,304 --> 00:01:39,099 and the solar system and that that material as that 23 00:01:39,099 --> 00:01:41,893 fills the solar system from our other spacecraft. 24 00:01:41,893 --> 00:01:45,522 But by putting all of these pieces together, we can really learn more 25 00:01:45,522 --> 00:01:49,025 about the solar corona and that material as it fills 26 00:01:49,025 --> 00:01:52,028 our solar system. 27 00:01:58,451 --> 00:02:01,412 So during a total solar eclipse, that's when the moon comes 28 00:02:01,412 --> 00:02:04,749 between us here on the Earth and the sun, and it blocks out the main bright 29 00:02:04,749 --> 00:02:05,834 part of the sun 30 00:02:05,834 --> 00:02:09,796 so that we can see the solar corona, the outer atmosphere of the sun. 31 00:02:10,046 --> 00:02:12,465 That outer atmosphere is extremely hot 32 00:02:12,465 --> 00:02:16,094 and it flows outwards, filling our solar system. 33 00:02:16,845 --> 00:02:20,682 And Parker is flying through the outer reaches of that solar corona. 34 00:02:20,890 --> 00:02:26,229 Really understanding how that energy is put into that material in the first place. 35 00:02:34,445 --> 00:02:37,448 Yeah, NASA has a number of cool missions coming up. 36 00:02:37,532 --> 00:02:39,284 One of the missions is called Punch. 37 00:02:39,284 --> 00:02:41,202 Punch has, 38 00:02:41,202 --> 00:02:43,121 3D imaging capability. 39 00:02:43,121 --> 00:02:43,872 So it's going to be able 40 00:02:43,872 --> 00:02:47,792 to see the corona in three dimensions, the outer atmosphere of the sun, 41 00:02:48,042 --> 00:02:52,088 and watch that corona as it expands outwards into the solar system 42 00:02:52,505 --> 00:02:57,218 and CODEX, which is, coronagraph that's on the International Space Station. 43 00:02:57,552 --> 00:03:00,638 So that also is going to be looking at the corona 44 00:03:01,306 --> 00:03:04,642 and measuring the temperature and the velocity of that, 45 00:03:05,977 --> 00:03:09,314 of that material as it flows outwards, which we can compare directly 46 00:03:09,314 --> 00:03:12,567 with what Parker measures in detail in those outer 47 00:03:12,567 --> 00:03:15,570 reaches of the corona. 48 00:03:21,492 --> 00:03:22,243 We have 49 00:03:22,243 --> 00:03:26,247 never had a human made object so close to the sun. 50 00:03:26,623 --> 00:03:31,336 To get that close, we had to use Venus to have our gravity assist, 51 00:03:31,336 --> 00:03:34,339 to slow Parker down so that it can get that close. 52 00:03:34,714 --> 00:03:36,216 Also, we had to not melt. 53 00:03:36,216 --> 00:03:40,053 That's why the Parker has this heat shield that holds the instruments 54 00:03:40,053 --> 00:03:43,056 at room temperature and keeps the heat of the sun away. 55 00:03:43,431 --> 00:03:45,308 And these are just amazing feats. 56 00:03:45,308 --> 00:03:47,393 And so it's so amazing that we are so close 57 00:03:47,393 --> 00:03:52,315 and really getting to measure in detail this material up close. 58 00:04:02,158 --> 00:04:02,784 You can learn 59 00:04:02,784 --> 00:04:06,579 more about Parker Solar Probe at NASA.gov/parker 60 00:04:06,579 --> 00:04:10,875 and you can also check us out on @NASASun.