WEBVTT FILE 1 00:00:02.600 --> 00:00:03.980 The Sun. 2 00:00:04.000 --> 00:00:05.380 It’s the solar system’s engine, 3 00:00:05.400 --> 00:00:08.480 and the only star in the sky that gets our attention… 4 00:00:08.500 --> 00:00:10.480 every day. 5 00:00:10.500 --> 00:00:11.480 But up close, 6 00:00:11.500 --> 00:00:14.880 it’s unlike anything we can see from Earth. 7 00:00:14.900 --> 00:00:16.180 It’s ferocious— 8 00:00:16.200 --> 00:00:19.400 a writhing mass of nuclear chaos, 9 00:00:19.420 --> 00:00:21.180 tangled magnetic lines, 10 00:00:21.200 --> 00:00:24.980 and a constant wind with inconceivably high temperatures 11 00:00:25.000 --> 00:00:32.180 and speeds close to a million miles an hour. 12 00:00:32.200 --> 00:00:35.980 Over the years NASA has sent probes all over the solar system… 13 00:00:36.000 --> 00:00:37.580 ...but never to the Sun. 14 00:00:37.600 --> 00:00:39.480 Check this out. 15 00:00:39.500 --> 00:00:41.180 This is the Parker Solar Probe… 16 00:00:41.200 --> 00:00:46.180 …and it’s going to be humanity’s first mission assigned to touch the Sun. 17 00:00:46.200 --> 00:00:49.970 It will fly to within 4 million miles of the Sun’s surface 18 00:00:49.990 --> 00:00:51.680 confronting brutal radiation 19 00:00:51.700 --> 00:00:56.580 and temperatures that can reach 1,000,000 degrees Fahrenheit. 20 00:00:56.600 --> 00:00:58.290 Parker Solar Probe has been prepped 21 00:00:58.310 --> 00:01:01.880 to fly right through that unforgiving atmosphere. 22 00:01:01.900 --> 00:01:05.180 It's a rough journey. 23 00:01:05.200 --> 00:01:07.780 Typically, if you want to head out into the solar system, 24 00:01:07.800 --> 00:01:10.280 you merge with orbital traffic. 25 00:01:10.300 --> 00:01:12.780 But if you want to head toward the center of the solar system, 26 00:01:12.800 --> 00:01:14.480 you've got to run the other way… 27 00:01:14.500 --> 00:01:17.080 and it takes a lot of energy. 28 00:01:17.100 --> 00:01:20.380 once it arrives, the spacecraft has got to take the heat. 29 00:01:20.400 --> 00:01:22.880 Bathed in radiation as it swoops in close, 30 00:01:22.900 --> 00:01:24.780 Parker Solar Probe will use an advanced 31 00:01:24.800 --> 00:01:26.780 carbon/carbon composite heat shield 32 00:01:26.800 --> 00:01:27.380 o protect its delicate instruments. 33 00:01:27.400 --> 00:01:32.280 And here’s a technical triumph: 34 00:01:32.300 --> 00:01:34.580 the spacecraft’s thermal regulation system 35 00:01:34.600 --> 00:01:37.180 will use just a single gallon of ordinary water 36 00:01:37.200 --> 00:01:38.880 H 2 O 37 00:01:38.900 --> 00:01:44.780 to collect and then dissipate heat…just like a car radiator. 38 00:01:44.800 --> 00:01:46.540 It will fly into the corona, 39 00:01:46.560 --> 00:01:50.340 the super hot region of gas and plasma surrounding the Sun. 40 00:01:50.360 --> 00:01:52.460 There’s hardly a there there, 41 00:01:52.480 --> 00:01:55.920 as high energy particles fly outward like streamers. 42 00:01:55.940 --> 00:01:58.860 But – and this is another weird thing about the sun- 43 00:01:58.880 --> 00:02:02.580 -the corona is hotter than the surface of the star itself. 44 00:02:02.600 --> 00:02:04.440 We have a few good theories about this– 45 00:02:04.460 --> 00:02:06.680 but we're really not sure why. 46 00:02:06.700 --> 00:02:09.570 There's some process in the atmosphere that keeps heating it up 47 00:02:09.590 --> 00:02:11.620 even as it gets further away from the core. 48 00:02:11.640 --> 00:02:15.330 Parker Solar Probe is going to try and figure it out. 49 00:02:15.350 --> 00:02:18.170 The corona also propels the solar wind out into space 50 00:02:18.190 --> 00:02:19.590 at incredible speeds 51 00:02:19.610 --> 00:02:21.990 way beyond the orbit of Pluto. 52 00:02:22.010 --> 00:02:27.660 No one knows for sure what accelerates it so far so fast. 53 00:02:27.680 --> 00:02:31.170 Parker Solar Probe is going to fly right through the origin of this wind, 54 00:02:31.190 --> 00:02:36.640 right where it starts, to figure out how the whole system works 55 00:02:36.660 --> 00:02:41.690 We can’t see those processes from Earth, or even from space. 56 00:02:41.710 --> 00:02:48.080 Parker Solar Probe is our first direct encounter with a star. 57 00:02:48.100 --> 00:02:51.780 Our Sun is the only star we can visit…. 58 00:02:51.800 --> 00:02:52.680 …which means this mission will gather 59 00:02:52.700 --> 00:02:57.470 important information about how stars work…everywhere. 60 00:02:57.490 --> 00:03:01.520 That’s information we can only get by going straight to the source. 61 00:03:01.540 --> 00:03:04.280 Some journeys are harder than others. 62 00:03:04.300 --> 00:03:08.880 Some destinations are further, higher, hotter. 63 00:03:08.900 --> 00:03:12.490 But the only way to explore a new destination 64 00:03:12.510 --> 00:03:15.190 is to actually make the journey. 65 00:03:15.210 --> 00:03:17.290 Parker Solar Probe: 66 00:03:17.310 --> 00:03:31.790 See you on The Sun.