1 00:00:00,030 --> 00:00:05,730 Parker Solar Probe has been around since 1958 in some form or another and now in 2 00:00:05,730 --> 00:00:10,500 2018 and we're getting ready to actually launch Parker Solar Probe. A lot of that has 3 00:00:10,500 --> 00:00:14,009 to do with the fact that getting some of the Sun is actually really hard and 4 00:00:14,009 --> 00:00:17,400 there's a lot of technology that needed to be developed in order to enable this 5 00:00:17,400 --> 00:00:20,760 mission there are many enabling technologies the 6 00:00:20,760 --> 00:00:25,019 solar arrays were very important the autonomy was very important one of the 7 00:00:25,019 --> 00:00:29,310 ones that was obviously also critical is the heat shield and developing the 8 00:00:29,310 --> 00:00:35,100 technology actually protect the probe at the Sun that titanium truss was also 9 00:00:35,100 --> 00:00:38,940 specially designed for Solar Probe. It's actually really a neat piece it's a a 10 00:00:38,940 --> 00:00:43,410 welded titanium trust that's about four feet tall but it only weighs about 50 11 00:00:43,410 --> 00:00:48,300 pounds and the key there is we're trying to minimize the conduction between the 12 00:00:48,300 --> 00:00:52,110 heat shield and the spacecraft so you want to have as little stuff there as 13 00:00:52,110 --> 00:00:54,270 possible the Parker Solar Probe heat shield is 14 00:00:54,270 --> 00:00:58,350 basically one giant sandwich panel and a sandwich panel is a lot like a honeycomb 15 00:00:58,350 --> 00:01:02,340 panel you find in a traditional spacecraft or on airplanes you have two 16 00:01:02,340 --> 00:01:07,049 outer face sheets and then you have a core in this case the two outer face 17 00:01:07,049 --> 00:01:10,590 sheets are carbon carbon composite which is a lot like the graphite epoxy you 18 00:01:10,590 --> 00:01:14,520 might find in your golf clubs it's just been superheated and then the inside is 19 00:01:14,520 --> 00:01:19,080 a carbon foam so the Parker Solar Probe heat shield has a white coating that's 20 00:01:19,080 --> 00:01:22,979 on the Sun facing surface of this giant frisbee that's protecting the rest of 21 00:01:22,979 --> 00:01:26,189 the spacecraft and that white coating was specially designed to here at the 22 00:01:26,189 --> 00:01:30,689 Lab in collaboration with REDD and the Space Department as well as the Whiting 23 00:01:30,689 --> 00:01:34,799 School at Johns Hopkins proper to actually work at the Sun, and was 24 00:01:34,799 --> 00:01:38,579 specifically designed for Solar Probe and the concept is basically you'd 25 00:01:38,579 --> 00:01:42,210 rather be in a white car in a hot day than a black car the hot day it's just 26 00:01:42,210 --> 00:01:46,770 that it just knocks down the heat that much more and so it's helping us stay 27 00:01:46,770 --> 00:01:49,759 cool at this the particles of the corona are very hot 28 00:01:49,759 --> 00:01:55,189 like 3 million degrees however they're very dispersed it's not all 3 million 29 00:01:55,189 --> 00:01:59,719 degrees everywhere it's a little hard to visualize but think about when you are 30 00:01:59,719 --> 00:02:03,679 baking cookies and you have your oven and you can stick your hand in and your 31 00:02:03,679 --> 00:02:06,950 hand doesn't burn up but if you touch something then you'd burn yourself so 32 00:02:06,950 --> 00:02:11,870 similarly when we're actually at the sun's corona we're not getting that hot 33 00:02:11,870 --> 00:02:16,489 because there's just not as much there so the temperature is actually lower 34 00:02:16,489 --> 00:02:19,340 than the overall temperature of the particles that are active the chrome 35 00:02:19,340 --> 00:02:23,209 when we're at closest approach the front surface of the heat shield will be at 36 00:02:23,209 --> 00:02:27,829 about 2500 degrees Fahrenheit the back surface the heat shield will be about 37 00:02:27,829 --> 00:02:31,700 600 degrees Fahrenheit but then the spacecraft bus is basically sitting at 38 00:02:31,700 --> 00:02:36,920 85 degrees Fahrenheit so the shield is actually really keeping everything very 39 00:02:36,920 --> 00:02:39,980 cool and that's most the stuff that's on that bus additionally there are a couple 40 00:02:39,980 --> 00:02:43,849 of instruments that are hanging out off the truss and they will be hot like the 41 00:02:43,849 --> 00:02:48,290 heat shield like SPC and FIELDS there's our brave instruments sticking out in 42 00:02:48,290 --> 00:02:52,310 the Sun but everything else will be kept at that nice temperature, 85 degrees (F) so 43 00:02:52,310 --> 00:02:55,370 they can be working properly and giving all that great science data that we're 44 00:02:55,370 --> 00:03:02,000 so excited about after working on this for 10 years it is really a pleasure to 45 00:03:02,000 --> 00:03:07,760 see it kind of actually coming to fruition to be one small part of this 46 00:03:07,760 --> 00:03:11,930 huge engineering team that is making science dreams come true it's just 47 00:03:11,930 --> 00:03:15,889 amazing I can't wait to rewrite textbooks and 48 00:03:15,889 --> 00:03:20,569 change the way we look at the Sun forever I'm whole ball of excited and I 49 00:03:20,569 --> 00:03:23,630 honestly don't know exactly how I'm gonna feel at launch but I'm really 50 00:03:23,630 --> 00:03:28,489 excited to pass this off to the Mission Operations team and see all the science 51 00:03:28,489 --> 00:03:35,709 data that comes down and just get to enjoy all that Solar Probe brings us 52 00:03:38,520 --> 00:03:40,580