WEBVTT FILE 1 00:00:00.060 --> 00:00:06.660 We're gonna step away from the Earth for a little bit and talk about in my view 2 00:00:06.660 --> 00:00:10.349 and some view the most important object in the solar system besides the one we 3 00:00:10.349 --> 00:00:18.300 live on but the one at the center of it the Sun. The thing that powers it all, so 4 00:00:18.300 --> 00:00:27.020 let's start off with the Sun we see every day is not too exciting I mean we 5 00:00:27.020 --> 00:00:31.560 know that we're not supposed to look at it. It's really really bright but even if 6 00:00:31.560 --> 00:00:36.540 you look at it with a telescope and look at it in invisible light unless there's 7 00:00:36.540 --> 00:00:40.640 a Sun SPOT too loud too loud okay can you turn down just a little bit 8 00:00:40.640 --> 00:00:48.960 unless you look at it outside of the atmosphere it's really just a big yellow 9 00:00:48.960 --> 00:00:55.559 ball maybe with a sunspot or two across it but if I step out in a space and look 10 00:00:55.559 --> 00:01:00.870 at the Sun with a telescope that sees wavelengths that I can't see with my own 11 00:01:00.870 --> 00:01:11.070 eye this is what I see. This is the Sun and extreme ultraviolet seen from the 12 00:01:11.070 --> 00:01:16.049 Solar Dynamics Observatory and you can see it's so much more dynamic we have a 13 00:01:16.049 --> 00:01:22.500 huge explosion here this is billions of tons of solar material blasting away 14 00:01:22.500 --> 00:01:26.090 from the earth that millions of miles an hour called a coronal mass ejection 15 00:01:26.090 --> 00:01:32.189 filling the entire solar system we have a flash of light, light through the 16 00:01:32.189 --> 00:01:36.810 entire electromagnetic spectrum from radio all the way to gamma rays with 17 00:01:36.810 --> 00:01:41.970 enough power, enough energy to power the world for a hundred thousand years 18 00:01:41.970 --> 00:01:48.540 that's called a solar flare and both of those huge eruptions create massive 19 00:01:48.540 --> 00:01:53.640 shockwaves that accelerate particles at near the speed of light and all of this 20 00:01:53.640 --> 00:01:59.399 stuff fills the solar system and interacts with everything in it with 21 00:01:59.399 --> 00:02:04.189 planets with their atmospheres with their magnetic fields if they have them 22 00:02:04.189 --> 00:02:11.009 with asteroids and comets but also with the things and the people that we put 23 00:02:11.009 --> 00:02:17.430 into space with our spacecraft, with our astronauts and so we want to be 24 00:02:17.430 --> 00:02:23.819 able to understand this, maybe even predict it and have something similar to 25 00:02:23.819 --> 00:02:29.099 terrestrial whether. We actually call it space weather but we want to be able to 26 00:02:29.099 --> 00:02:35.519 protect our assets and protect the people as we send them back to the moon 27 00:02:35.519 --> 00:02:43.860 and beyond to Mars and because we have a new initiative now a new program Artemis 28 00:02:43.860 --> 00:02:51.629 to go back to the moon to send the next man and the first woman to step foot on 29 00:02:51.629 --> 00:02:59.329 the lunar surface we have a unique opportunity. We can now do unique science 30 00:02:59.329 --> 00:03:06.180 from the moon in particular unique science to understand this beast sitting 31 00:03:06.180 --> 00:03:09.239 at the inner in the beginning of us in this in the center of our solar system 32 00:03:09.239 --> 00:03:15.299 and understand better the influence that it has on us and protect those people 33 00:03:15.299 --> 00:03:18.060 that were sending to the moon and to Mars 34 00:03:18.060 --> 00:03:25.290 so next slide please, this is actually a really nice observation so here is the 35 00:03:25.290 --> 00:03:29.849 same spacecraft a different wavelength but extreme ultraviolet but look you see 36 00:03:29.849 --> 00:03:35.840 this object move in front of it okay that's the moon, that's the moon 37 00:03:35.840 --> 00:03:42.180 basically eclipsing the Sun we're seeing this from space and in fact we can use 38 00:03:42.180 --> 00:03:47.400 this opportunity to learn things about the moon itself these images are so 39 00:03:47.400 --> 00:03:53.340 detailed that when you see that shadow come past what you're actually seeing is 40 00:03:53.340 --> 00:03:58.260 if you look at the bottom it's not smooth right here there are little bumps 41 00:03:58.260 --> 00:04:03.449 on it you're actually seeing the moons of your see... sorry you're seeing the 42 00:04:03.449 --> 00:04:10.290 mountains of the moon when you look at this edge. So using a solar telescope 43 00:04:10.290 --> 00:04:14.190 we're actually learning something about the moon but we can turn this around 44 00:04:14.190 --> 00:04:20.209 because the moon gives us a unique perspective, next slide please 45 00:04:20.269 --> 00:04:25.409 we have some, we have a unique opportunity because sitting on the 46 00:04:25.409 --> 00:04:30.360 surface of the Moon we have no atmosphere, okay 47 00:04:30.360 --> 00:04:35.410 giving us the ability to observe these wavelengths of light that we can't see 48 00:04:35.410 --> 00:04:40.690 from the ground on the earth because they're stopped by our atmosphere those 49 00:04:40.690 --> 00:04:47.289 extreme ultraviolet or gamma rays or x-rays and also the moon does not have a 50 00:04:47.289 --> 00:04:54.430 magnetic field because not only do we see the light coming from the Sun all of 51 00:04:54.430 --> 00:04:58.240 those particles when they get to the Earth are affected by the magnetic field 52 00:04:58.240 --> 00:05:03.729 of the Earth they actually create a very interesting complicated environment for 53 00:05:03.729 --> 00:05:08.080 example creating the Van Allen radiation belts which we have to deal with as we 54 00:05:08.080 --> 00:05:15.520 fly through them away from the Earth so sitting on this object orbiting the 55 00:05:15.520 --> 00:05:22.770 earth we have a unique platform for us to observe the Sun and to observe the 56 00:05:22.770 --> 00:05:31.599 environment around the Sun. We can look at those huge blobs of material coronal 57 00:05:31.599 --> 00:05:37.110 mass ejections leaving the Sun. We can study the particles as they're reaching 58 00:05:37.110 --> 00:05:43.919 the Earth as they pass by the Moon, so if we go to the next slide please 59 00:05:44.610 --> 00:05:48.699 so what you're looking at here is the same explosion that I showed you at the 60 00:05:48.699 --> 00:05:55.479 very beginning and we're gonna back away from that, so you can see what happens 61 00:05:55.479 --> 00:06:02.889 when that object, those particles leave the Sun we have this background of 62 00:06:02.889 --> 00:06:06.940 particles called the solar wind that's always flowing away from the Sun and 63 00:06:06.940 --> 00:06:13.300 then on top of that you have this bigger cluster of particles that coronal mass 64 00:06:13.300 --> 00:06:20.759 ejection traveling from the Sun through the solar system and eventually 65 00:06:20.759 --> 00:06:29.530 interacting with objects in the solar system, here we see it passing Venus and 66 00:06:29.530 --> 00:06:33.970 you'll notice the particles are actually impinging the atmosphere of Venus 67 00:06:33.970 --> 00:06:39.460 directly because Venus doesn't have a magnetic field 68 00:06:39.460 --> 00:06:45.069 so they're moving straight impacting the atmosphere creating a unique environment 69 00:06:45.069 --> 00:06:52.690 and as they continue on and eventually reach the Earth now you see the 70 00:06:52.690 --> 00:06:57.099 particles are actually moving around it okay because the Earth's magnetic field 71 00:06:57.099 --> 00:07:04.530 is acting as a sort of force field protecting to somewhat the Earth 72 00:07:04.530 --> 00:07:10.240 creating a very interesting and complicated environment so when we sit 73 00:07:10.240 --> 00:07:15.490 on the Moon we don't have those aspects we don't have the atmosphere we don't 74 00:07:15.490 --> 00:07:20.050 have the magnetic fields but there are a couple of things that are unique about 75 00:07:20.050 --> 00:07:24.550 that environment, let's go to the next slide, let's actually skip ahead I want 76 00:07:24.550 --> 00:07:31.380 to pass this one and just skip to this so that magnetic field of the Earth and 77 00:07:31.380 --> 00:07:36.759 we're in this case the Sun is in this direction as it's coming as all those 78 00:07:36.759 --> 00:07:40.810 particles are coming past us they're stretching the magnetic field of the 79 00:07:40.810 --> 00:07:45.310 Earth creating this sort of elongated almost tadpole like structure we call 80 00:07:45.310 --> 00:07:52.750 this the magnetosphere, there are particles around it particles building 81 00:07:52.750 --> 00:07:57.070 up along the back part this is an incredibly complicated environment that 82 00:07:57.070 --> 00:08:04.419 our spacecraft and the ISS is traveling through but also in order to understand 83 00:08:04.419 --> 00:08:09.849 this we have a unique perspective with the Moon because in fact the Moon as 84 00:08:09.849 --> 00:08:15.449 it's orbiting the Earth it's actually passing in and out of this structure 85 00:08:15.449 --> 00:08:22.449 during the new moon when the Sun is over there and the Moon is directly on the 86 00:08:22.449 --> 00:08:27.430 other side of the Earth it's actually sitting right in here so for about six 87 00:08:27.430 --> 00:08:33.360 days the Moon orbits through the magnetosphere and allows us to sample 88 00:08:33.360 --> 00:08:37.990 what's happening in this unique environment and as the Moon moves around 89 00:08:37.990 --> 00:08:43.990 it we sample different parts of this whole structure we see different 90 00:08:43.990 --> 00:08:50.140 characteristics different environments and eventually for a full moon it's 91 00:08:50.140 --> 00:08:53.260 sitting over on this side almost completely out 92 00:08:53.260 --> 00:08:59.770 what we call the magnetosphere so we have this observing platform this 93 00:08:59.770 --> 00:09:06.040 natural observing platform that's moving around the magnetosphere allowing us to 94 00:09:06.040 --> 00:09:12.520 sample this hazardous complicated space that we have to travel through to 95 00:09:12.520 --> 00:09:18.880 measure the particles to measure the electric and magnetic fields to measure 96 00:09:18.880 --> 00:09:26.050 the plasma created in this whole structure and at the same time we're 97 00:09:26.050 --> 00:09:32.470 able to get a unique view of what's happening coming from the Sun as we are 98 00:09:32.470 --> 00:09:39.220 orbiting moving with the Moon as it's orbiting the Earth because again we have 99 00:09:39.220 --> 00:09:45.790 no atmosphere so now we can have very large powerful telescopes that we don't 100 00:09:45.790 --> 00:09:51.550 have to put into a spacecraft we can actually have on the body itself to 101 00:09:51.550 --> 00:09:58.450 allow us to study all that's happening from the Sun in multiple wavelengths of 102 00:09:58.450 --> 00:10:04.960 light measuring different types of particles different types of electric 103 00:10:04.960 --> 00:10:10.960 and magnetic fields structures to ultimately understand this kind of this 104 00:10:10.960 --> 00:10:16.330 very complicated environment that we have to travel through and that we have 105 00:10:16.330 --> 00:10:24.850 to ultimately live in as we bring people to the Moon and someday on to Mars so 106 00:10:24.850 --> 00:10:31.870 the Moon is providing something for us that is unique and exciting to allow us 107 00:10:31.870 --> 00:10:38.590 to understand the environment created by the Sun and as we understand that not 108 00:10:38.590 --> 00:10:43.810 only do we get a better handle on how to deal with it how to live with it how to 109 00:10:43.810 --> 00:10:49.330 travel through it but what we learn about our own Sun ultimately tells us 110 00:10:49.330 --> 00:10:55.090 about other stars other solar systems and the planets and bodies that are 111 00:10:55.090 --> 00:11:01.120 interacting with them so we're looking forward to 2024 and beyond as we start 112 00:11:01.120 --> 00:11:09.220 to explore this new unique environment to study our star and ultimately put 113 00:11:09.220 --> 00:11:14.950 other kinds of telescopes other kinds of instruments to study other stars other 114 00:11:14.950 --> 00:11:22.860 aspects of not just our solar system but the universe so thank you very much