WEBVTT FILE 1 00:00:00.133 --> 00:00:03.169 My name is Kelsey Young, and my role with the Artemis missions 2 00:00:03.169 --> 00:00:06.272 is, I am the Artemis Science Flight Operations Lead. 3 00:00:06.873 --> 00:00:10.143 What that means is I'm responsible for making sure that science, 4 00:00:10.143 --> 00:00:13.113 all of our science objectives, are incorporated into the Artemis 5 00:00:13.179 --> 00:00:16.182 missions from a perspective of the flight control team. 6 00:00:16.449 --> 00:00:19.652 Do we have science representation on the flight control team? Does 7 00:00:19.652 --> 00:00:23.156 that science team have the infrastructure that they need to be successful? 8 00:00:23.423 --> 00:00:26.793 How will Artemis astronauts accomplish science objectives? 9 00:00:26.793 --> 00:00:27.894 How will they be trained? 10 00:00:27.894 --> 00:00:31.364 How will we design traverses around science objectives? 11 00:00:31.631 --> 00:00:34.200 So my role as the Artemis Science Flight Operations Lead 12 00:00:34.200 --> 00:00:37.437 is really to make sure that science has the right role 13 00:00:37.437 --> 00:00:40.440 to play in the operations of these exciting Artemis missions. 14 00:00:41.374 --> 00:00:44.110 For Artemis II, my role on the Artemis II mission is 15 00:00:44.110 --> 00:00:46.913 I am the lead for the lunar science objectives for the mission. 16 00:00:46.913 --> 00:00:50.650 So when the crew are flying by the moon, they'll be taking pictures, 17 00:00:50.650 --> 00:00:52.619 of course, out the window at the lunar surface. 18 00:00:52.619 --> 00:00:54.487 They'll be making observations, 19 00:00:54.487 --> 00:00:57.490 and my role is to lead those lunar science objectives. 20 00:00:58.258 --> 00:01:00.994 The JETT5 mission was the highest fidelity Artemis 21 00:01:00.994 --> 00:01:03.897 III surface mission simulation to date. 22 00:01:03.897 --> 00:01:06.933 It included a science team that works both before the mission 23 00:01:06.933 --> 00:01:08.001 and during the mission, 24 00:01:08.001 --> 00:01:11.638 to insert science objectives in as high a fidelity way as possible. 25 00:01:11.871 --> 00:01:14.607 What that science team did was, before the mission happened, 26 00:01:14.607 --> 00:01:18.178 they interrogated the landing site with, of course, their science glasses on. 27 00:01:18.378 --> 00:01:20.447 What science questions did they want to answer? 28 00:01:20.447 --> 00:01:23.783 Where do they want the crew member to go to address those science objectives? 29 00:01:24.050 --> 00:01:27.587 And the EVA, or spacewalk, traverses were built in large part 30 00:01:27.587 --> 00:01:29.422 around those science objectives. 31 00:01:29.422 --> 00:01:33.460 During the JETT5 test, that same science team supported the EVA’s 32 00:01:33.460 --> 00:01:35.595 from Mission Control in Houston. 33 00:01:35.595 --> 00:01:39.032 So they were able to provide science guidance up to the crew 34 00:01:39.132 --> 00:01:42.068 on where to sample, how to best address the science objectives, 35 00:01:42.068 --> 00:01:44.904 and how to maximize the return from the JETT5 mission, 36 00:01:44.904 --> 00:01:48.241 just like they'll be doing with the Artemis III mission to the lunar south pole. 37 00:01:49.309 --> 00:01:50.310 Mission simulations like 38 00:01:50.310 --> 00:01:54.781 JETT5 are so critical to prepare the team for Artemis surface exploration. 39 00:01:54.781 --> 00:01:57.484 It's critical to test the hardware, like the geology 40 00:01:57.484 --> 00:02:00.553 sampling tools in these high fidelity analog environments, 41 00:02:00.787 --> 00:02:03.756 but it's also really important to prepare the ground teams, the flight 42 00:02:03.756 --> 00:02:07.193 control team, and specifically the science team for what it's going to be like 43 00:02:07.293 --> 00:02:10.730 to actually be conducting these science operations on the lunar surface. 44 00:02:11.064 --> 00:02:14.033 For example, how should the science team structure themselves? 45 00:02:14.033 --> 00:02:17.637 How do they insert that science guidance, those science recommendations, 46 00:02:17.637 --> 00:02:20.340 up into the rest of the mission control team? 47 00:02:20.340 --> 00:02:23.176 How do we develop the ground support infrastructure, 48 00:02:23.176 --> 00:02:26.079 the tools that we need to work in mission control? 49 00:02:26.079 --> 00:02:27.914 These mission simulations are really critical 50 00:02:27.914 --> 00:02:30.984 to give us these testing opportunities, to allow us to figure out how our 51 00:02:30.984 --> 00:02:31.851 teams will operate. 52 00:02:32.919 --> 00:02:33.386 The San 53 00:02:33.386 --> 00:02:37.223 Francisco volcanic field is the field site for the JETT5 mission simulation. 54 00:02:37.223 --> 00:02:40.527 It's near Flagstaff, Arizona, which is an area that's actually long 55 00:02:40.527 --> 00:02:44.497 been used as an analog for preparing for planetary surface exploration. 56 00:02:45.031 --> 00:02:48.835 Apollo crews trained not too far away from where the JETT5 mission simulation 57 00:02:48.835 --> 00:02:53.273 occurred, and that San Francisco volcanic field was chosen in large part 58 00:02:53.273 --> 00:02:55.108 because the terrain, you know, 59 00:02:55.108 --> 00:02:58.211 mimics the lunar surface in a lot of really critical ways. 60 00:02:58.511 --> 00:03:03.449 It has the sci - the types of science objectives accessible to mission 61 00:03:03.449 --> 00:03:08.188 simulation crews that Apollo and Artemis astronauts have answered and will answer. 62 00:03:08.755 --> 00:03:10.957 It's the right scale of exploration. 63 00:03:10.957 --> 00:03:14.327 So the science targets, the EVA targets, the spacewalk targets 64 00:03:14.527 --> 00:03:18.498 are at the right scale of exploration that Artemis astronauts will experience. 65 00:03:18.565 --> 00:03:22.936 So it gives us a really high fidelity and robust way to test our hardware 66 00:03:22.936 --> 00:03:25.738 and our infrastructure in a high fidelity environment. 67 00:03:25.738 --> 00:03:29.108 And for me, as a scientist, it's really exciting because it enables us 68 00:03:29.108 --> 00:03:32.579 to ask robust and compelling science questions 69 00:03:32.745 --> 00:03:35.515 that our crew members for JETT5 will have to answer 70 00:03:35.515 --> 00:03:39.085 and have to rely on the science team real time to help them answer, 71 00:03:39.285 --> 00:03:42.922 which makes it a really ideal testing opportunity to start to prepare for the 72 00:03:42.922 --> 00:03:43.823 Artemis missions. 73 00:03:44.924 --> 00:03:47.994 The JETT5 EVA’s, or spacewalks, the traverses 74 00:03:47.994 --> 00:03:50.163 that the astronauts were running out in the field, 75 00:03:50.163 --> 00:03:53.032 were designed in part around science objectives. 76 00:03:53.032 --> 00:03:56.803 They included astronauts visiting sites of interest 77 00:03:56.803 --> 00:04:01.407 from a scientific perspective, collecting samples, collecting samples of the rocks 78 00:04:01.407 --> 00:04:04.677 in the regolith in the area to answer science questions 79 00:04:04.677 --> 00:04:07.981 that the science team was really excited to have the astronauts perspective on. 80 00:04:08.381 --> 00:04:12.952 We conducted some of the JETT5 EVA’s during the day and some of them at night, 81 00:04:12.986 --> 00:04:17.056 and the reason for that was to test a variety of lighting conditions. 82 00:04:17.390 --> 00:04:20.693 One of the exciting things about exploration at the lunar south pole 83 00:04:20.693 --> 00:04:23.496 is that the lighting environment is really dynamic. 84 00:04:23.496 --> 00:04:27.533 The sun is going to be moving within the course of one surface mission, 85 00:04:27.533 --> 00:04:29.502 and the astronauts will have to be prepared 86 00:04:29.502 --> 00:04:32.171 to encounter a variety of different lighting environments. 87 00:04:32.171 --> 00:04:35.275 So by testing some during the day and some at night, it enables 88 00:04:35.275 --> 00:04:38.711 our teams to prepare for everything that Artemis astronauts might experience. 89 00:04:39.812 --> 00:04:41.247 The JETT5 EVA’s were 90 00:04:41.247 --> 00:04:45.018 conducted with astronauts in the field out in Arizona in our test site, 91 00:04:45.184 --> 00:04:48.421 but they were supported by a mission control team back on Earth, 92 00:04:48.488 --> 00:04:51.624 so to speak, which in this case meant Houston, Texas, in Mission Control. 93 00:04:51.858 --> 00:04:56.129 So we had a full EVA flight control team supporting the JETT5 EVA’s, 94 00:04:56.362 --> 00:04:59.332 the traverses as they were conducted, and as a part of that flight 95 00:04:59.332 --> 00:05:02.568 control team, we had a full science team in the loop as well. 96 00:05:02.835 --> 00:05:07.140 So just like we expect for future Artemis missions, we had a science back room 97 00:05:07.140 --> 00:05:11.678 full of lunar scientists and geologists providing guidance to the crew real time, 98 00:05:12.178 --> 00:05:15.448 and we also had a science flight controller embedded in the EVA 99 00:05:15.448 --> 00:05:18.718 flight control team as that sort of senior voice for science 100 00:05:18.718 --> 00:05:21.287 within the rest of the EVA flight control disciplines. 101 00:05:22.322 --> 00:05:23.856 The Science Evaluation 102 00:05:23.856 --> 00:05:26.859 Room is the science back room for Artemis missions. 103 00:05:26.859 --> 00:05:31.531 And we actually had that science back room populated for the JETT5 EVA’s as well. 104 00:05:31.898 --> 00:05:35.101 What the science back room, or Science Evaluation Room for Artemis 105 00:05:35.201 --> 00:05:39.272 is, is actually the brain trust of lunar scientists and geologists 106 00:05:39.505 --> 00:05:43.543 who are responsible for accomplishing our lunar science and lunar surface science 107 00:05:43.543 --> 00:05:47.680 and geologic observations and objectives during each Artemis mission. 108 00:05:48.014 --> 00:05:51.684 In that room, we have a whole host of the lunar science 109 00:05:51.684 --> 00:05:56.356 and geology community represented, and their job is to feed insights 110 00:05:56.356 --> 00:05:59.859 and recommendations up to the crew during a mission to make sure 111 00:05:59.859 --> 00:06:03.162 that those objectives are represented and accomplished throughout the mission. 112 00:06:03.429 --> 00:06:06.199 So it's really kind of where the lunar science magic happens 113 00:06:06.199 --> 00:06:08.401 within the Flight Control team and within Mission Control 114 00:06:08.401 --> 00:06:10.036 back on Earth during an Artemis mission. 115 00:06:11.070 --> 00:06:14.507 The Science Evaluation Room, or science back room, for an Artemis mission 116 00:06:14.507 --> 00:06:18.611 has a lot of different kind of roles and expertise represented within it. 117 00:06:18.845 --> 00:06:22.448 You have lunar scientists, you have geologists, you have experts 118 00:06:22.448 --> 00:06:25.618 in imagery and imagery analysis because images are, 119 00:06:25.618 --> 00:06:29.355 of course, a critical data set for the science community after a mission. 120 00:06:29.655 --> 00:06:32.692 You have experts in sample science, people who are really wanting 121 00:06:32.725 --> 00:06:35.161 to study the samples when they return to Earth. 122 00:06:35.161 --> 00:06:40.600 You have software experts and lunar data experts all working together to make sure 123 00:06:40.600 --> 00:06:41.367 that the science 124 00:06:41.367 --> 00:06:44.370 objectives, the lunar science objectives of that mission accomplished, 125 00:06:44.537 --> 00:06:45.905 and that science expertise 126 00:06:45.905 --> 00:06:48.908 can be injected through the Flight Control team real time. 127 00:06:49.542 --> 00:06:51.611 Artemis lunar science objectives will include 128 00:06:51.611 --> 00:06:55.047 those accomplished through geology, through geologic sampling. 129 00:06:55.047 --> 00:06:59.185 We’ll be using geology tools, like a rock hammer, to get samples in situ 130 00:06:59.185 --> 00:07:00.920 to collect for return to Earth. 131 00:07:00.920 --> 00:07:01.988 But they'll also include 132 00:07:01.988 --> 00:07:06.459 science payloads or science instruments that crew deploy on the lunar surface, 133 00:07:06.492 --> 00:07:10.897 but that return data back to the science teams for those instruments on Earth. 134 00:07:11.130 --> 00:07:14.567 So the lunar science team, the Artemis mission science teams, 135 00:07:14.734 --> 00:07:19.372 will include those representing geology, lunar science, the lunar science payloads, 136 00:07:19.372 --> 00:07:22.775 and they'll all be working together to accomplish the lunar science objectives. 137 00:07:23.576 --> 00:07:27.346 It takes a lot of work to create a geology and science 138 00:07:27.346 --> 00:07:30.683 well-trained crew member, and we do that in a number of different settings. 139 00:07:30.683 --> 00:07:32.819 We do it in the classroom, we do it in the field, 140 00:07:32.819 --> 00:07:36.789 we do it through mission simulations, and we do it by pulling on science 141 00:07:36.789 --> 00:07:39.859 community members from across the number of science disciplines 142 00:07:39.859 --> 00:07:42.228 for which we have Artemis science objectives. 143 00:07:42.228 --> 00:07:45.331 Definitely takes a science village to create that well-trained crew member, 144 00:07:45.431 --> 00:07:47.200 and we're fortunate to have those well-trained 145 00:07:47.200 --> 00:07:50.236 crew members as our science team proxies on the lunar surface.