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.