1 00:00:00,600 --> 00:00:04,371 We learned a lot from the Apollo samples, but we still have a lot 2 00:00:04,371 --> 00:00:06,306 left to learn about the Moon. 3 00:00:06,306 --> 00:00:10,110 The Apollo missions visited only a pretty narrow swath of the Moon, 4 00:00:10,410 --> 00:00:13,413 all the missions were concentrated near the near side equator. 5 00:00:13,613 --> 00:00:15,815 Really interesting and really critical insights 6 00:00:15,815 --> 00:00:17,484 were unlocked with the Apollo samples, 7 00:00:17,484 --> 00:00:20,520 but we have so many questions still to answer about the Moon 8 00:00:20,520 --> 00:00:22,522 and the evolution of the Moon. 9 00:00:23,023 --> 00:00:29,896 [Dramatic music] 10 00:00:29,896 --> 00:00:31,965 Launch commentator: And liftoff of Artemis One! 11 00:00:31,965 --> 00:00:35,735 We rise together, back to the Moon and beyond. 12 00:00:37,337 --> 00:00:38,838 NASA's Artemis missions 13 00:00:38,838 --> 00:00:42,208 are NASA's plan to send people to the surface of the Moon. 14 00:00:42,442 --> 00:00:46,880 We'll be sending people and roving assets and scientific equipment 15 00:00:46,980 --> 00:00:50,083 to, among other things, answer a lot of really compelling science questions. 16 00:00:50,583 --> 00:00:52,685 Scientists have a lot to learn about the Moon. 17 00:00:52,685 --> 00:00:55,155 It's our nearest celestial neighbor here to Earth. 18 00:00:55,155 --> 00:00:57,724 So what the Moon has experienced, we've experienced, 19 00:00:57,724 --> 00:00:59,626 except here on Earth, we have things like plate 20 00:00:59,626 --> 00:01:03,830 tectonics, oceans, forests, people that erase the rock record. 21 00:01:03,963 --> 00:01:07,267 Whereas on the Moon, that whole record of our planet's history, of the Moon's 22 00:01:07,267 --> 00:01:10,370 history is just kind of waiting there at the surface for us to explore. 23 00:01:10,804 --> 00:01:13,773 The South Pole, which is where Artemis missions are going to target, 24 00:01:13,773 --> 00:01:16,776 is specifically interesting for a couple key reasons. 25 00:01:16,910 --> 00:01:17,911 We think there are volatiles 26 00:01:17,911 --> 00:01:20,747 at the South Pole of the Moon that are not present near the equator. 27 00:01:20,747 --> 00:01:23,983 Things like water and water ice that are trapped in the lunar regolith, 28 00:01:23,983 --> 00:01:28,288 which basically just means lunar soil, that can easily become untrapped from that 29 00:01:28,288 --> 00:01:31,691 lunar regolith and scientists can scoop up and study for return to Earth. 30 00:01:32,425 --> 00:01:35,495 The lunar South Pole is a really exciting scientific target, 31 00:01:35,495 --> 00:01:38,465 and it also comes with some challenges for operating. 32 00:01:38,465 --> 00:01:42,469 For example, the lighting environment will change drastically within the course 33 00:01:42,469 --> 00:01:46,139 of one mission and even over sometimes the course of one spacewalk. 34 00:01:46,306 --> 00:01:50,076 So preparing the crew members, preparing the hardware that we're sending 35 00:01:50,076 --> 00:01:53,713 to the Moon, and preparing the mission control teams is really, really important. 36 00:01:54,147 --> 00:01:56,516 The South Pole-Aitken Basin is particularly exciting. 37 00:01:56,516 --> 00:02:00,320 We think it's one of the oldest and largest impact basins in the solar system, 38 00:02:00,420 --> 00:02:04,090 and if we can get the right rock from the South Pole-Aitken Basin 39 00:02:04,090 --> 00:02:07,594 and bring it back to our labs here on Earth, we can use that sample 40 00:02:07,660 --> 00:02:11,197 to constrain the entire evolution of our solar system and really understand 41 00:02:11,197 --> 00:02:15,768 the timing of how the Moon and our planet and the entire solar system evolved. 42 00:02:15,768 --> 00:02:21,574 [Music]