1 00:00:00,266 --> 00:00:03,002 NASA's Artemis missions are NASA's plan 2 00:00:03,002 --> 00:00:05,155 to send people to the surface of the Moon. 3 00:00:05,366 --> 00:00:08,140 We'll be sending people and roving assets 4 00:00:08,140 --> 00:00:09,926 and scientific equipment 5 00:00:09,933 --> 00:00:11,611 to, among other things, answer a lot of 6 00:00:11,611 --> 00:00:13,063 really compelling science questions. 7 00:00:20,366 --> 00:00:22,433 Launch commentator: And liftoff of Artemis One! 8 00:00:22,433 --> 00:00:26,266 We rise together, back to the Moon and beyond. 9 00:00:27,100 --> 00:00:29,233 Scientists have a lot to learn about the Moon. 10 00:00:29,233 --> 00:00:31,700 It's our nearest celestial neighbor here to Earth. 11 00:00:31,700 --> 00:00:34,166 So what the Moon has experienced, we've experienced, 12 00:00:34,166 --> 00:00:36,966 except here on Earth, we have things like plate tectonics 13 00:00:36,966 --> 00:00:40,366 oceans, forests, people that erase the rock record. 14 00:00:40,500 --> 00:00:42,308 Whereas on the Moon, that whole record 15 00:00:42,308 --> 00:00:43,326 of our planet's history, 16 00:00:43,342 --> 00:00:45,127 of the Moon's history is just kind of waiting 17 00:00:45,133 --> 00:00:46,900 there at the surface for us to explore. 18 00:00:47,200 --> 00:00:49,532 The South Pole is specifically interesting 19 00:00:49,532 --> 00:00:51,184 for a couple key reasons. 20 00:00:51,266 --> 00:00:53,366 We think there are volatiles at the South Pole of the Moon 21 00:00:53,366 --> 00:00:55,133 that are not present near the equator. 22 00:00:55,133 --> 00:00:57,123 Things like water and water ice that are 23 00:00:57,123 --> 00:00:58,358 trapped in the lunar regolith, 24 00:00:58,433 --> 00:01:00,443 that can easily become untrapped 25 00:01:00,443 --> 00:01:01,461 from that lunar regolith 26 00:01:01,466 --> 00:01:03,366 and scientists can scoop up and study. 27 00:01:03,566 --> 00:01:05,063 The South Pole-Aitken Basin is one of the 28 00:01:05,063 --> 00:01:06,166 oldest and largest 29 00:01:06,166 --> 00:01:07,833 impact basins in the solar system, 30 00:01:07,966 --> 00:01:10,119 and if we can get the right rock 31 00:01:10,119 --> 00:01:12,121 from the South Pole-Aitken Basin and bring it back 32 00:01:12,133 --> 00:01:15,000 to our labs here on Earth, we can use that sample 33 00:01:15,066 --> 00:01:17,692 to constrain the entire evolution of our solar system 34 00:01:17,692 --> 00:01:20,395 and really understand the timing of how the Moon 35 00:01:20,400 --> 00:01:22,966 and our planet and the entire solar system evolved.