1 00:00:00,000 --> 00:00:01,960 Music 2 00:00:01,960 --> 00:00:06,520 As you watch the Moon over the course of a month, you'll notice that different 3 00:00:06,529 --> 00:00:11,200 features are illuminated by the Sun at different times. However, there are some 4 00:00:11,210 --> 00:00:14,900 parts of the Moon that never see sunlight. These areas are called 5 00:00:14,900 --> 00:00:19,070 permanently shadowed regions, and they appear dark because unlike on the Earth, 6 00:00:19,070 --> 00:00:22,820 the axis of the Moon is nearly perpendicular to the direction of the 7 00:00:22,820 --> 00:00:27,140 Sun's light. The result is that the bottoms of certain craters, like here at 8 00:00:27,140 --> 00:00:31,279 the Moon's south pole, are never pointed toward the Sun, with some remaining dark 9 00:00:31,279 --> 00:00:35,989 for over two billion years. However, thanks to new data from NASA's Lunar 10 00:00:35,989 --> 00:00:39,829 Reconnaissance Orbiter, we can now see into these dark craters in incredible 11 00:00:39,829 --> 00:00:44,539 detail. Seeing the shape of the crater is important, and LRO has used its LOLA 12 00:00:44,539 --> 00:00:48,350 instrument to make the best yet topographical maps of these craters by 13 00:00:48,350 --> 00:00:52,609 reflecting lasers off the lunar surface. This has allowed us to see the shapes of 14 00:00:52,609 --> 00:00:57,319 the craters' interiors from any angle, and by making 3D models, we can light up the 15 00:00:57,319 --> 00:01:01,519 crater floors as if we had a giant flashlight. And although the Sun never 16 00:01:01,519 --> 00:01:05,960 illuminates these craters, other stars still cast a faint light into the 17 00:01:05,960 --> 00:01:11,240 permanent shadows. LRO's LAMP instrument can actually measure this light, giving 18 00:01:11,240 --> 00:01:15,470 us yet another view of this unique region on the Moon. LRO's DIVINER 19 00:01:15,470 --> 00:01:20,540 instrument can also measure temperature, revealing the extreme cold within the 20 00:01:20,540 --> 00:01:26,210 craters. Finally, LRO's LEND instrument can measure the speed of neutrons to 21 00:01:26,210 --> 00:01:30,800 detect elements like hydrogen in the lunar soil. So, while there are some areas 22 00:01:30,800 --> 00:01:35,450 on the Moon that never see the light of day, LRO will keep collecting data so 23 00:01:35,450 --> 00:01:39,200 that we can learn more about them. And as we continue to study the Moon, we'll 24 00:01:39,200 --> 00:01:43,370 improve our understanding of Earth's original satellite, and, pun fully 25 00:01:43,370 --> 00:01:46,360 intended, bring new discoveries to light. 26 00:01:46,360 --> 00:01:48,700 Music 27 00:01:48,700 --> 00:01:57,540 Beep, Beep, Beep