WEBVTT FILE 1 00:00:00.000 --> 00:00:02.000 Humming sound 2 00:00:02.000 --> 00:00:09.220 Music 3 00:00:09.220 --> 00:00:12.075 Since the 1960's, scientists have suspected that 4 00:00:12.075 --> 00:00:15.115 frozen water could survive in permanently shadowed craters 5 00:00:15.115 --> 00:00:18.165 at the Moon's poles. Both hydrogen and oxygen 6 00:00:18.165 --> 00:00:20.555 could be trapped within the lunar soil. 7 00:00:20.795 --> 00:00:23.115 So to find water on the Moon, scientists 8 00:00:23.115 --> 00:00:26.025 are looking for indications of hydrogen using the Lunar 9 00:00:26.025 --> 00:00:28.885 Reconnaissance Orbiter's LEND neutron detector. 10 00:00:29.125 --> 00:00:32.185 By observing the interaction of neutrons with the lunar soil, 11 00:00:32.185 --> 00:00:35.640 scientists can interpret how much hydrogen is likely to be present. 12 00:00:35.900 --> 00:00:38.385 In order to make a detailed interpretation, however, 13 00:00:38.385 --> 00:00:41.840 LEND needs to observe a large number of neutrons 14 00:00:42.565 --> 00:00:45.135 Because LRO is constantly moving, LEND is never over 15 00:00:45.135 --> 00:00:48.075 one place long enough to count many neutrons. 16 00:00:48.075 --> 00:00:51.085 So, to make a detailed interpretation of neutron flux, 17 00:00:51.085 --> 00:00:54.680 scientists add together many measurements from many orbits. 18 00:00:55.300 --> 00:00:58.300 With each orbit LEND's dataset gets larger 19 00:00:58.305 --> 00:01:01.105 and its picture of neutron flux continually improves 20 00:01:01.105 --> 00:01:04.620 over time. The dark blue regions in this visualization 21 00:01:04.620 --> 00:01:07.015 are places on the south pole of the Moon with a 22 00:01:07.015 --> 00:01:10.425 suppressed flux of neutrons because of their interaction of hydrogen. 23 00:01:10.795 --> 00:01:13.555 These areas strongly suggest the presence of water 24 00:01:13.555 --> 00:01:15.005 frozen within the soil. 25 00:01:15.005 --> 00:01:16.285 Music 26 00:01:16.285 --> 00:01:19.295 While previous lunar missions have observed indications of hydrogen 27 00:01:19.300 --> 00:01:22.720 at the Moon's south pole, the LEND measurements for the first time 28 00:01:22.720 --> 00:01:24.775 pinpoint where hydrogen, and thus water, 29 00:01:24.775 --> 00:01:26.335 is likely to exist. 30 00:01:27.005 --> 00:01:29.755 By combining years of LEND data, scientists 31 00:01:29.755 --> 00:01:33.065 see accumulating evidence that there is water on the Moon. 32 00:01:33.505 --> 00:01:36.045 And as LRO continues to return data, 33 00:01:36.045 --> 00:01:39.315 our picture of the Moon and its water will continue to get better 34 00:01:39.315 --> 00:01:40.695 in the years ahead. 35 00:01:40.700 --> 00:01:44.560 Music 36 00:01:44.600 --> 00:01:49.760 Beep, Beep, Beep 37 00:01:49.760 --> 00:01:53.600 Music