1 00:00:00,010 --> 00:00:04,120 [silence] 2 00:00:04,140 --> 00:00:08,170 [silence, followed by music] 3 00:00:08,190 --> 00:00:12,250 [music] Narrator: As the moon orbits the Earth, it occasionally passes through the Earth's shadow, resulting 4 00:00:12,270 --> 00:00:16,340 in a spectacular change in the moon's appearance for a short time. This event is called a 5 00:00:16,360 --> 00:00:20,420 lunar eclipse, and it happens at least twice a year, providing a rare show that's worth staying awake 6 00:00:20,440 --> 00:00:24,460 for. But what would a lunar eclipse look like if you were on the moon? From that perspective, 7 00:00:24,480 --> 00:00:28,510 you would actually be viewing a solar eclipse, with the Earth blocking the Sun for a short period of 8 00:00:28,530 --> 00:00:32,560 time. The view would be spectacular, but there's more to it than that. 9 00:00:32,580 --> 00:00:36,580 Having such a large-scale "lights out" on the moon gives scientists a unique opportunity to study 10 00:00:36,600 --> 00:00:40,600 the moon's surface, and NASA's Lunar Reconnaissance Orbiter is in a position to do just 11 00:00:40,620 --> 00:00:44,720 that. So, what exactly does LRO plan to study? When the Sun is 12 00:00:44,740 --> 00:00:48,830 obscured, the moon cools down, but not every area cools at the same rate. 13 00:00:48,850 --> 00:00:52,950 Rough areas of the moon, with large rocks and boulders, cool down more slowly than areas with fewer 14 00:00:52,970 --> 00:00:57,040 large rocks. By measuring the temperature of the moon as it cools, scientists can identify 15 00:00:57,060 --> 00:01:01,070 which areas are rougher than areas. Earth-based telescopes have been doing something like this 16 00:01:01,090 --> 00:01:05,110 for years, but they're so far away that it's hard to get a good view. LRO's DIVINER 17 00:01:05,130 --> 00:01:09,150 instrument, on the other hand, can measure temperature at an extremely high resolution, 18 00:01:09,170 --> 00:01:13,200 giving scientists a first-ever up-close measurement of this kind. By taking these 19 00:01:13,220 --> 00:01:17,220 measurements, scientists can infer the size and density of moon rocks on a very small scale, 20 00:01:17,240 --> 00:01:21,240 teaching them new things about the moon's surface. And while they might not be able to get 21 00:01:21,260 --> 00:01:25,360 a view of the solar eclipse from the moon, they'll still get a look at the moon that's just as exciting. 22 00:01:33,530 --> 00:01:29,460 [beeping]