1 00:00:00,010 --> 00:00:04,120 Narrator: If you wanted to learn more about the history of the Earth and other rocky 2 00:00:04,140 --> 00:00:08,250 planets in the solar system, where would you look? For years, scientists have turned to 3 00:00:08,270 --> 00:00:12,360 one of the solar system's most common features: Impact craters. Left over 4 00:00:12,380 --> 00:00:16,470 from earlier periods of our planet's history, these sometimes giant holes in the surface can 5 00:00:16,490 --> 00:00:20,550 teach us about the Earth based on how they've changed over time. However, since even the newest 6 00:00:20,570 --> 00:00:24,630 impact craters on the Earth have changed due to wind, rain, snow, and even 7 00:00:24,650 --> 00:00:28,690 lakes filling them, we need to compare them to a fresh crater that still looks like it did when it was 8 00:00:28,710 --> 00:00:32,730 first created. So where exactly can scientists find a crater like this? Certainly 9 00:00:32,750 --> 00:00:36,770 not on Earth, but there's one on the Moon that's just about perfect. The Linné Crater, 10 00:00:36,790 --> 00:00:40,800 a small impact crater located in the western Mare Serenitatis, is extremely young, 11 00:00:40,820 --> 00:00:44,940 and scientists have always thought that it might be a great example to use to compare with other craters. 12 00:00:44,960 --> 00:00:49,090 Now, thanks to high-resolution, three-dimensional data generated from NASA's 13 00:00:49,110 --> 00:00:53,190 Lunar Reconnaissance Orbiter, scientists are sure of it. So why use a crater 14 00:00:53,210 --> 00:00:57,290 on the Moon, and why this specific example? Unlike craters on Earth--and even 15 00:00:57,310 --> 00:01:01,400 Mars--many Moon craters are well-preserved because they erode much more slowly. 16 00:01:01,420 --> 00:01:05,490 However, despite that, not all Moon craters are ideal for comparison. 17 00:01:05,510 --> 00:01:09,560 After a crater is first formed, it can be impacted again and again by other objects, 18 00:01:09,580 --> 00:01:13,640 which modify its original shape. This is why scientists have been looking for a crater 19 00:01:13,660 --> 00:01:17,710 that's not so beaten up, and one that preserves all the telltale signs of how impact cratering 20 00:01:17,730 --> 00:01:21,750 works. The Linné Crater fits the bill perfectly. By looking at 21 00:01:21,770 --> 00:01:25,780 data from LRO's LROC instrument, scientists have confirmed that it has remained largely 22 00:01:25,800 --> 00:01:29,810 untouched aside from normal wear and tear, which is what makes it so perfect for comparison. 23 00:01:29,830 --> 00:01:33,970 They've also discovered some interesting and unexpected things. For decades, 24 00:01:33,990 --> 00:01:38,110 lunar scientists counted on the simplest craters, like Linné, as being bowl-shaped. 25 00:01:38,130 --> 00:01:42,230 However, thanks to the new data, scientists have discovered that they actually resemble 26 00:01:42,250 --> 00:01:46,360 an upside-down cone. This, along with other findings, sheds new light not 27 00:01:46,380 --> 00:01:50,480 only on Linné Crater, but also on the evolution of similar craters on the Earth, Moon, 28 00:01:50,500 --> 00:01:54,540 and other planets, allowing us to get a better picture of our own history. In fact, 29 00:01:54,560 --> 00:01:58,610 the simple shape of Linné, and the way large boulders are strewn around its rim, are 30 00:01:58,630 --> 00:02:02,680 the basic tools of "forensic geology" that allow scientists to understand how craters started 31 00:02:02,700 --> 00:02:06,740 out on the Earth and Mars before water and wind wear them away. Without craters 32 00:02:06,760 --> 00:02:10,780 like Linné on the Moon, we wouldn't know how landforms evolve over time in the presence of weather, 33 00:02:10,800 --> 00:02:14,820 climate change, and other factors. And all by looking at what initially 34 00:02:14,840 --> 00:02:18,830 appears to be just another hole in the ground. 35 00:02:18,850 --> 00:02:22,970 [beeping] 36 00:02:22,990 --> 00:02:27,080 [beeping, silence]