WEBVTT FILE 1 00:00:00.000 --> 00:00:04.020 music 2 00:00:04.040 --> 00:00:08.160 What we're talking about is several visualizations of 3 00:00:08.180 --> 00:00:12.360 path of the Moon's shadow during the eclipse in 2017. 4 00:00:12.380 --> 00:00:16.530 Everything in it is driven by the data, so the color of the 5 00:00:16.550 --> 00:00:20.700 ground, the position of the path of totality, the lighting from the sun, 6 00:00:20.720 --> 00:00:24.840 the sun angle. All of those are things that are based on data. 7 00:00:24.860 --> 00:00:28.930 A lot of NASA products were used to create this visualization. I used the 8 00:00:28.950 --> 00:00:33.100 Lunar Reconnaissance Orbiter--the laser altimetry data from that-- 9 00:00:33.120 --> 00:00:37.290 which gives us a digital map of the elevations on the Moon. 10 00:00:37.310 --> 00:00:41.360 For the Earth I used something called SRTM, this was a radar that was flown on the space shuttle. 11 00:00:41.380 --> 00:00:45.440 For the positions of the Earth, the Moon, and the sun, 12 00:00:45.460 --> 00:00:49.590 I used a JPL ephemeris. An ephemeris is just a list 13 00:00:49.610 --> 00:00:53.790 of positions, but it's the most accurate tabulation 14 00:00:53.810 --> 00:00:57.980 of those positions. This visualization is unique because it shows the effect of both 15 00:00:58.000 --> 00:01:02.090 the irregular edge of the Moon, the limb of the Moon, 16 00:01:02.110 --> 00:01:06.190 we call it, and the elevation of the observer. Now, we've known for a long time 17 00:01:06.210 --> 00:01:10.230 that the elevation of the observer affects where the shadow is, 18 00:01:10.250 --> 00:01:14.400 and we've also known that the mountains and the valleys along the edge 19 00:01:14.420 --> 00:01:18.540 of the Moon affect the shadow. So, you may have seen 20 00:01:18.560 --> 00:01:22.710 eclipse maps in the past that the image of the umbra, 21 00:01:22.730 --> 00:01:26.830 that shape of the shadow on the Earth, is drawn as a smooth oval, but 22 00:01:26.850 --> 00:01:30.950 we know that the Moon isn't smooth. Around the edge of the Moon, we have these sort of 23 00:01:30.970 --> 00:01:35.020 jagged peaks and valleys. And a peak can block the sun a little bit 24 00:01:35.040 --> 00:01:39.100 earlier than we thought, and a valley can let the sun in a few seconds 25 00:01:39.120 --> 00:01:43.220 longer than we thought. The combined effect of these peaks and valleys is to 26 00:01:43.240 --> 00:01:47.370 create a shape that is not really an oval, it's more like a polygon. 27 00:01:47.390 --> 00:01:51.430 But it hasn't actually been seen in exactly this way before 28 00:01:51.450 --> 00:01:55.550 where we calculate those circumstances for every point on the map. 29 00:01:55.570 --> 00:01:59.680 and draw that shape. Totality is that 30 00:01:59.700 --> 00:02:03.750 two minutes--or two and a half minutes--when the Moon completely 31 00:02:03.770 --> 00:02:07.860 covers the sun. The sudden darkness of totality is just something 32 00:02:07.880 --> 00:02:12.010 that a lot of people can't compare to anything else. 33 00:02:12.030 --> 00:02:16.160 I love the idea that I'm giving this kind of map to other people, and especially that 34 00:02:16.180 --> 00:02:20.360 it's more detailed and more accurate, so that people are actually in the right place 35 00:02:20.380 --> 00:02:24.400 to see it. 36 00:02:24.420 --> 00:02:28.580 tone 37 00:02:28.600 --> 00:02:32.670 beeping 38 00:02:32.690 --> 00:02:33.834 beeping