WEBVTT 1 00:00:06.956 --> 00:00:10.867 A total solar eclipse is an extraordinary event. 2 00:00:11.358 --> 00:00:12.600 For a few minutes, 3 00:00:12.774 --> 00:00:15.360 night falls in the middle of the day! 4 00:00:15.385 --> 00:00:17.660 How is this possible? 5 00:00:17.685 --> 00:00:18.974 In astronomy, 6 00:00:18.999 --> 00:00:21.957 an eclipse occurs when one celestial body 7 00:00:21.982 --> 00:00:24.144 moves into the shadow of another, 8 00:00:24.169 --> 00:00:26.777 blocking out some or all of its light. 9 00:00:27.232 --> 00:00:28.335 On Earth, 10 00:00:28.360 --> 00:00:30.693 this can happen on two occasions: 11 00:00:30.718 --> 00:00:33.025 The Moon can pass behind the Earth 12 00:00:33.050 --> 00:00:35.271 and cross the Earth's shadow cone. 13 00:00:35.706 --> 00:00:39.587 Or the Moon can pass between the Sun and the Earth, 14 00:00:39.612 --> 00:00:43.103 and it is the Earth that crosses the Moon's shadow cone. 15 00:00:43.128 --> 00:00:45.302 What do we see on Earth? 16 00:00:45.706 --> 00:00:47.712 During a lunar eclipse, 17 00:00:47.737 --> 00:00:50.197 the observer is on the night side. 18 00:00:50.222 --> 00:00:53.362 The night is clear beacause the Moon is full. 19 00:00:53.818 --> 00:00:54.965 But suddenly 20 00:00:54.990 --> 00:00:58.910 a shadow moves in and seems to nibble at the moon. 21 00:00:58.935 --> 00:01:02.255 It's the Earth's shadow blocking the sunlight. 22 00:01:04.848 --> 00:01:08.090 A total eclipse is much more impressive 23 00:01:08.115 --> 00:01:11.058 because it happens during the day. 24 00:01:11.083 --> 00:01:13.036 The moon moves slowly 25 00:01:13.061 --> 00:01:16.840 and positions itself between the sun and our eyes. 26 00:01:16.865 --> 00:01:20.081 Its shadow is cast on the Earth. 27 00:01:20.414 --> 00:01:23.871 An observer cannot see the moon moving in front of the Sun 28 00:01:23.896 --> 00:01:26.449 because the Sun is much too bright. 29 00:01:26.474 --> 00:01:28.193 To see it, 30 00:01:28.218 --> 00:01:30.277 one must wear protective glasses. 31 00:01:30.302 --> 00:01:32.152 When the alignment is perfect 32 00:01:32.177 --> 00:01:34.808 and the solar disk is completely obscured, 33 00:01:34.833 --> 00:01:37.855 darkness suddenly sets in. 34 00:01:37.880 --> 00:01:42.074 This is the only moment allowed to remove the protective glasses 35 00:01:42.099 --> 00:01:46.465 and experience the magic of a total solar eclipse. 36 00:01:46.490 --> 00:01:49.199 The moon covers the sun perfectly 37 00:01:49.224 --> 00:01:52.285 and a thin, bright crown surrounds it. 38 00:01:52.310 --> 00:01:54.980 This is the solar corona. 39 00:01:55.005 --> 00:01:58.669 It's not the eclipse that causes this appearance. 40 00:01:58.694 --> 00:02:01.407 The corona is always present. 41 00:02:01.484 --> 00:02:03.652 The occultation of the solar disk 42 00:02:03.677 --> 00:02:08.691 reveals this outer layer of the solar atmosphere to our eyes. 43 00:02:08.716 --> 00:02:13.199 The conditions that allow you to see a total solar eclipse are rare: 44 00:02:13.224 --> 00:02:13.902 First, 45 00:02:13.927 --> 00:02:19.488 the alignment between the Sun, the Moon, and the observer must be perfect, 46 00:02:19.513 --> 00:02:23.004 otherwise the moon will only cover part of the Sun. 47 00:02:23.029 --> 00:02:25.582 The sky will darken, but not completely. 48 00:02:25.607 --> 00:02:27.496 This is a partial eclipse, 49 00:02:27.521 --> 00:02:30.568 and the observer cannot remove his protective glasses 50 00:02:30.593 --> 00:02:32.652 at any time while looking at the Sun. 51 00:02:32.677 --> 00:02:35.996 Because the Moon's orbit is slightly elliptical, 52 00:02:36.021 --> 00:02:39.355 the distance between the Earth and the moon varies. 53 00:02:39.380 --> 00:02:42.480 If the Moon is too far away at the time of alignment, 54 00:02:42.505 --> 00:02:44.824 an annular eclipse is observed. 55 00:02:44.849 --> 00:02:46.959 and some brightness remains 56 00:02:47.505 --> 00:02:49.277 If the Moon is too close, 57 00:02:49.302 --> 00:02:53.543 its apparent diameter will be larger than that of the Sun. 58 00:02:53.568 --> 00:02:58.621 The eclipse is total, but the solar corona is not visible. 59 00:02:58.646 --> 00:03:00.027 The last condition, 60 00:03:00.052 --> 00:03:03.262 is to be lucky enough to be in the right place 61 00:03:03.287 --> 00:03:05.685 on the narrow path of totality. 62 00:03:05.710 --> 00:03:08.308 Finally, an amazing coincidence 63 00:03:08.333 --> 00:03:11.826 makes the eclipse absolutely incredible. 64 00:03:11.851 --> 00:03:15.420 The Moon is 400 times smaller than the Sun, 65 00:03:15.445 --> 00:03:20.029 but it also happens to be 400 times closer. 66 00:03:20.054 --> 00:03:21.123 In other words, 67 00:03:21.148 --> 00:03:23.793 the Earth is in the unique position 68 00:03:23.818 --> 00:03:26.058 that allows the lunar disk to appear 69 00:03:26.083 --> 00:03:28.782 the same size as the solar disk. 70 00:03:30.537 --> 00:03:33.389 If a total solar eclipse is happening nearby, 71 00:03:33.414 --> 00:03:36.070 you do not want to miss such an event. 72 00:03:36.148 --> 00:03:39.117 The next one will probably be a century later. 73 00:03:39.142 --> 00:03:41.273 And don't forget your glasses