1 00:00:00,100 --> 00:00:03,766 The great thing about a lunar eclipse is that you don't need special equipment, 2 00:00:03,766 --> 00:00:06,366 and you don't need to be in a particular location. 3 00:00:06,366 --> 00:00:09,433 Everybody in the United States is going to be able to see this. 4 00:00:09,800 --> 00:00:12,400 They just need to go outside and locate the Moon. 5 00:00:12,400 --> 00:00:15,500 So a total lunar eclipse happens when the Sun, the Earth, 6 00:00:15,500 --> 00:00:17,133 and the Moon are aligned. 7 00:00:17,133 --> 00:00:21,000 The Moon goes around the Earth once a month, but we don't get an eclipse 8 00:00:21,000 --> 00:00:24,266 every month because the Moon's orbit is a little bit tilted. 9 00:00:25,233 --> 00:00:28,066 We get that alignment about every six months. 10 00:00:28,066 --> 00:00:31,800 And so the Earth's shadow stretches across 11 00:00:31,800 --> 00:00:35,133 240,000 miles and lands on the Moon. 12 00:00:35,500 --> 00:00:39,366 Eclipses don't happen every month because the Moon's orbit is tilted 13 00:00:39,366 --> 00:00:40,766 by about five degrees. 14 00:00:40,766 --> 00:00:45,133 And so some months during the full Moon, it's going to pass a little bit 15 00:00:45,133 --> 00:00:46,666 above the Earth's shadow. 16 00:00:46,666 --> 00:00:49,800 And some months it's going to pass a little bit below. About once 17 00:00:49,800 --> 00:00:52,933 every six months, it actually passes through the Earth's shadow. 18 00:00:53,433 --> 00:00:56,533 Now it doesn't hit the middle of that shadow every time. 19 00:00:56,533 --> 00:00:59,233 So some lunar eclipses are just partial. 20 00:00:59,233 --> 00:01:03,766 But every year or year and a half, we get a total lunar eclipse 21 00:01:03,766 --> 00:01:06,766 where the Moon passes through the center of the Earth's shadow, 22 00:01:06,900 --> 00:01:09,900 and every part of the Moon is blocked from the Sun. 23 00:01:10,000 --> 00:01:13,000 The best thing about a lunar eclipse is that it's beautiful. 24 00:01:13,033 --> 00:01:18,366 So the Moon during totality will turn shades of orange and red and brown. 25 00:01:18,700 --> 00:01:23,800 It's being hit by all of the sunrises and sunsets projected from the Earth.