1
00:00:00,380 --> 00:00:03,480
A lunar eclipse as seen from Earth is leisurely,

2
00:00:03,480 --> 00:00:05,480
taking three hours or more.

3
00:00:05,780 --> 00:00:07,680
When the moon enters the umbra,

4
00:00:07,680 --> 00:00:11,760
a dark biteout appears and grows - the partial phase.

5
00:00:12,040 --> 00:00:14,860
When the moon is entirely inside the umbra,

6
00:00:14,860 --> 00:00:18,740
totality begins and can last for an hour or more.

7
00:00:19,500 --> 00:00:22,960
The moon appears red because the only light reaching it

8
00:00:22,960 --> 00:00:25,460
is refracted through Earth's atmosphere.

9
00:00:26,280 --> 00:00:30,880
One side may be brighter than the other because it is closer to the edge of the umbra.

10
00:00:31,560 --> 00:00:35,500
When part of the moon emerges from the umbra, totality is over.

11
00:00:35,960 --> 00:00:39,840
When all of the moon emerges, it's the end of the eclipse.