April 2052 lunar eclipse
| Penumbral eclipse | |||||||||
The Moon's hourly motion shown right to left | |||||||||
| Date | April 14, 2052 | ||||||||
|---|---|---|---|---|---|---|---|---|---|
| Gamma | 1.0628 | ||||||||
| Magnitude | −0.1294 | ||||||||
| Saros cycle | 142 (20 of 73) | ||||||||
| Penumbral | 276 minutes, 0 seconds | ||||||||
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A penumbral lunar eclipse will occur at the Moon’s ascending node of orbit on Sunday, April 14, 2052, with an umbral magnitude of −0.1294. A lunar eclipse occurs when the Moon moves into the Earth's shadow, causing the Moon to be darkened. A penumbral lunar eclipse occurs when part or all of the Moon's near side passes into the Earth's penumbra. Unlike a solar eclipse, which can only be viewed from a relatively small area of the world, a lunar eclipse may be viewed from anywhere on the night side of Earth. Occurring about 2.4 days before apogee (on April 16, 2052, at 13:00 UTC), the Moon's apparent diameter will be smaller.