August 2053 lunar eclipse
| Penumbral eclipse | |||||||||
The Moon's hourly motion shown right to left | |||||||||
| Date | August 29, 2053 | ||||||||
|---|---|---|---|---|---|---|---|---|---|
| Gamma | 1.0165 | ||||||||
| Magnitude | −0.0319 | ||||||||
| Saros cycle | 119 (64 of 83) | ||||||||
| Penumbral | 277 minutes, 51 seconds | ||||||||
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A penumbral lunar eclipse will occur at the Moon’s descending node of orbit on Friday, August 29, 2053, with an umbral magnitude of −0.0319. It will be a relatively rare total penumbral lunar eclipse, with the Moon passing entirely within the penumbral shadow without entering the darker umbral shadow. 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 4.7 days after apogee (on August 24, 2053, at 14:30 UTC), the Moon's apparent diameter will be smaller.