Penumbral eclipse | |||||||||
![]() Penumbral eclipse as viewed from Oria, Italy, 18:54 UTC | |||||||||
Date | September 16, 2016 | ||||||||
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Gamma | 1.0548 | ||||||||
Magnitude | −0.0624 | ||||||||
Saros cycle | 147 (9 of 71) | ||||||||
Penumbral | 239 minutes, 17 seconds | ||||||||
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A penumbral lunar eclipse occurred at the Moon’s descending node of orbit on Friday, September 16, 2016,[1] with an umbral magnitude of −0.0624. 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 1.8 days before perigee (on September 18, 2016, at 13:00 UTC), the Moon's apparent diameter was larger.[2]