Penumbral eclipse | |||||||||
![]() The Moon barely clipped the northern penumbral shadow of the Earth. | |||||||||
Date | August 18, 2016 | ||||||||
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Gamma | 1.559 | ||||||||
Magnitude | −0.9925 | ||||||||
Saros cycle | 109 (72 of 72) | ||||||||
Penumbral | 33 minutes, 36 seconds | ||||||||
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A penumbral lunar eclipse occurred at the Moon’s descending node of orbit on Thursday, August 18, 2016,[1] with an umbral magnitude of −0.9925. 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 3.4 days before perigee (on August 21, 2016, at 21:20 UTC), the Moon's apparent diameter was larger.[2]
The HM National Almanac Office's online canon of eclipses lists this event as the last eclipse on Saros Series 109,[3] while NASA lists August 8, 1998 as the last eclipse of the series, and has this event missing the shadow.[4]
This eclipse grazed the northern boundary of the Earth's penumbral shadow. The event lasted 33 minutes and 36 seconds, beginning at 9:25 UTC and ending at 9:59. This produced a maximum penumbral magnitude of 0.0166.[5] Eclipses of such small magnitudes are visually imperceptible; a penumbral magnitude of approximately 0.6 is required for even skilled observers to detect.[6]
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