August 2016 lunar eclipse

August 2016 lunar eclipse
Penumbral eclipse
The Moon barely clipped the northern penumbral shadow of the Earth.
DateAugust 18, 2016
Gamma1.559
Magnitude−0.9925
Saros cycle109 (72 of 72)
Penumbral33 minutes, 36 seconds
Contacts (UTC)
P19:25:36
Greatest9:42:24
P49:59:12

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]

  1. ^ "August 18, 2016 Almost Lunar Eclipse". timeanddate. Retrieved 16 November 2024.
  2. ^ "Moon Distances for London, United Kingdom, England". timeanddate. Retrieved 16 November 2024.
  3. ^ Cite error: The named reference HMNAO was invoked but never defined (see the help page).
  4. ^ Cite error: The named reference NEWS was invoked but never defined (see the help page).
  5. ^ Espenak 1989, p. 150.
  6. ^ Espenak & Meeus 2009, p. 11.

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