November 2041 lunar eclipse

A partial lunar eclipse will take place on November 8, 2041.[3]

November 2041 lunar eclipse
Partial eclipse
Date8 November 2041
Gamma0.9212
Magnitude0.1696[1]
Saros cycle146 (12 of 72[2])
Partiality90 minutes 21 seconds
Penumbral268 minutes 0 seconds

More Detalis

Date: Friday 8 November 2041

Penumbral Magnitude: 1.16567

Umbral Magnitude: 0.16963

Gamma: 0.91124

Saros Series: 146th (12 of 72)

Delta T: 1 minute, 20.2 seconds

Greatest Eclipse: 08 Nov 2041 04:33:44.1 UTC (04:35:04.2 TD)

Ecliptic Opposition: 08 Nov 2041 04:43:22.0 UTC (04:44:42.2 TD)

Equatorial Opposition: 08 Nov 2041 05:14:06.0 UTC (05:15:26.2 TD)

Sun right ascension: 14.91

Sun declination: -16.7

Sun diameter: 1937.0 arcseconds

Moon right ascension: 2.89

Moon declination: 17.5

Moon diameter: 1944.8 arcseconds

Earth's shadow right ascension: 2.91

Earth's shadow declination: 16.7

Visibility

Lunar year series (354 days)

Lunar eclipse series sets from 2038-2042
Descending node   Ascending node
Saros Date
Viewing
Type
Chart
Saros Date
Viewing
Type
Chart
111 2038 Jun 17
Penumbral
116 2038 Dec 11
Penumbral
121 2039 Jun 06
Partial
126 2039 Nov 30
Partial
131 2040 May 26
Total
136 2040 Nov 18
Total
141 2041 May 16
Partial
146 2041 Nov 08
Partial
Last set 2038 Jul 16 Last set 2038 Jan 21
Next set 2042 Apr 05 Next set 2042 Sep 29

Metonic series

This eclipse is the second of four Metonic cycle lunar eclipses on the same date, May 15–16, each separated by 19 years.

The Metonic cycle repeats nearly exactly every 19 years and represents a Saros cycle plus one lunar year. Because it occurs on the same calendar date, the earth's shadow will be in nearly the same location relative to the background stars.

  1. 1984 May 15.19 - penumbral (111)
  2. 2003 May 16.15 - total (121)
  3. 2022 May 16.17 - total (131)
  4. 2041 May 16.03 - penumbral (141)
  1. 1984 Nov 08.75 - penumbral (116)
  2. 2003 Nov 09.05 - total (126)
  3. 2022 Nov 08.46 - total (136)
  4. 2041 Nov 08.19 - partial (146)
  5. 2060 Nov 08.17 - penumbral (156)

See also

Notes

  1. For a partial or total lunar eclipse, this value denotes the umbral magnitude. For a penumbral lunar eclipse, this denotes the penumbral magnitude.
  2. Lunar Saros 146 - Fred Espenak and Jean Meeus (NASA's GSFC)
  3. Hermit Eclipse: Saros cycle 146


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