Visibility
| Partial eclipse | |||||||||||||
| Date | 16 May 2041 | ||||||||||||
|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
| Gamma | −0.9746 | ||||||||||||
| Magnitude | 0.0645 [1] | ||||||||||||
| Saros cycle | 141 (25 of 72) | ||||||||||||
| Partiality | 58 minutes 27 seconds | ||||||||||||
| Penumbral | 269 minutes 44 seconds | ||||||||||||
| |||||||||||||
A partial lunar eclipse will take place on May 16, 2041. [2]
This is the 25th member of Lunar Saros 141. The previous event was the May 2023 lunar eclipse.
| 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 | |
| 156 | 2042 Oct 28  | Penumbral | ||||
| Last set | 2038 Jul 16 | Last set | 2038 Jan 21 | |||
| Next set | 2042 Apr 05 | Next set | 2042 Sep 29 | |||
This eclipse is the fourth and final 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.
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A penumbral lunar eclipse took place on Sunday 24 April 2005, the first of two lunar eclipses in 2005. At maximum eclipse, 86.5% of the Moon's disc was partially shaded by the Earth, which caused a slight shadow gradient across its disc; this subtle effect may have been visible to careful observers. No part of the Moon was in complete shadow. The eclipse lasted 4 hours and 6 minutes overall, and was visible from east Asia, Australia, and the Americas.
A partial lunar eclipse took place on Monday 17 October 2005, the second of two lunar eclipses in 2005. A tiny bite out of the Moon may have been visible at maximum, though just 6.25% of the Moon was shadowed in a partial eclipse which lasted for nearly 56 minutes and was visible over east Asia, Australasia, and most of the North America. A shading across the Moon from the Earth's penumbral shadow should have been visible at maximum eclipse.
A total lunar eclipse took place on Monday, October 28, 1985, the second of two total lunar eclipses in 1985, the first being on May 4, 1985.
A penumbral lunar eclipse took place on Thursday, March 3, 1988, the first of two lunar eclipses in 1988, the second being on August 27, 1988. Earlier sources compute this as a 0.3% partial eclipse lasting under 14 minutes, and newest calculations list it as a penumbral eclipse that never enters the umbral shadow. In a rare total penumbral eclipse, the entire Moon was partially shaded by the Earth, and the shading across the Moon should have been quite visible at maximum eclipse. The penumbral phase lasted for 4 hours, 53 minutes and 50.6 seconds in all, though for most of it, the eclipse was extremely difficult or impossible to see. The Moon was 2.2 days after apogee, making it 6.1% smaller than average.
A penumbral lunar eclipse took place on Thursday, June 27, 1991, the second of four lunar eclipses in 1991. The moon entered the Earth's penumbra for about 3 hours, and was difficult to see. This lunar eclipse is the predecessor of the Solar eclipse of July 11, 1991.
A penumbral lunar eclipse took place on Thursday, November 8, 1984, the last of three lunar eclipses in 1984. This subtle penumbral eclipse may have been visible to a skilled observer at maximum eclipse. 90% of the Moon's disc was partially shaded by the Earth, which caused a gentle shadow gradient across its disc at maximum; the eclipse as a whole lasted 4 hours and 28 minutes.
A penumbral lunar eclipse took place on Tuesday, May 15, 1984, the first of three lunar eclipses in 1984. This was a deep penumbral eclipse, with the southern limb of the Moon close to the Earth's shadow.
A penumbral lunar eclipse occurred on Friday, 5 May 2023, the first of two lunar eclipses in 2023. The moon's apparent diameter was 0.1% larger than average because it occurred 5.5 days before perigee. This was the deepest penumbral eclipse since February 2017 and until September 2042.
A partial lunar eclipse occurred on Saturday, 28 October 2023 (UTC).
A partial lunar eclipse will take place on Friday 28 August 2026. The moon will be almost be inside the umbra, but not quite be contained within the umbral shadow at greatest eclipse.
A penumbral lunar eclipse will take place on 20–21 February 2027.
A partial lunar eclipse will take place on November 8, 2041.
A partial lunar eclipse took place on Monday, August 17, 1970, the second of two lunar eclipses in 1970, the first was on February 21 of that year. The Earth's shadow on the Moon was clearly visible in this eclipse, with 41% of the Moon in shadow; the partial eclipse lasted for 2 hours and 11 minutes. It was the second of two lunar eclipses in 1970.
A total lunar eclipse took place on Monday, April 24, 1967, the first of two total lunar eclipses in 1967, the second being on October 18, 1967.
A penumbral lunar eclipse took place on Wednesday, February 21, 1951. This was 6.4 days after the Moon reached apogee.
A penumbral lunar eclipse will take place on March 3, 2045.
A total lunar eclipse will take place on September 7, 2044. It will be the first total eclipse in Lunar Saros 138.
A total lunar eclipse will take place on March 13, 2044.
A penumbral lunar eclipse will take place on December 20, 2048.
A total lunar eclipse will take place on May 6, 2050.
