| Penumbral Lunar Eclipse February 22, 2035 | |
|---|---|
 The moon will perceptibly dim as the moon passes through the Earth's northern penumbral shadow | |
| Series | 114 (60 of 71) |
| Gamma | -1.0357 |
| Magnitude | 0.9652 |
| Duration (hr:mn:sc) | |
| Penumbral | 4:15:42 |
| Contacts UTC | |
| P1 | 6:58:21 |
| Greatest | 9:06:12 |
| P4 | 11:14:03 |
A penumbral lunar eclipse will take place on February 22, 2035. It will be visible to the naked eye as 96.52% of the Moon will be immersed in Earth's penumbral shadow. [1]
It will be visible before sunrise east of North America though the Moon will have set below the horizon east of South America while it'll still be visible from the rest of South America.
 Visibility map |
| Ascending node | Descending node | |||||
|---|---|---|---|---|---|---|
| Saros | Date Viewing | Type Chart | Saros | Date Viewing | Type Chart | |
| 114 | 2035 Feb 22  | Penumbral | 119 | 2035 Aug 19  | Partial | |
| 124 | 2036 Feb 11  | Total | 129 | 2036 Aug 07  | Total | |
| 134 | 2037 Jan 31  | Total | 139 | 2037 Jul 27  | Partial | |
| 144 | 2038 Jan 21  | Penumbral | 149 | 2038 Jul 16  | Penumbral | |
| Last set | 2034 Apr 03 | Last set | 2034 Sep 28 | |||
| Next set | 2038 Jun 17 | Next set | 2038 Dec 11 | |||
Lunar Saros series 114, repeating every 18 years and 11 days, has a total of 71 lunar eclipse events including 13 total lunar eclipses.
First Penumbral Lunar Eclipse: 0971 May 13
First Partial Lunar Eclipse: 1115 Aug 07
First Total Lunar Eclipse: 1458 Feb 28
First Central Lunar Eclipse: 1530 Apr 12
Greatest Eclipse of Lunar Saros 114: 1584 May 24
Last Central Lunar Eclipse: 1638 Jun 26
Last Total Lunar Eclipse: 1674 Jul 17
Last Partial Lunar Eclipse: 1890 Nov 26
Last Penumbral Lunar Eclipse: 2233 Jun 22
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A penumbral lunar eclipse took place on Tuesday, April 14, 1987, the first of two lunar eclipses in 1987, the second being on October 7, 1987. This subtle penumbral eclipse may have been visible to a skilled observer at maximum eclipse. 77.703% 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 3 hours, 54 minutes and 12.8 seconds. The Moon was just 4.6 days before perigee, making it 0.5% larger than average.
A penumbral lunar eclipse took place on Tuesday, December 20, 1983, the second of two lunar eclipses in 1983. At the maximum eclipse, 89% of the Moon's disk 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 2 minutes overall.
A penumbral lunar eclipse took place on Tuesday, January 20, 1981, the first of two lunar eclipses in 1981. 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 and 24 minutes in all, though for most of it, the eclipse was extremely difficult or impossible to see. The moon's apparent diameter was larger because the eclipse occurred 5.2 days after perigee.
A partial lunar eclipse occurred on 19 November 2021. The eclipse occurred towards a micromoon. This was the longest partial lunar eclipse since 18 February 1440, and the longest until 8 February, 2669; however, many eclipses, including the November 2022 lunar eclipse, have a longer period of umbral contact at next to 3 hours 40 minutes. It was often referred to as a "Beaver Blood Moon" although not technically fulfilling the criteria for a true blood moon (totality).
A penumbral lunar eclipse will take place on Monday, March 25, 2024. It will be visible to the naked eye as 95.57% of the Moon will be immersed in Earth's penumbral shadow.
A penumbral lunar eclipse took place on Saturday, March 1, 1980, the first of three penumbral lunar eclipses in 1980. This subtle penumbral eclipse may have been visible to a skilled observer at maximum eclipse. 65.455% 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 3 hours, 58 minutes and 33.3 seconds.
A penumbral lunar eclipse will take place on January 21, 2038. It will be visible to the naked eye as 89.96% of the Moon will be immersed in Earth's penumbral shadow. It is the first of 4 penumbral lunar eclipses in 2038, with the next eclipse on 17 June.
A partial lunar eclipse took place on Thursday, May 13, 1976, the first of two lunar eclipses in 1976, the second being a penumbral lunar eclipse on November 6, 1976. At maximum eclipse, a small bite out of the Moon should have been visible. The eclipse lasted for 1 hour, 15 minutes and 23.8 seconds, with just 12.17% of the Moon in shadow at maximum. Occurring only 1.1 days after perigee, the Moon's apparent diameter 5.4% larger than average.
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A penumbral lunar eclipse took place on Wednesday, December 8, 1965. At maximum eclipse, 88% 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 1 minute overall.
A penumbral lunar eclipse took place on Wednesday, January 9, 1963, the first of three lunar eclipses in 1963.
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