| Partial Lunar Eclipse July 27, 2037 | |
|---|---|
 The moon passes west to east (right to left) across the Earth's umbral shadow, shown in hourly intervals. | |
| Series | 139 (23 of 81) |
| Gamma | -0.5582 |
| Magnitude | 0.8095 |
| Duration (hr:mn:sc) | |
| Partial | 3:12:25 |
| Penumbral | 5:40:49 |
| Contacts UTC | |
| P1 | 1:19:29 |
| U1 | 2:33:41 |
| Greatest | 4:09:53 |
| U4 | 5:46:05 |
| P4 | 7:00:17 |
A partial lunar eclipse will take place on July 27, 2037. [1]
| 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 139, repeating every 18 years and 11 days, has a total of 79 lunar eclipse events including 42 umbral lunar eclipses (15 partial lunar eclipses and 27 total lunar eclipses)..
| Greatest | First | |||
|---|---|---|---|---|
The greatest eclipse of the series will occur on 2199 Nov 02, lasting 102 minutes. [2] | Penumbral | Partial | Total | Central |
| 1658 Dec 09 | 1947 Jun 03 | 2073 Aug 17 | 2109 Sep 09 | |
| Last | ||||
| Central | Total | Partial | Penumbral | |
| 2488 Apr 26 | 2542 May 30 | 2686 Aug 25 | 3065 Apr 13 | |
| 1911 May 13 | 1929 May 23 | 1947 Jun 03 | |||
 |  |  |  |  |  |
| 1965 Jun 14 | 1983 Jun 25 | 2001 Jul 05 | |||
 |  |  |  |  |  |
| 2019 Jul 16 | 2037 Jul 27 | 2055 Aug 07 | |||
 |  | | |  |  |
| 2073 Aug 17 | 2091 Aug 29 | ||||
 | This lunar eclipse-related article is a stub. You can help Wikipedia by expanding it. |
A total lunar eclipse occurred from 5:27 to 11:06 UTC on 21 December 2010, coinciding with the date of the Winter solstice in the Northern Hemisphere and Summer solstice in the Southern Hemisphere. It was visible in its entirety as a total lunar eclipse in North and South America, Iceland, Ireland, Britain and northern Scandinavia.
A total lunar eclipse took place on Tuesday 4 May 2004, the first of two total lunar eclipses in 2004, the second being on 28 October 2004.
A partial lunar eclipse took place on Thursday 5 July 2001, the second of three lunar eclipses in 2001. The Earth's shadow on the moon was clearly visible in this eclipse, with 49.614% of the Moon in shadow; the partial eclipse lasted for 2 hours, 40 minutes and 0.5 seconds. Occurring only 3.9 days before apogee, the Moon’s apparent diameter was 5.021% smaller than average.
A partial lunar eclipse took place on Wednesday, July 28, 1999, the second of two lunar eclipses in 1999.
A partial lunar eclipse took place on Saturday, June 25, 1983, the first of two lunar eclipses in 1983 with an umbral eclipse magnitude of 0.33479. A partial lunar eclipse happens when the Earth moves between the Sun and the Full Moon, but they are not precisely aligned. Only part of the Moon's visible surface moves into the dark part of the Earth's shadow. A partial lunar eclipse occurs when the Earth moves between the Sun and Moon but the three celestial bodies do not form a straight line in space. When that happens, a small part of the Moon's surface is covered by the darkest, central part of the Earth's shadow, called the umbra. The rest of the Moon is covered by the outer part of the Earth's shadow called the penumbra. The Earth's shadow on the moon was clearly visible in this eclipse, with 33% of the Moon in shadow; the partial eclipse lasted for 2 hours and 15 minutes.
A partial lunar eclipse took place on Friday, July 17, 1981, the second of two lunar eclipses in 1981. The Earth's shadow on the Moon was clearly visible in this eclipse, with 55% of the Moon in shadow; the partial eclipse lasted for 2 hours and 43 minutes.
A partial lunar eclipse took place on Monday, June 15, 1992, the first of two lunar eclipses in 1992, the second being with a total lunar eclipse on Wednesday, December 9.
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 Friday, July 26, 1991, the third of four lunar eclipses in 1991. This was the 2nd member of Lunar Saros 148. The previous event was on 15 July 1973, and the 1st eclipse of the series. The next event was on 6 August 2009.
A penumbral lunar eclipse took place on Wednesday, January 30, 1991, the first of four lunar eclipses in 1991.
A partial lunar eclipse occurred on the 16 and 17 July 2019. The Moon was covered 65.31% by the Earth's umbral shadow at maximum eclipse.
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 partial lunar eclipse will take place on Saturday, June 15, 2030.
A penumbral lunar eclipse will take place on May 7, 2031.
A partial lunar eclipse took place on Monday, June 14, 1965. At maximum eclipse, a small bite out of the Moon should have been visible. The eclipse lasted for 1 hour and 40 minutes, with just 18% of the Moon in shadow at maximum.
A total lunar eclipse will take place on September 7, 2044. It will be the first total eclipse in Lunar Saros 138.
A total solar eclipse occurred at the ascending node of the Moon's orbit on Tuesday, July 2, 2019, with an eclipse magnitude of 1.0459. Totality was visible from the southern Pacific Ocean east of New Zealand to the Coquimbo Region in Chile and Central Argentina at sunset, with the maximum of 4 minutes 33 seconds visible from the Pacific Ocean. The Moon was only 2.4 days before perigee, making it fairly large.
A partial lunar eclipse took place on Tuesday, June 3, 1947. A tiny bite out of the Moon may have been visible at maximum, though just 2.02% of the Moon was shadowed in a partial eclipse which lasted for 34 minutes and 42 seconds. A shading across the moon from the Earth's penumbral shadow should have been visible at maximum eclipse.
A total lunar eclipse will occur on Wednesday, June 9, 2123, with maximum eclipse at 05:06 UTC. A dramatic total eclipse lasting 106 minutes and 6 seconds will plunge the full Moon into deep darkness, as it passes right through the centre of the Earth's umbral shadow. While the visual effect of a total eclipse is variable, the Moon may be stained a deep orange or red colour at maximum eclipse. This will be a great spectacle for everyone who sees it. The partial eclipse will last for 3 hours and 56 minutes in total. The penumbral eclipse lasts for 6 hours and 14 minutes. Maximum eclipse is at 05:06:28 UT. This will be the longest Total Lunar Eclipse since 16 July 2000, and the longest one until 12 May 2264 and 27 July 3107, though the eclipse on June 19, 2141 will be nearly identical in all aspects. This will also be the longest of the 22nd century and the second longest of the 3rd millennium. The eclipse on June 19, 2141 will be the second longest of the 22nd century and the third longest of the third millennium.
A partial lunar eclipse will take place on August 7, 2055. It will last 3 hours, 23 minutes, and 23 seconds. It will be the last of the first set of partial eclipses in Lunar Saros 139.
