Total eclipse | |||||||||||||||||
Date | 13-14 March 2025 | ||||||||||||||||
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Gamma | 0.34846 | ||||||||||||||||
Magnitude | 1.18038 | ||||||||||||||||
Saros cycle | 123 (53 of 72) | ||||||||||||||||
Totality | 66 minutes, 3.9 seconds | ||||||||||||||||
Partiality | 218 minutes, 55.8 seconds | ||||||||||||||||
Penumbral | 363 minutes, 22.4 seconds | ||||||||||||||||
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A total lunar eclipse will take place on Friday, 14 March 2025, the first of two total lunar eclipses in 2025. The Moon will take place near apogee during this eclipse, making it appear smaller than usual. The second eclipse will take place on 7-8 September 2025, happening near apogee. Occurring only 3.4 days before apogee (apogee on 17 March 2025), the Moon’s apparent diameter will be 5.4% smaller than average. [1] [2]
This lunar eclipse marks the beginning of an almost tetrad, with 3 total lunar eclipses and a deep partial lunar eclipse (greater than 90%), with others being 07 Sep 2025 (T), 03 Mar 2026 (T) and 28 Aug 2026 (P). [3]
It will be completely visible from the Americas, will be seen rising over New Zealand and eastern Asia, and setting over western Europe and western Africa.[ citation needed ]
Lunar eclipse series sets from 2024–2027 | ||||||||
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Descending node | Ascending node | |||||||
Saros | Date | Type Viewing | Gamma | Saros | Date Viewing | Type Chart | Gamma | |
113 | 2024 Mar 25 | Penumbral | 1.06098 | 118 | 2024 Sep 18 | Partial | −0.97920 | |
123 | 2025 Mar 14 | Total | 0.34846 | 128 | 2025 Sep 07 | Total | −0.27521 | |
133 | 2026 Mar 03 | Total | −0.37651 | 138 | 2026 Aug 28 | Partial | 0.49644 | |
143 | 2027 Feb 20 | Penumbral | −1.04803 | 148 | 2027 Aug 17 | Penumbral | 1.27974 | |
Last set | 2023 May 05 | Last set | 2023 Oct 28 | |||||
Next set | 2028 Jan 12 | Next set | 2027 Jul 18 |
Lunar saros series 123, repeating every 18 years and 11 days, has 25 total lunar eclipses. The first total lunar eclipse of this series was on July 16, 1628 , and last will be on April 4, 2061 . The two longest occurrence of this series were on September 20, 1736 and October 1, 1754 when totality lasted 106 minutes.
It last occurred on March 3, 2007 and will next occur on 25 March 2043.
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 in nearly the same location relative to the background stars.
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A lunar eclipse will be preceded and followed by solar eclipses by 9 years and 5.5 days (a half saros). [4] Related to Solar Saros 130.
March 9, 2016 | March 20, 2034 |
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A total lunar eclipse took place on 3 March 2007, the first of two eclipses in 2007. The Moon entered the penumbral shadow at 20:18 UTC, and the umbral shadow at 21:30 UTC. The total phase lasted between 22:44 UTC and 23:58 UTC with a distinctive brick-red shade. The Moon left the umbra shadow at 01:11 UTC and left the penumbra shadow at 02:24 UTC 2007-03-04. The second lunar eclipse of 2007 occurred on 28 August.
A total lunar eclipse occurred on February 20 and February 21, 2008. It was visible in the eastern evening sky on February 20 for all of North and South America, and on February 21 in the predawn western sky from most of Africa and Europe. Greatest Eclipse occurring on Thursday, February 21, 2008, at 03:26:03 UTC, totality lasting 49 minutes and 45.6 seconds.
A total lunar eclipse took place on Sunday 9 November 2003, the second of two total lunar eclipses in 2003, the first being on 16 May 2003. It is the first total lunar eclipse of 21st century which happened on a micromoon day. The Moon barely edged into total eclipse for 21 minutes and 58 seconds. With the Moon just 1.78% of its diameter into the Earth's umbral shadow, the Moon may have been quite bright, but even so, this should have been worth seeing. The partial eclipse lasted for 3 hours, 31 minutes and 25 seconds. Occurring only 1.4 days before apogee, the Moon's apparent diameter was 6.4% smaller than average.
A total lunar eclipse took place on Thursday 28 October 2004, the second of two total lunar eclipses in 2004, the first being on 4 May 2004. It was the first lunar eclipse to take place during a World Series game, which when seen from Busch Memorial Stadium in St, Louis, Missouri, provided a surreal sight on the night the Boston Red Sox won their first World Series in 86 years to end the Curse of the Bambino. Occurring 5.6 days before apogee, the Moon's apparent diameter was smaller. The Moon was 10.1 days after perigee and 5.6 days before apogee.
A total lunar eclipse will take place on Tuesday, March 3, 2026, the first of two lunar eclipses in 2026.
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 total lunar eclipse took place on Friday, September 27, 1996, the second of two lunar eclipses in 1996, the first being on Thursday, April 4. This is the 41st member of Lunar Saros 127. The previous event is the September 1978 lunar eclipse. The next event is the October 2014 lunar eclipse.
A total lunar eclipse occurred on Tuesday, 8 November 2022. The southern limb of the Moon passed through the center of the Earth's shadow. It surpassed the previous eclipse as the longest total lunar eclipse visible from nearly all of North America since 17 August 1989, and until 26 June 2029. Occurring only 5.8 days before apogee, the Moon's apparent diameter was smaller. The next total lunar eclipse will take place on 14 March 2025. A lunar occultation of Uranus happened during the eclipse. It was the first total lunar eclipse on Election Day in US history. This event was referred in media coverage as a "beaver blood moon".
A total lunar eclipse took place on Friday, June 4, 1993, the first of two total lunar eclipses in 1993, the second being on Monday, November 29. The Moon was plunged into darkness for 1 hour and 36 minutes, in a deep total eclipse which saw the Moon 56% of its diameter inside the Earth's umbral shadow. The visual effect of this depends on the state of the Earth's atmosphere, but the Moon may have been stained a deep red colour. The partial eclipse lasted for 3 hours and 38 minutes in total. The moon passed through the center of the Earth's shadow.
A total lunar eclipse took place on Friday, March 24, 1978, the first of two total lunar eclipses in 1978. The moon passed through the center of the Earth's shadow. The Moon was plunged into darkness for 1 hour, 30 minutes and 40.2 seconds, in a deep total eclipse which saw the Moon 45.179% of its diameter inside the Earth's umbral shadow. The visual effect of this depends on the state of the Earth's atmosphere, but the Moon may have been stained a deep red colour. The partial eclipse lasted for 3 hours, 38 minutes and 34.5 seconds in total.
A total lunar eclipse took place at the Moon's descending node of the orbit on Wednesday, February 10, 1971, the first of two total lunar eclipses in 1971. It had an umbral magnitude of 1.30819. The Moon narrowly missed the center of the Earth's shadow due its gamma being >0.2725 at 0.27413. The Moon was plunged into darkness for 1 hour, 22 minutes and 11.4 seconds, in a deep total eclipse which saw the Moon 30.819% of its diameter inside the Earth's umbral shadow. The visual effect of this depends on the state of the Earth's atmosphere, but the Moon may have been stained a deep red colour. The partial eclipse lasted for 3 hours, 44 minutes and 42.9 seconds and in total. Occurring only 2.7 days before apogee, the Moon's apparent diameter was 5.9% smaller than average.
A total lunar eclipse took place on Friday, October 17, 1986, the second of two total lunar eclipses in 1986, the first being on April 24, 1986. The Moon was plunged into darkness for 1 hour, 13 minutes and 41 seconds, in a deep total eclipse which saw the Moon 24.545% of its diameter inside the Earth's umbral shadow. The visual effect of this depends on the state of the Earth's atmosphere, but the Moon may have been stained a deep red colour. The partial eclipse lasted for 3 hours, 36 minutes and 49.5 seconds in total. The Moon was 5.4 days before apogee, making it 3.3% smaller than average.
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 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 total lunar eclipse will take place on 7-8 September 2025. The Moon will barely miss the center of the Earth's shadow. It will be the second of two total lunar eclipses. Occurring roughly 3 days before perigee, the Moon will appear larger than usual.
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 total lunar eclipse took place on Tuesday, November 18, 1975, the second of two total lunar eclipses in 1975. A shallow total eclipse saw the Moon in relative darkness for 40 minutes and 11.1 seconds. The Moon was 6.421% of its diameter into the Earth's umbral shadow, and should have been significantly darkened. The partial eclipse lasted for 3 hours, 29 minutes and 2.1 seconds in total. Occurring only 4.9 days after apogee, the Moon's apparent diameter was 4% smaller than average.
A partial lunar eclipse took place on Tuesday, June 4, 1974, the first of two lunar eclipses in 1974. The Moon was strikingly shadowed in this deep partial eclipse which lasted 3 hours and 14 minutes, with 82.695% of the Moon in darkness at maximum. Occurring 4.5 days before apogee, the Moon's apparent diameter was 4.4% smaller than average.
A partial lunar eclipse took place on Saturday, February 21, 1970. It was the first of two partial lunar eclipses in 1970, the other being on August 17 of the same year. A tiny bite out of the Moon may have been visible at maximum, though just 5% of the Moon was shadowed in a partial eclipse which lasted for 52 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 take place on September 19, 2043.