| Partial eclipse | |||||||||||||
| Date | 18 September 2024 | ||||||||||||
|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
| Gamma | −0.97920 | ||||||||||||
| Magnitude | 0.08491 | ||||||||||||
| Saros cycle | 118 (52 of 73) | ||||||||||||
| Partiality | 62 minutes, 49 seconds | ||||||||||||
| Penumbral | 246 minutes, 22 seconds | ||||||||||||
| |||||||||||||
A partial lunar eclipse will take place on Wednesday, 18 September 2024, the second of two lunar eclipses in 2024 and the final partial lunar eclipse of Lunar Saros 118.
It will be completely visible over western parts of Africa and Europe, South and eastern North America, all of South America and parts of Antarctica, will be seen rising over the rest of North America, and setting over the rest of Africa, Europe and the Middle East.
  |
 Visibility map |
| Lunar eclipse series sets from 2024–2027 | ||||||||
|---|---|---|---|---|---|---|---|---|
| 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 | |||||
It is the last partial lunar eclipse of Saros cycle 118.
A lunar eclipse will be preceded and followed by solar eclipses by 9 years and 5.5 days (a half saros). [1] This lunar eclipse is related to two partial solar eclipses of Solar Saros 125.
| 13 September 2015 | 23 September 2033 |
|---|---|
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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 penumbral lunar eclipse took place on 14 March 2006, the first of two lunar eclipses in 2006.
A total lunar eclipse took place at 0308 UT (GMT) on Thursday, August 17, 1989, the second of two total lunar eclipses in 1989.
A total lunar eclipse will take place on August 7, 2036. The southern tip of the Moon will pass through the center of the Earth's shadow. This is the last central lunar eclipse of Saros cycle 129.
A total lunar eclipse took place on Thursday, April 4, 1996, the first of two total lunar eclipses in 1996, the other being on Friday, September 27. The Moon passed through the center of the Earth's shadow.
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 total lunar eclipse took place on Thursday, April 24, 1986, the first of two total lunar eclipses in 1986, the second being on October 17, 1986. The Moon was plunged into darkness for 1 hour, 3 minutes and 34.8 seconds, in a deep total eclipse which saw the Moon 20.217% 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, 18 minutes and 46.8 seconds in total. The Moon was just 1.2 days before perigee, making it 5.3% larger than average.
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 total lunar eclipse took place on Friday, November 29, 1974, the second of two lunar eclipses in 1974. The Moon was plunged into darkness for 1 hour, 15 minutes and 45 seconds, in a deep total eclipse which saw the Moon 28.961% 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, 28 minutes and 58.7 seconds in total. The penumbral eclipse lasted for 5 hours, 33 minutes and 11.6 seconds. The partial eclipse lasted for 3 hours, 28 minutes and 58.7 seconds. The total eclipse lasted for 1 hour, 15 minutes and 45 seconds. Occurring only 3.6 days before perigee, the Moon's apparent diameter was 1.4% larger than average.
A partial lunar eclipse occurred on Saturday, 28 October 2023 (UTC).
A penumbral lunar eclipse took place on Monday, March 25, 2024. It was visible to the naked eye as 95.57% of the Moon was immersed in Earth's penumbral shadow, making it the deepest penumbral eclipse overall since May 5, 2023, and the deepest for North and South America since February 11, 2017.
A total lunar eclipse will take place on Friday, March 14, 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 perigee. Occurring only 3.4 days before apogee, the Moon's apparent diameter will be 5.4% smaller than average.
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 partial lunar eclipse will take place on Wednesday, January 12, 2028.
A partial lunar eclipse will take place on Thursday, July 6, 2028.
A total lunar eclipse took place on Saturday, September 16, 1978, the second of two total lunar eclipses in 1978. The Moon was plunged into darkness for 1 hour, 18 minutes and 39 seconds, in a deep total eclipse which saw the Moon 32.683% 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, 27 minutes and 11.6 seconds in total.
A penumbral lunar eclipse took place on Wednesday, May 4, 1966, the first of two penumbral lunar eclipses in 1966. It was visible from South America, Europe, Africa, Asia, Australia and Antarctica.
A partial lunar eclipse took place on Saturday, July 6, 1963 with an umbral eclipse magnitude of 0.70602. The Moon was strikingly shadowed in this deep partial eclipse which lasted 3 hours exactly, with 71% of the Moon in darkness at maximum. 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. It was the second of three lunar eclipses in 1963, the first was a penumbral lunar eclipse on January 9, 1963 and the third and last was on December 30, 1963.
A partial lunar eclipse took place on Tuesday, August 5, 1952. The Earth's shadow on the Moon was clearly visible in this eclipse, with 53.2% of the Moon in shadow; the partial eclipse lasted for 2 hours and 27 minutes. The Moon's apparent diameter was larger and Supermoon because the eclipse occurred only 45 minutes before perigee.
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