A partial lunar eclipse took place on Saturday, April 15, 1995, the first of two lunar eclipses in 1995, the second being with a penumbral lunar eclipse on Sunday, October 8.
It was completely visible over eastern Asia, Australia, Pacific and western North America, seen rising over eastern Asia, and setting over western North America.
This is the first of four lunar year eclipses at the ascending node of the Moon's orbit.
Lunar eclipse series sets from 1995–1998 | ||||||||
---|---|---|---|---|---|---|---|---|
Ascending node | Descending node | |||||||
Saros Photo | Date Viewing | Type Chart | Gamma | Saros Photo | Date Viewing | Type Chart | Gamma | |
112 | 1995 Apr 15 | Partial | −0.95939 | 117 | 1995 Oct 08 | Penumbral | 1.11794 | |
122 | 1996 Apr 04 | Total | −0.25339 | 127 | 1996 Sep 27 | Total | 0.34264 | |
132 | 1997 Mar 24 | Partial | 0.48990 | 137 | 1997 Sep 16 | Total | −0.37684 | |
142 | 1998 Mar 13 | Penumbral | 1.19644 | 147 | 1998 Sep 06 | Penumbral | −1.10579 | |
Last set | 1994 May 25 | Last set | 1994 Nov 18 | |||||
Next set | 1999 Jan 31 | Next set | 1998 Aug 08 |
Lunar Saros series 112, repeating every 18 years and 11 days, has a total of 72 lunar eclipse events including 15 total lunar eclipses.
Greatest | First | |||
---|---|---|---|---|
The greatest eclipse of the series occurred on 1490 Jun 02, lasting 100 minutes. [1] | Penumbral | Partial | Total | Central |
859 May 20 | 985 Aug 03 | 1364 Mar 18 | 1436 Apr 30 | |
Last | ||||
Central | Total | Partial | Penumbral | |
1562 Jul 16 | 1616 Aug 27 | 2013 Apr 25 | 2139 Jul 12 |
There are 11 series events between 1901 and 2100, grouped into threes (called an exeligmos), each column with approximately the same viewing longitude on earth.
1905 Feb 19 | 1923 Mar 3 | 1941 Mar 13 | |||
1959 Mar 24 | 1977 Apr 04 | 1995 Apr 15 | |||
2013 Apr 25 | 2031 May 07 | 2049 May 17 | |||
2067 May 28 | 2085 Jun 08 | ||||
A lunar eclipse will be preceded and followed by solar eclipses by 9 years and 5.5 days (a half saros). [2] This lunar eclipse is related to two partial solar eclipses of Solar Saros 119.
April 9, 1986 | April 19, 2004 |
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A total lunar eclipse took place on May 4, 2004, the first of two total lunar eclipses in 2004, the second being on October 28, 2004.
A penumbral lunar eclipse took place on 14 March 2006, the first of two lunar eclipses in 2006.
A penumbral lunar eclipse took place on 6 August 2009, the third of four lunar eclipses in 2009. The moon's small entry into the Earth's penumbral shadow produced an extremely subtle dimming of the moon's southern edge, difficult to observe visually.
A penumbral lunar eclipse took place on May 26, 2002, the first of three lunar eclipses in 2002.
A partial lunar eclipse took place on 4 June 2012. It was the first of two lunar eclipses occurring in 2012, the second eclipse set to happen on 28 November. The moon was about 37% covered by the Earth's northern umbral shadow at maximum eclipse.
A partial lunar eclipse took place on 25 April 2013, the first of three lunar eclipses in 2013. Only a tiny sliver (1.48%) of the Moon was covered by the Earth's umbral shadow at maximum eclipse, but the entire northern half of the Moon was darkened from being inside the penumbral shadow. This was one of the shortest partial eclipses of the Moon for the 21st century, lasting 27 minutes. This was the last of 58 umbral lunar eclipses of Lunar Saros 112.
A total lunar eclipse will take place on July 7, 2047. It will last 1 hour 40 minutes and 49 seconds and 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 39 minutes in total.
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 partial lunar eclipse took place on Saturday, December 21, 1991, the last of four lunar eclipses in 1991. The moon grazed the northern edge of the umbral shadow. It occurred near perigee, and as described, such event was known as a supermoon.
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 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 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.
A partial lunar eclipse took place on Monday, April 4, 1977, the first of two lunar eclipses in 1977. At maximum eclipse, a small bite out of the Moon should have been visible. The eclipse lasted for 1 hour and 34.76 minutes, with just 19.289% of the Moon in shadow at maximum.
A total lunar eclipse took place on Saturday, April 13, 1968, the first of two total eclipses in 1968, the second being on October 6, 1968.
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.
A penumbral lunar eclipse took place on Saturday, November 6, 1976, the second of two lunar eclipses in 1976, the first being on May 13. This subtle penumbral eclipse may have been visible to a skilled observer at maximum eclipse. 83.827% 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, 25 minutes and 52.1 seconds. Occurring only 0.3 days after apogee, the moon's apparent diameter was 6.5% smaller than average.
A total lunar eclipse took place on Wednesday, October 18, 1967, the second of two total lunar eclipses in 1967, the first being on April 24, 1967.
A penumbral lunar eclipse will take place on May 17, 2049.
Saros cycle series 112 for lunar eclipses occurs at the moon's ascending node, 18 years 11 and 1/3 days. It contains 72 events, with 15 total eclipses, starting in 1364 and ending in 1616. Solar Saros 119 interleaves with this lunar Saros with an event occurring every 9 years 5 days alternating between each saros series.