A penumbral lunar eclipse took place on Sunday, September 6, 1998, the last of three lunar eclipses in 1998.
A penumbral lunar eclipse took place on Sunday, September 6, 1998, the last of three lunar eclipses in 1998.
This is the last of four lunar year eclipses at the descending 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 | |||||
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 154.
| August 31, 1989 | September 11, 2007 |
|---|---|
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A penumbral lunar eclipse took place on April 24, 2005, the first of two lunar eclipses in 2005. At maximum eclipse, 86.5% 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 6 minutes overall, and was visible from east Asia, Australia, and the Americas.
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 Sunday, January 31, 1999, the first of two lunar eclipses in 1999.
A penumbral lunar eclipse took place on Friday, March 13, 1998, the first of three lunar eclipses in 1998.
A penumbral lunar eclipse took place on 16 September 2016, the last of three lunar eclipses in 2016.
A penumbral lunar eclipse took place at the Moon's ascending node on 11 February 2017, the first of two lunar eclipses in 2017. It was not quite a total penumbral lunar eclipse. It occurred the same day as comet 45P/Honda–Mrkos–Pajdušáková made a close approach to Earth. It also occurred on the Lantern Festival, the first since 9 February 2009. Occurring only 4.4 days after perigee, the moon's apparent diameter was larger.
A partial lunar eclipse took place on Monday, August 6, 1990, the second of two lunar eclipses in 1990.
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 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 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, May 15, 1984, the first of three lunar eclipses in 1984. This was a deep penumbral eclipse, with the southern limb of the Moon close to the Earth's shadow.
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 penumbral lunar eclipse took place on Sunday, July 27, 1980, the second of three penumbral lunar eclipses in 1980. This very subtle penumbral eclipse was essentially invisible to the naked eye; though it lasted 2 hours, 17 minutes and 36.3 seconds, just 25.354% of the Moon's disc was in partial shadow. The moon passed in the northern edge of the Earth's penumbral shadow, and was the 70th lunar eclipse of Saros cycle 109.
A penumbral lunar eclipse will take place on 20–21 February 2027.
A penumbral lunar eclipse will take place on Tuesday, August 17, 2027. It will cause a subtle dimming as 54.56% of the Moon will cross within Earth's penumbral shadow.
A penumbral lunar eclipse will take place on 18 July 2027. The Moon will barely clip the edge of the Earth's penumbral shadow, and the eclipse will be impossible to see in practice. The event is listed as a miss by some sources.
A penumbral lunar eclipse took place at the Moon's descending node of the orbit on Tuesday, August 26, 1980, the last of three penumbral lunar eclipses in 1980 with a penumbral magnitude of 0.70891. This subtle penumbral eclipse may have been visible to a skilled observer at maximum eclipse. 70.891% 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, 34 minutes and 26 seconds.
A partial lunar eclipse will take place on November 30, 2039. At 3 hours 26 minutes, it is the longest partial lunar eclipse since November 19, 2021, which is the previous member of Lunar Saros 126.
A penumbral lunar eclipse took place on Thursday, September 25, 1969, the last of three penumbral lunar eclipses in 1969, the first being on Wednesday, April 2, and the second being on Wednesday, August 27. At maximum eclipse, 90% 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 5 minutes overall.
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