A penumbral lunar eclipse took place on Friday, November 18, 1994, the second of two lunar eclipses in 1994, the first was a partial lunar eclipse on Wednesday, May 25.
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This event followed the total solar eclipse of November 3, 1994.
A penumbral lunar eclipse took place on Friday, November 18, 1994, the second of two lunar eclipses in 1994, the first was a partial lunar eclipse on Wednesday, May 25.
This event followed the total solar eclipse of November 3, 1994.
| Lunar eclipse series sets from 1991–1994 | ||||||||
|---|---|---|---|---|---|---|---|---|
| Ascending node | Descending node | |||||||
| Saros | Date Viewing | Type Chart | Gamma | Saros | Date Viewing | Type Chart | Gamma | |
| 110 | 1991 Jun 27  | Penumbral | −1.40641 | 115 | 1991 Dec 21  | Partial | 0.97094 | |
| 120 | 1992 Jun 15  | Partial | −0.62887 | 125 | 1992 Dec 9  | Total | 0.31438 | |
| 130 | 1993 Jun 4  | Total | 0.16376 | 135 | 1993 Nov 29  | Total | −0.39941 | |
| 140 | 1994 May 25  | Partial | 0.89334 | 145 | 1994 Nov 18  | Penumbral | −1.10479 | |
| Last set | 1991 Jul 26 | Last set | 1991 Jan 30 | |||||
| Next set | 1995 Apr 15 | Next set | 1995 Oct 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 total solar eclipses of Solar Saros 152.
| November 12, 1985 | November 23, 2003 |
|---|---|
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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.
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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.
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A penumbral lunar eclipse took place on Wednesday, April 2, 1969, the first of three penumbral lunar eclipses in 1969, the second being on Wednesday, August 27, and the last being on Thursday, September 25. This subtle penumbral eclipse may have been visible to a skilled observer at maximum eclipse. 70.337% 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, 43 minutes and 46.9 seconds. Occurring only 4.2 days before perigee, the Moon's apparent diameter was 0.9% larger than average.
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