Visibility
| Total eclipse | |||||||||||||||||
| Date | 28 October 1985 | ||||||||||||||||
|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
| Gamma | 0.35197 | ||||||||||||||||
| Magnitude | 1.23687 | ||||||||||||||||
| Saros cycle | 126 (44 of 72) | ||||||||||||||||
| Totality | 43 minutes, 52.2 seconds | ||||||||||||||||
| Partiality | 214 minutes, 58.1 seconds | ||||||||||||||||
| Penumbral | 365 minutes, 8.9 seconds | ||||||||||||||||
| |||||||||||||||||
A total lunar eclipse took place on Monday, October 28, 1985, the second of two total lunar eclipses in 1985, the first being on May 4, 1985. [1]
| Lunar eclipse series sets from 1984–1987 | ||||||||
|---|---|---|---|---|---|---|---|---|
| Descending node | Ascending node | |||||||
| Saros | Date Viewing | Type Chart | Gamma | Saros | Date Viewing | Type Chart | Gamma | |
| 111 | 1984 May 15  | Penumbral | 1.11308 | 116 | 1984 Nov 08  | Penumbral | −1.08998 | |
| 121 | 1985 May 04  | Total | 0.35197 | 126 | 1985 Oct 28  | Total | −0.40218 | |
| 131 | 1986 Apr 24  | Total | −0.36826 | 136 | 1986 Oct 17  | Total | 0.31887 | |
| 141 | 1987 Apr 14  | Penumbral | −1.13641 | 146 | 1987 Oct 07  | Penumbral | 1.01890 | |
| Last set | 1984 Jun 13 | Last set | 1983 Dec 20 | |||||
| Next set | 1988 Mar 03 | Next set | 1988 Aug 27 | |||||
It is part of saros series 126 .
Lunar saros series 126, repeating every 18 years and 11 days, has a total of 70 lunar eclipse events including 14 total lunar eclipses. Solar Saros 133 interleaves with this lunar saros with an event occurring every 9 years 5 days alternating between each saros series.
First penumbral lunar eclipse: 18 July 1228
First partial lunar eclipse: 24 March 1625
First total lunar eclipse: 19 June 1769
First central lunar eclipse: 11 July 1805
Greatest eclipse of the lunar saros 126: 13 August 1859, lasting 106 minutes.
Last central lunar eclipse: 26 September 1931
Last total lunar eclipse: 9 November 2003
Last partial lunar eclipse: 5 June 2346
Last penumbral lunar eclipse: 19 August 2472
1901-2100
This eclipse is the second of four Metonic cycle lunar eclipses on the same date, October 28–29, each separated by 19 years:
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.
| Metonic events: May 4 and October 28 | |
|---|---|
| Descending node | Ascending node |
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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). [2] This lunar eclipse is related to two total solar eclipses of Solar Saros 133.
| October 23, 1976 | November 3, 1994 |
|---|---|
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A penumbral lunar eclipse took place on Thursday, November 8, 1984, the last of three lunar eclipses in 1984. This subtle penumbral eclipse may have been visible to a skilled observer at maximum eclipse. 90% 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 and 28 minutes.
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.
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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.
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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 total lunar eclipse took place on Monday, September 15, 1913. The moon passed through the center of the Earth's shadow.
A total lunar eclipse will take place on March 13, 2044.
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A total lunar eclipse took place on Friday, October 7, 1949, the second of two lunar eclipses in 1949.
A total lunar eclipse took place on Saturday, September 26, 1931. The Moon passed through the central of the Earth's shadow. This was the last central lunar eclipse of Saros cycle 126.
A total lunar eclipse will occur on Wednesday, June 9, 2123, with maximum eclipse at 05:06 UTC. A dramatic total eclipse lasting 106 minutes and 6 seconds 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 56 minutes in total. The penumbral eclipse lasts for 6 hours and 14 minutes. Maximum eclipse is at 05:06:28 UT. This will be the longest Total Lunar Eclipse since 16 July 2000, and the longest one until 12 May 2264 and 27 July 3107, though the eclipse on June 19, 2141 will be nearly identical in all aspects. This will also be the longest of the 22nd century and the second longest of the 3rd millennium. The eclipse on June 19, 2141 will be the second longest of the 22nd century and the third longest of the third millennium.
A penumbral lunar eclipse will occur on November 8, 2060. It will be too small to be visually perceptible.
