October 1966 lunar eclipse
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A penumbral lunar eclipse occurred at the Moon’s ascending node of orbit on Saturday, October 29, 1966, with an umbral magnitude of −0.1249. A lunar eclipse occurs when the Moon moves into the Earth's shadow, causing the Moon to be darkened. A penumbral lunar eclipse occurs when part or all of the Moon's near side passes into the Earth's penumbra. Unlike a solar eclipse, which can only be viewed from a relatively small area of the world, a lunar eclipse may be viewed from anywhere on the night side of Earth. Occurring about 4 days after apogee (on October 25, 1966, at 9:55 UTC), the Moon's apparent diameter was smaller.
Visibility
The eclipse was completely visible over northeast Asia, much of North America, and the Pacific Ocean, seen rising over east and southeast Asia and Australia and setting over eastern North America and South America.
Eclipse details
Shown below is a table displaying details about this particular solar eclipse. It describes various parameters pertaining to this eclipse.
| Parameter | Value |
|---|---|
| Penumbral Magnitude | 0.95172 |
| Umbral Magnitude | −0.12488 |
| Gamma | −1.05999 |
| Sun Right Ascension | 14h12m57.7s |
| Sun Declination | -13°22'20.9" |
| Sun Semi-Diameter | 16'06.2" |
| Sun Equatorial Horizontal Parallax | 08.9" |
| Moon Right Ascension | 02h14m38.8s |
| Moon Declination | +12°29'37.7" |
| Moon Semi-Diameter | 14'57.5" |
| Moon Equatorial Horizontal Parallax | 0°54'53.8" |
| ΔT | 37.2 s |
Eclipse season
This eclipse is part of an eclipse season, a period, roughly every six months, when eclipses occur. Only two (or occasionally three) eclipse seasons occur each year, and each season lasts about 35 days and repeats just short of six months (173 days) later; thus two full eclipse seasons always occur each year. Either two or three eclipses happen each eclipse season. In the sequence below, each eclipse is separated by a fortnight.
| October 29 Ascending node (full moon) | November 12 Descending node (new moon) |
|---|---|
| Penumbral lunar eclipse Lunar Saros 116 | Total solar eclipse Solar Saros 142 |
Related eclipses
Eclipses in 1966
- A penumbral lunar eclipse on May 4.
- An annular solar eclipse on May 20.
- A penumbral lunar eclipse on October 29.
- A total solar eclipse on November 12.
Metonic
- Preceded by: Lunar eclipse of January 9, 1963
- Followed by: Lunar eclipse of August 17, 1970
Tzolkinex
- Preceded by: Lunar eclipse of September 17, 1959
- Followed by: Lunar eclipse of December 10, 1973
Half-Saros
- Preceded by: Solar eclipse of October 23, 1957
- Followed by: Solar eclipse of November 3, 1975
Tritos
- Preceded by: Lunar eclipse of November 29, 1955
- Followed by: Lunar eclipse of September 27, 1977
Lunar Saros 116
- Preceded by: Lunar eclipse of October 18, 1948
- Followed by: Lunar eclipse of November 8, 1984
Inex
- Preceded by: Lunar eclipse of November 18, 1937
- Followed by: Lunar eclipse of October 8, 1995
Triad
- Preceded by: Lunar eclipse of December 28, 1879
- Followed by: Lunar eclipse of August 29, 2053
Lunar eclipses of 1966–1969
This eclipse is a member of a semester series. An eclipse in a semester series of lunar eclipses repeats approximately every 177 days and 4 hours (a semester) at alternating nodes of the Moon's orbit.
The penumbral lunar eclipse on August 27, 1969 occurs in the next lunar year eclipse set.
| Lunar eclipse series sets from 1966 to 1969 | |||||||
|---|---|---|---|---|---|---|---|
| Descending node | Ascending node | ||||||
| Saros | Date Viewing | Type Chart | Gamma | Saros | Date Viewing | Type Chart | Gamma |
| 111 | 1966 May 04 | Penumbral | 1.0554 | 116 | 1966 Oct 29 | Penumbral | −1.0600 |
| 121 | 1967 Apr 24 | Total | 0.2972 | 126 | 1967 Oct 18 | Total | −0.3653 |
| 131 | 1968 Apr 13 | Total | −0.4173 | 136 | 1968 Oct 06 | Total | 0.3605 |
| 141 | 1969 Apr 02 | Penumbral | −1.1765 | 146 | 1969 Sep 25 | Penumbral | 1.0656 |
Metonic series
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 |
| 1966 May 4 - Penumbral (111) 1985 May 4 - Total (121) 2004 May 4 - Total (131) 2023 May 5 - Penumbral (141) | 1966 Oct 29 - Penumbral (116) 1985 Oct 28 - Total (126) 2004 Oct 28 - Total (136) 2023 Oct 28 - Partial (146) 2042 Oct 28 - Penumbral (156) |
Saros 116
This eclipse is a part of Saros series 116, repeating every 18 years, 11 days, and containing 73 events. The series started with a penumbral lunar eclipse on March 11, 993 AD. It contains partial eclipses from June 16, 1155 through September 11, 1299; total eclipses from September 21, 1317 through July 11, 1786; and a second set of partial eclipses from July 22, 1804 through October 7, 1930. The series ends at member 73 as a penumbral eclipse on May 14, 2291.
The longest duration of totality was produced by member 40 at 102 minutes, 40 seconds on May 16, 1696. All eclipses in this series occur at the Moon’s ascending node of orbit.
| Greatest | First | |||
|---|---|---|---|---|
| The greatest eclipse of the series occurred on 1696 May 16, lasting 102 minutes, 40 seconds. | Penumbral | Partial | Total | Central |
| 993 Mar 11 | 1155 Jun 16 | 1317 Sep 21 | 1588 Mar 13 | |
| Last | ||||
| Central | Total | Partial | Penumbral | |
| 1750 Jun 19 | 1786 Jul 11 | 1930 Oct 07 | 2291 May 14 |
Eclipses are tabulated in three columns; every third eclipse in the same column is one exeligmos apart, so they all cast shadows over approximately the same parts of the Earth.
| Series members 46–67 occur between 1801 and 2200: | |||||
|---|---|---|---|---|---|
| 46 | 47 | 48 | |||
| 1804 Jul 22 | 1822 Aug 03 | 1840 Aug 13 | |||
| 49 | 50 | 51 | |||
| 1858 Aug 24 | 1876 Sep 03 | 1894 Sep 15 | |||
| 52 | 53 | 54 | |||
| 1912 Sep 26 | 1930 Oct 07 | 1948 Oct 18 | |||
| 55 | 56 | 57 | |||
| 1966 Oct 29 | 1984 Nov 08 | 2002 Nov 20 | |||
| 58 | 59 | 60 | |||
| 2020 Nov 30 | 2038 Dec 11 | 2056 Dec 22 | |||
| 61 | 62 | 63 | |||
| 2075 Jan 02 | 2093 Jan 12 | 2111 Jan 25 | |||
| 64 | 65 | 66 | |||
| 2129 Feb 04 | 2147 Feb 15 | 2165 Feb 26 | |||
| 67 | |||||
| 2183 Mar 09 | |||||
Tritos series
This eclipse is a part of a tritos cycle, repeating at alternating nodes every 135 synodic months (≈ 3986.63 days, or 11 years minus 1 month). Their appearance and longitude are irregular due to a lack of synchronization with the anomalistic month (period of perigee), but groupings of 3 tritos cycles (≈ 33 years minus 3 months) come close (≈ 434.044 anomalistic months), so eclipses are similar in these groupings.
| Series members between 1801 and 2200 | |||||||||
|---|---|---|---|---|---|---|---|---|---|
| 1803 Feb 06 (Saros 101) | 1814 Jan 06 (Saros 102) | 1824 Dec 06 (Saros 103) | 1846 Oct 04 (Saros 105) | ||||||
| 1857 Sep 04 (Saros 106) | 1868 Aug 03 (Saros 107) | 1879 Jul 03 (Saros 108) | 1890 Jun 03 (Saros 109) | 1901 May 03 (Saros 110) | |||||
| 1912 Apr 01 (Saros 111) | 1923 Mar 03 (Saros 112) | 1934 Jan 30 (Saros 113) | 1944 Dec 29 (Saros 114) | 1955 Nov 29 (Saros 115) | |||||
| 1966 Oct 29 (Saros 116) | 1977 Sep 27 (Saros 117) | 1988 Aug 27 (Saros 118) | 1999 Jul 28 (Saros 119) | 2010 Jun 26 (Saros 120) | |||||
| 2021 May 26 (Saros 121) | 2032 Apr 25 (Saros 122) | 2043 Mar 25 (Saros 123) | 2054 Feb 22 (Saros 124) | 2065 Jan 22 (Saros 125) | |||||
| 2075 Dec 22 (Saros 126) | 2086 Nov 20 (Saros 127) | 2097 Oct 21 (Saros 128) | 2108 Sep 20 (Saros 129) | 2119 Aug 20 (Saros 130) | |||||
| 2130 Jul 21 (Saros 131) | 2141 Jun 19 (Saros 132) | 2152 May 18 (Saros 133) | 2163 Apr 19 (Saros 134) | 2174 Mar 18 (Saros 135) | |||||
| 2185 Feb 14 (Saros 136) | 2196 Jan 15 (Saros 137) | ||||||||
Inex series
This eclipse is a part of the long period inex cycle, repeating at alternating nodes, every 358 synodic months (≈ 10,571.95 days, or 29 years minus 20 days). Their appearance and longitude are irregular due to a lack of synchronization with the anomalistic month (period of perigee). However, groupings of 3 inex cycles (≈ 87 years minus 2 months) comes close (≈ 1,151.02 anomalistic months), so eclipses are similar in these groupings.
| Series members between 1801 and 2200 | |||||
|---|---|---|---|---|---|
| 1822 Feb 06 (Saros 111) | 1851 Jan 17 (Saros 112) | 1879 Dec 28 (Saros 113) | |||
| 1908 Dec 07 (Saros 114) | 1937 Nov 18 (Saros 115) | 1966 Oct 29 (Saros 116) | |||
| 1995 Oct 08 (Saros 117) | 2024 Sep 18 (Saros 118) | 2053 Aug 29 (Saros 119) | |||
| 2082 Aug 08 (Saros 120) | 2111 Jul 21 (Saros 121) | 2140 Jun 30 (Saros 122) | |||
| 2169 Jun 09 (Saros 123) | 2198 May 20 (Saros 124) | ||||
Half-Saros cycle
A lunar eclipse will be preceded and followed by solar eclipses by 9 years and 5.5 days (a half saros). This lunar eclipse is related to two solar eclipses of Solar Saros 123.
See also
Notes
External links
- Eclipse Predictions by Fred Espenak, NASA/GSFC