# October 2032 lunar eclipse

A total lunar eclipse will occur at the Moon’s descending node of orbit on Monday, October 18, 2032, with an umbral magnitude of 1.1039. A lunar eclipse occurs when the Moon moves into the Earth's shadow, causing the Moon to be darkened. A total lunar eclipse occurs when the Moon's near side entirely passes into the Earth's umbral shadow. 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. A total lunar eclipse can last up to nearly two hours, while a total solar eclipse lasts only a few minutes at any given place, because the Moon's shadow is smaller. Occurring about 2.1 days after perigee (on October 16, 2032, at 17:25 UTC), the Moon's apparent diameter will be larger.
This lunar eclipse is the second of a tetrad, with four total lunar eclipses in series, the others being on April 25, 2032; April 14, 2033; and October 8, 2033.

## Visibility

The eclipse will be completely visible over east Africa, Europe, and Asia, seen rising over west Africa and eastern South America and setting over Australia and the western Pacific Ocean.

## Eclipse details

Shown below is a table displaying details about this particular solar eclipse. It describes various parameters pertaining to this eclipse.
October 18, 2032 Lunar Eclipse Parameters :
| Parameter | Value |
| Penumbral Magnitude | 2.08413 |
| Umbral Magnitude | 1.10390 |
| Gamma | 0.41692 |
| Sun Right Ascension | 13h36m15.4s |
| Sun Declination | -10°01'20.8" |
| Sun Semi-Diameter | 16'03.4" |
| Sun Equatorial Horizontal Parallax | 08.8" |
| Moon Right Ascension | 01h35m47.9s |
| Moon Declination | +10°25'28.7" |
| Moon Semi-Diameter | 16'22.8" |
| Moon Equatorial Horizontal Parallax | 1°00'07.0" |
| ΔT | 75.3 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.
Eclipse season of October–November 2032 :
| October 18 Descending node (full moon) | November 3 Ascending node (new moon) |
| Total lunar eclipse Lunar Saros 127 | Partial solar eclipse Solar Saros 153 |

## Related eclipses
### Eclipses in 2032

* A total lunar eclipse on April 25.
* An annular solar eclipse on May 9.
* A total lunar eclipse on October 18.
* A partial solar eclipse on November 3.

### Metonic

* Preceded by: Lunar eclipse of December 31, 2028
* Followed by: Lunar eclipse of August 7, 2036

### Tzolkinex

* Preceded by: Lunar eclipse of September 7, 2025
* Followed by: Lunar eclipse of November 30, 2039

### Half-Saros

* Preceded by: Solar eclipse of October 14, 2023
* Followed by: Solar eclipse of October 25, 2041

### Tritos

* Preceded by: Lunar eclipse of November 19, 2021
* Followed by: Lunar eclipse of September 19, 2043

### Lunar Saros 127

* Preceded by: Lunar eclipse of October 8, 2014
* Followed by: Lunar eclipse of October 30, 2050

### Inex

* Preceded by: Lunar eclipse of November 9, 2003
* Followed by: Lunar eclipse of September 29, 2061

### Triad

* Preceded by: Lunar eclipse of December 19, 1945
* Followed by: Lunar eclipse of August 20, 2119

### Lunar eclipses of 2031–2034

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 June 5, 2031 occurs in the previous lunar year eclipse set.
Lunar eclipse series sets from 2031 to 2034 :
| Ascending node | Ascending node | Ascending node | Ascending node | Descending node | Descending node | Descending node | Descending node |
| Saros | Date Viewing | Type Chart | Gamma | Saros | Date Viewing | Type Chart | Gamma |
| 112 | 2031 May 07 | Penumbral | −1.0694 | 117 | 2031 Oct 30 | Penumbral | 1.1774 |
| 122 | 2032 Apr 25 | Total | −0.3558 | 127 | 2032 Oct 18 | Total | 0.4169 |
| 132 | 2033 Apr 14 | Total | 0.3954 | 137 | 2033 Oct 08 | Total | −0.2889 |
| 142 | 2034 Apr 03 | Penumbral | 1.1144 | 147 | 2034 Sep 28 | Partial | −1.0110 |

### Saros 127

This eclipse is a part of Saros series 127, repeating every 18 years, 11 days, and containing 72 events. The series started with a penumbral lunar eclipse on July 9, 1275. It contains partial eclipses from November 4, 1473 through May 18, 1780; total eclipses from May 29, 1798 through November 9, 2068; and a second set of partial eclipses from November 20, 2086 through June 17, 2429. The series ends at member 72 as a penumbral eclipse on September 2, 2555.
The longest duration of totality was produced by member 35 at 101 minutes, 46 seconds on July 23, 1888. All eclipses in this series occur at the Moon’s descending node of orbit.
| Greatest | First | First | First | First |
| The greatest eclipse of the series occurred on 1888 Jul 23, lasting 101 minutes, 46 seconds. | Penumbral | Partial | Total | Central |
| The greatest eclipse of the series occurred on 1888 Jul 23, lasting 101 minutes, 46 seconds. | 1275 Jul 09 | 1473 Nov 04 | 1798 May 29 | 1834 Jun 21 |
| Last ||||
| The greatest eclipse of the series occurred on 1888 Jul 23, lasting 101 minutes, 46 seconds. | Central | Total | Partial | Penumbral |
| The greatest eclipse of the series occurred on 1888 Jul 23, lasting 101 minutes, 46 seconds. | 1960 Sep 05 | 2068 Nov 09 | 2429 Jun 17 | 2555 Sep 02 |
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 31–52 occur between 1801 and 2200: :
| 31 | 31 | 32 | 32 | 33 | 33 |
| 1816 Jun 10 | 1816 Jun 10 | 1834 Jun 21 | 1834 Jun 21 | 1852 Jul 01 | 1852 Jul 01 |
| 34 | 34 | 35 | 35 | 36 | 36 |
| 1870 Jul 12 | 1870 Jul 12 | 1888 Jul 23 | 1888 Jul 23 | 1906 Aug 04 | 1906 Aug 04 |
| 37 | 37 | 38 | 38 | 39 | 39 |
| 1924 Aug 14 | 1924 Aug 14 | 1942 Aug 26 | 1942 Aug 26 | 1960 Sep 05 | 1960 Sep 05 |
| 40 | 40 | 41 | 41 | 42 | 42 |
| 1978 Sep 16 | 1978 Sep 16 | 1996 Sep 27 | 1996 Sep 27 | 2014 Oct 08 | 2014 Oct 08 |
| 43 | 43 | 44 | 44 | 45 | 45 |
| 2032 Oct 18 | 2032 Oct 18 | 2050 Oct 30 | 2050 Oct 30 | 2068 Nov 09 | 2068 Nov 09 |
| 46 | 46 | 47 | 47 | 48 | 48 |
| 2086 Nov 20 | 2086 Nov 20 | 2104 Dec 02 | 2104 Dec 02 | 2122 Dec 13 | 2122 Dec 13 |
| 49 | 49 | 50 | 50 | 51 | 51 |
| 2140 Dec 23 | 2140 Dec 23 | 2159 Jan 04 | 2159 Jan 04 | 2177 Jan 14 | 2177 Jan 14 |
| 52 ||
| 2195 Jan 26 ||

### 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 Aug 03 (Saros 106) | 1803 Aug 03 (Saros 106) | 1814 Jul 02 (Saros 107) | 1814 Jul 02 (Saros 107) | 1825 Jun 01 (Saros 108) | 1825 Jun 01 (Saros 108) | 1836 May 01 (Saros 109) | 1836 May 01 (Saros 109) | 1847 Mar 31 (Saros 110) | 1847 Mar 31 (Saros 110) |
| 1858 Feb 27 (Saros 111) | 1858 Feb 27 (Saros 111) | 1869 Jan 28 (Saros 112) | 1869 Jan 28 (Saros 112) | 1879 Dec 28 (Saros 113) | 1879 Dec 28 (Saros 113) | 1890 Nov 26 (Saros 114) | 1890 Nov 26 (Saros 114) | 1901 Oct 27 (Saros 115) | 1901 Oct 27 (Saros 115) |
| 1912 Sep 26 (Saros 116) | 1912 Sep 26 (Saros 116) | 1923 Aug 26 (Saros 117) | 1923 Aug 26 (Saros 117) | 1934 Jul 26 (Saros 118) | 1934 Jul 26 (Saros 118) | 1945 Jun 25 (Saros 119) | 1945 Jun 25 (Saros 119) | 1956 May 24 (Saros 120) | 1956 May 24 (Saros 120) |
| 1967 Apr 24 (Saros 121) | 1967 Apr 24 (Saros 121) | 1978 Mar 24 (Saros 122) | 1978 Mar 24 (Saros 122) | 1989 Feb 20 (Saros 123) | 1989 Feb 20 (Saros 123) | 2000 Jan 21 (Saros 124) | 2000 Jan 21 (Saros 124) | 2010 Dec 21 (Saros 125) | 2010 Dec 21 (Saros 125) |
| 2021 Nov 19 (Saros 126) | 2021 Nov 19 (Saros 126) | 2032 Oct 18 (Saros 127) | 2032 Oct 18 (Saros 127) | 2043 Sep 19 (Saros 128) | 2043 Sep 19 (Saros 128) | 2054 Aug 18 (Saros 129) | 2054 Aug 18 (Saros 129) | 2065 Jul 17 (Saros 130) | 2065 Jul 17 (Saros 130) |
| 2076 Jun 17 (Saros 131) | 2076 Jun 17 (Saros 131) | 2087 May 17 (Saros 132) | 2087 May 17 (Saros 132) | 2098 Apr 15 (Saros 133) | 2098 Apr 15 (Saros 133) | 2109 Mar 17 (Saros 134) | 2109 Mar 17 (Saros 134) | 2120 Feb 14 (Saros 135) | 2120 Feb 14 (Saros 135) |
| 2131 Jan 13 (Saros 136) | 2131 Jan 13 (Saros 136) | 2141 Dec 13 (Saros 137) | 2141 Dec 13 (Saros 137) | 2152 Nov 12 (Saros 138) | 2152 Nov 12 (Saros 138) | 2163 Oct 12 (Saros 139) | 2163 Oct 12 (Saros 139) | 2174 Sep 11 (Saros 140) | 2174 Sep 11 (Saros 140) |
| 2185 Aug 11 (Saros 141) | 2185 Aug 11 (Saros 141) | 2196 Jul 10 (Saros 142) | 2196 Jul 10 (Saros 142) |

### 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 :
| 1801 Mar 30 (Saros 119) | 1801 Mar 30 (Saros 119) | 1830 Mar 09 (Saros 120) | 1830 Mar 09 (Saros 120) | 1859 Feb 17 (Saros 121) | 1859 Feb 17 (Saros 121) |
| 1888 Jan 28 (Saros 122) | 1888 Jan 28 (Saros 122) | 1917 Jan 08 (Saros 123) | 1917 Jan 08 (Saros 123) | 1945 Dec 19 (Saros 124) | 1945 Dec 19 (Saros 124) |
| 1974 Nov 29 (Saros 125) | 1974 Nov 29 (Saros 125) | 2003 Nov 09 (Saros 126) | 2003 Nov 09 (Saros 126) | 2032 Oct 18 (Saros 127) | 2032 Oct 18 (Saros 127) |
| 2061 Sep 29 (Saros 128) | 2061 Sep 29 (Saros 128) | 2090 Sep 08 (Saros 129) | 2090 Sep 08 (Saros 129) | 2119 Aug 20 (Saros 130) | 2119 Aug 20 (Saros 130) |
| 2148 Jul 31 (Saros 131) | 2148 Jul 31 (Saros 131) | 2177 Jul 11 (Saros 132) | 2177 Jul 11 (Saros 132) |

### 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 partial solar eclipses of Solar Saros 134.
| October 14, 2023 | October 25, 2041 |