October 2032 lunar eclipse
| Total lunar eclipse October 18, 2032 | |
|---|---|
Ecliptic north up The moon will pass through the center of the Earth's shadow. | |
| Saros (and member) | 127 (43 of 72) |
| Gamma | |
| Duration (hr:mn:sc) | |
| Totality | |
| Partial | |
| Penumbral | |
| Contacts (UTC) | |
| P1 | |
| U1 | |
| U2 | |
| Greatest | |
| U3 | |
| U4 | |
| P4 | |
A total lunar eclipse will take place on October 18, 2032.[1]
Visibility
Related lunar eclipses
Lunar year series
| Ascending node | Descending node | |||||
|---|---|---|---|---|---|---|
| Saros | Date Viewing |
Type Chart |
Saros | Date Viewing |
Type Chart | |
| 112 | 2031 May 07 |
Penumbral |
117 | 2031 Oct 30 |
Penumbral | |
| 122 | 2032 Apr 25 |
Total |
127 | 2032 Oct 18 |
Total | |
| 132 | 2033 Apr 14 |
Total |
137 | 2033 Oct 08 |
Total | |
| 142 | 2034 Apr 03 |
Penumbral |
147 | 2034 Sep 28 |
Partial | |
| Last set | 2031 Jun 05 | Last set | 2030 Dec 09 | |||
| Next set | 2035 Feb 22 | Next set | 2035 Aug 19 | |||
Tritos series
The tritos series repeats 31 days short of 11 years at alternating nodes. Sequential events have incremental Saros cycle indices.
This series produces 20 total eclipses between April 24, 1967 and August 1, 2167, only being partial on November 19, 2021.
| Descending node | Ascending node | |||||
|---|---|---|---|---|---|---|
| Saros | Date Viewing |
Type chart |
Saros | Date Viewing |
Type chart | |
| 115 | 1901 Oct 27 |
Partial |
116 | 1912 Sep 26 |
Partial | |
| 117 | 1923 Aug 26 |
Partial |
118 | 1934 Jul 26 |
Partial | |
| 119 | 1945 Jun 25 |
Partial |
120 | 1956 May 24 |
Partial | |
| 121 | 1967 Apr 24 |
Total |
122 | 1978 Mar 24 |
Total | |
| 123 | 1989 Feb 20 |
Total |
124 | 2000 Jan 21 |
Total | |
| 125 | 2010 Dec 21 |
Total |
126 | 2021 Nov 19 |
Partial | |
| 127 | 2032 Oct 18 |
Total |
128 | 2043 Sep 19 |
Total | |
| 129 | 2058 Jun 6 |
Total |
130 | 2069 May 6 |
Total | |
| 131 | 2080 Apr 4 |
Total |
132 | 2091 Mar 5 |
Total | |
See also
Notes
External links
- 2032 Oct 18 chart: Eclipse Predictions by Fred Espenak, NASA/GSFC
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