October 2051 lunar eclipse
A total lunar eclipse will take place on October 19, 2051. The northern limb of the Moon will pass through the center of the Earth's shadow.
| Total eclipse | |||||||||||||||||
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| Date | 19 October 2051 | ||||||||||||||||
|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
| Gamma | −0.2542 | ||||||||||||||||
| Magnitude | 1.4118[1] | ||||||||||||||||
| Saros cycle | 137 (28 of 78) | ||||||||||||||||
| Totality | 83 minutes 34 seconds | ||||||||||||||||
| Partiality | 204 minutes 17 seconds | ||||||||||||||||
| Penumbral | 314 minutes 11 seconds | ||||||||||||||||
| |||||||||||||||||
This will be the first central eclipse of Saros series 137 and the fourth and final lunar eclipse in the 2050–2051 tetrad.
Less than a day from perigee, the Moon's apparent diameter will be larger, and be considered a supermoon.
Visibility
It will be completely visible over Central Asia, and Africa, seen rising over Western Africa, and South America, and setting over Australia.

Related lunar eclipses
Lunar year series
| Ascending node | Descending node | |||||
|---|---|---|---|---|---|---|
| Saros | Date Viewing |
Type Chart |
Saros | Date Viewing |
Type Chart | |
| 112 | 2049 May 17![]() |
Penumbral![]() |
117 | 2049 Nov 09![]() |
Penumbral![]() | |
| 122 | 2050 May 06![]() |
Total![]() |
127 | 2050 Oct 30![]() |
Total![]() | |
| 132 | 2051 Apr 26![]() |
Total![]() |
137 | 2051 Oct 19![]() |
Total![]() | |
| 142 | 2052 Apr 14![]() |
Penumbral![]() |
147 | 2052 Oct 08![]() |
Partial![]() | |
| Last set | 2049 Jun 15 | Last set | 2048 Dec 20 | |||
| Next set | 2053 Aug 29 | Next set | 2053 Mar 04 | |||
Saros series
It is part of Saros series 137.
Notes
- For a partial or total lunar eclipse, this value denotes the umbral magnitude. For a penumbral lunar eclipse, this denotes the penumbral magnitude.
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