| Total eclipse | |||||||||||||||||
 | |||||||||||||||||
| 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 | ||||||||||||||||
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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.
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.
- ^ For a partial or total lunar eclipse, this value denotes the umbral magnitude. For a penumbral lunar eclipse, this denotes the penumbral magnitude.