| Total eclipse | |||||||||||||||||
 | |||||||||||||||||
| Date | 30 October 2050 | ||||||||||||||||
|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
| Gamma | 0.4435 | ||||||||||||||||
| Magnitude | 1.0538[1] | ||||||||||||||||
| Saros cycle | 127 (44 of 72[2]) | ||||||||||||||||
| Totality | 34 minutes 30 seconds | ||||||||||||||||
| Partiality | 192 minutes 51 seconds | ||||||||||||||||
| Penumbral | 313 minutes 8 seconds | ||||||||||||||||
| |||||||||||||||||
A total lunar eclipse will take place on October 30, 2050.
This will be the second lunar eclipse in the 2050–2051 tetrad. Taking place near perigee, the Moon's apparent diameter will be larger.
- ^ For a partial or total lunar eclipse, this value denotes the umbral magnitude. For a penumbral lunar eclipse, this denotes the penumbral magnitude.
- ^ Lunar Saros 127 - Fred Espenak's GSFC Eclipse Canon