| Total eclipse | |||||||||||||||||
 | |||||||||||||||||
| Date | 25 March 2043 | ||||||||||||||||
|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
| Gamma | 0.3849 | ||||||||||||||||
| Magnitude | 1.1142[1] | ||||||||||||||||
| Saros cycle | 123 (54 of 72[2]) | ||||||||||||||||
| Totality | 53 minutes 24 seconds | ||||||||||||||||
| Partiality | 214 minutes 37 seconds | ||||||||||||||||
| Penumbral | 359 minutes 16 seconds | ||||||||||||||||
| |||||||||||||||||
A total lunar eclipse will take place on March 25, 2043.
This lunar eclipse is the first of a tetrad, four total lunar eclipses in series. The last series was in 2032 and 2033, starting with an April 2032 lunar eclipse. The next tetrad series is in 2050 and 2051, starting with the May 2050 lunar eclipse.
- ^ 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 123 - Fred Espenak and Jean Meeus (NASA's GSFC)