| Type: | total |
| Date: | March 14, 2025 |
| Gamma: | 0.3485 |
| Magnitude: | 1.1804 |
| Saros Ser: | 123 |
| Saros No: | 53 of 72 |
| Totality: | 66 minutes, 3.9 seconds |
| Partiality: | 218 minutes, 55.8 seconds |
| Penumbral: | 363 minutes, 22.4 seconds |
| P1: | 3:57:09.4 |
| U1: | 5:09:22.6 |
| U2: | 6:25:57.5 |
| Greatest: | 6:58:44.5 |
| U3: | 7:32:01.5 |
| U4: | 8:48:18.5 |
| P4: | 10:00:31.9 |
| Previous: | September 2024 |
| Next: | September 2025 |
A total lunar eclipse will occur at the Moon’s descending node of orbit on Friday, March 14, 2025,[1] with an umbral magnitude of 1.1804. A lunar eclipse occurs when the Moon moves into the Earth's shadow, causing the Moon to be darkened. A total lunar eclipse occurs when the Moon's near side entirely passes into the Earth's umbral shadow. Unlike a solar eclipse, which can only be viewed from a relatively small area of the world, a lunar eclipse may be viewed from anywhere on the night side of Earth. A total lunar eclipse can last up to nearly two hours, while a total solar eclipse lasts only a few minutes at any given place, because the Moon's shadow is smaller. Occurring about 3.3 days before apogee (on March 17, 2025, at 12:35 UTC), the Moon's apparent diameter will be smaller.[2]
This lunar eclipse will be the first of an almost tetrad, with the others being on September 8, 2025 (total); March 3, 2026 (total); and August 28, 2026 (partial).[3]
The eclipse will be completely visible over North and South America, seen rising over Australia and northeast Asia and setting over Africa and Europe.[4]
Shown below is a table displaying details about this particular solar eclipse. It describes various parameters pertaining to this eclipse.[5]
| Penumbral Magnitude | 2.26146 | |
| Umbral Magnitude | 1.18038 | |
| Gamma | 0.34846 | |
| Sun Right Ascension | 23h37m46.0s | |
| Sun Declination | -02°24'16.8" | |
| Sun Semi-Diameter | 16'05.2" | |
| Sun Equatorial Horizontal Parallax | 08.8" | |
| Moon Right Ascension | 11h38m23.0s | |
| Moon Declination | +02°40'54.6" | |
| Moon Semi-Diameter | 14'52.8" | |
| Moon Equatorial Horizontal Parallax | 0°54'36.8" | |
| ΔT | 71.7 s |
See also: Eclipse cycle. This eclipse is part of an eclipse season, a period, roughly every six months, when eclipses occur. Only two (or occasionally three) eclipse seasons occur each year, and each season lasts about 35 days and repeats just short of six months (173 days) later; thus two full eclipse seasons always occur each year. Either two or three eclipses happen each eclipse season. In the sequence below, each eclipse is separated by a fortnight.
It last occurred on March 3, 2007 and will next occur on 25 March 2043.
A lunar eclipse will be preceded and followed by solar eclipses by 9 years and 5.5 days (a half saros).[6] Related to Solar Saros 130.