| bgcolor=#e7dcc3 colspan=2 | Total Lunar Eclipse January 19, 1954 | ||
|---|---|---|---|
| (No photo) | |||
The moon passes west to east (right to left) across the Earth's umbral shadow, shown in hourly intervals. | |||
| align=center bgcolor=#c0d0e0 | Series | 133 (23 of 71) | |
| align=center bgcolor=#c0d0e0 | Gamma | -0.4357 | |
| align=center bgcolor=#c0d0e0 | Magnitude | 1.0322 | |
| align=center bgcolor=#c0b0e0 colspan=2 | Duration (hr:mn:sc) | ||
| align=center bgcolor=#b0a0e0 | Totality | 28:23 | |
| align=center bgcolor=#c0a0e0 | Partial | 3:22:56 | |
| align=center bgcolor=#d0d0e0 | Penumbral | 5:41:22 | |
| align=center bgcolor=#a0d0e0 colspan=2 | Contacts (UTC) | ||
| align=center bgcolor=#d0d0e0 | P1 | 23:41:45 | |
| align=center bgcolor=#c0a0e0 | U1 | 0:50:54 | |
| align=center bgcolor=#b0a0e0 | U2 | 2:18:15 | |
| align=center bgcolor=#a0a0e0 | Greatest | 2:32:21 | |
| align=center bgcolor=#b0a0e0 | U3 | 2:46:27 | |
| align=center bgcolor=#c0a0e0 | U4 | 4:13:48 | |
| align=center bgcolor=#d0d0e0 | P4 | 5:22:57 | |
It was part of Saros series 133.
A lunar eclipse will be preceded and followed by solar eclipses by 9 years and 5.5 days (a half saros).[2] This lunar eclipse is related to two annular solar eclipses of Solar Saros 140.