| bgcolor=#e7dcc3 colspan=2 | Total Lunar Eclipse October 7, 1949 | ||
|---|---|---|---|
| (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 | 126 (42 of 72) | |
| align=center bgcolor=#c0d0e0 | Gamma | -0.3219 | |
| align=center bgcolor=#c0d0e0 | Magnitude | 1.2236 | |
| align=center bgcolor=#c0b0e0 colspan=2 | Duration (hr:mn:sc) | ||
| align=center bgcolor=#b0a0e0 | Totality | 1:12:50 | |
| align=center bgcolor=#c0a0e0 | Partial | 3:42:53 | |
| align=center bgcolor=#d0d0e0 | Penumbral | 6:09:11 | |
| align=center bgcolor=#a0d0e0 colspan=2 | Contacts UTC | ||
| align=center bgcolor=#d0d0e0 | P1 | 23:52:19 | |
| align=center bgcolor=#c0a0e0 | U1 | 1:05:28 | |
| align=center bgcolor=#b0a0e0 | U2 | 2:50:31 | |
| align=center bgcolor=#a0a0e0 | Greatest | 2:56:55 | |
| align=center bgcolor=#b0a0e0 | U3 | 3:33:19 | |
| align=center bgcolor=#c0a0e0 | U4 | 4:48:22 | |
| align=center bgcolor=#d0d0e0 | P4 | 6:01:31 | |
A lunar eclipse will be preceded and followed by solar eclipses by 9 years and 5.5 days (a half saros).[1] This lunar eclipse is related to two total solar eclipses of Solar Saros 133.