| bgcolor=#e7dcc3 colspan=2 | Total Lunar Eclipse October 18, 1967 | ||
|---|---|---|---|
| (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 (43 of 72) | |
| align=center bgcolor=#c0d0e0 | Gamma | -0.3653 | |
| align=center bgcolor=#c0d0e0 | Magnitude | 1.1426 | |
| align=center bgcolor=#c0b0e0 colspan=2 | Duration (hr:mn:sc) | ||
| align=center bgcolor=#b0a0e0 | Totality | 59:45 | |
| align=center bgcolor=#c0a0e0 | Partial | 3:38:52 | |
| align=center bgcolor=#d0d0e0 | Penumbral | 6:07:07 | |
| align=center bgcolor=#a0d0e0 colspan=2 | Contacts UTC | ||
| align=center bgcolor=#d0d0e0 | P1 | 7:12:15 | |
| align=center bgcolor=#c0a0e0 | U1 | 8:26:21 | |
| align=center bgcolor=#b0a0e0 | U2 | 9:45:54 | |
| align=center bgcolor=#a0a0e0 | Greatest | 10:15:48 | |
| align=center bgcolor=#b0a0e0 | U3 | 10:45:42 | |
| align=center bgcolor=#c0a0e0 | U4 | 12:05:15 | |
| align=center bgcolor=#d0d0e0 | P4 | 13:19:21 | |
It was completely visible over Asia, Australia, Pacific Ocean, North America, South America, and Arctic, seen rising over Asia and Australia and setting over North America and South America.
This eclipse is the third of four Metonic cycle lunar eclipses on the same date, April 23–24, each separated by 19 years:
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 total solar eclipses of Solar Saros 133.