bgcolor=#e7dcc3 colspan=2 | Partial Lunar Eclipse June 15, 1992 | ||
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The moon passes west to east (right to left) across the Earth's umbral shadow, shown in hourly intervals. | |||
align=center bgcolor=#c0d0e0 | Series | 120 (57 of 84) | |
align=center bgcolor=#c0d0e0 | Gamma | -0.6288 | |
align=center bgcolor=#c0d0e0 | Magnitude | 0.6822 | |
align=center bgcolor=#c0b0e0 colspan=2 | Duration (hr:mn:sc) | ||
align=center bgcolor=#c0a0e0 | Partial | 2:59:47 | |
align=center bgcolor=#d0d0e0 | Penumbral | 5:32:10 | |
align=center bgcolor=#a0d0e0 colspan=2 | Contacts UTC | ||
align=center bgcolor=#d0d0e0 | P1 | 19:19:49 | |
align=center bgcolor=#c0a0e0 | U1 | 20:31:49 | |
align=center bgcolor=#a0a0e0 | Greatest | 21:31:49 | |
align=center bgcolor=#c0a0e0 | U4 | 22:29:22 | |
align=center bgcolor=#d0d0e0 | P4 | 23:21:43 |
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 127.