bgcolor=#e7dcc3 colspan=2 | Penumbral Lunar Eclipse 18 July 2027 | ||
---|---|---|---|
align=center colspan=2 | The moon will imperceptibly dim as it clips the Earth's southern penumbral shadow | ||
align=center bgcolor=#c0d0e0 | 110 (72 of 72) | ||
align=center bgcolor=#c0d0e0 | -1.576 | ||
align=center bgcolor=#c0d0e0 | 0.0014 | ||
align=center bgcolor=#c0b0e0 colspan=2 | Duration (hr:mn:sc) | ||
align=center bgcolor=#d0d0e0 | Penumbral | 0:11:47 | |
align=center bgcolor=#a0d0e0 colspan=2 | Contacts | ||
align=center bgcolor=#d0d0e0 | P1 | ||
align=center bgcolor=#a0a0e0 | Greatest | 16:02:53 | |
align=center bgcolor=#d0d0e0 | P4 | 16:08:45 |
Insofar as it is visible at all, it will be visible over Asia and Australia.
This eclipse is a member of Saros series 110. The previous event occurred on July 7, 2009. This is the last lunar eclipse of this series.
A lunar eclipse will be preceded and followed by solar eclipses by 9 years and 5.5 days (a half saros).[3] This lunar eclipse is related to two partial solar eclipses of Solar Saros 117.