June 1992 lunar eclipse explained

bgcolor=#e7dcc3 colspan=2Partial Lunar Eclipse
June 15, 1992

The moon passes west to east (right to left) across the Earth's umbral shadow, shown in hourly intervals.
align=center bgcolor=#c0d0e0Series120 (57 of 84)
align=center bgcolor=#c0d0e0Gamma-0.6288
align=center bgcolor=#c0d0e0Magnitude0.6822
align=center bgcolor=#c0b0e0 colspan=2Duration (hr:mn:sc)
align=center bgcolor=#c0a0e0 Partial 2:59:47
align=center bgcolor=#d0d0e0 Penumbral 5:32:10
align=center bgcolor=#a0d0e0 colspan=2Contacts UTC
align=center bgcolor=#d0d0e0 P1 19:19:49
align=center bgcolor=#c0a0e0 U1 20:31:49
align=center bgcolor=#a0a0e0Greatest 21:31:49
align=center bgcolor=#c0a0e0 U4 22:29:22
align=center bgcolor=#d0d0e0 P4 23:21:43
A partial lunar eclipse took place on Monday, June 15, 1992, the first of two lunar eclipses in 1992, the second being with a total lunar eclipse on Wednesday, December 9.

Related eclipses

Eclipses of 1992

Half-Saros cycle

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.

Tritos series

Tzolkinex

See also

External links

Notes and References

  1. Mathematical Astronomy Morsels, Jean Meeus, p.110, Chapter 18, The half-saros