| bgcolor=#e7dcc3 colspan=2 | Total Lunar Eclipse May 6, 2069 | |
|---|---|---|
| align=center colspan=2 | The Moon passes west to east (right to left) across the Earth's umbral shadow, shown in hourly intervals. | |
| align=center bgcolor=#c0d0e0 | 132 (33 of 71) | |
| align=center bgcolor=#c0d0e0 | 0.272 | |
| align=center bgcolor=#c0d0e0 | 1.327 | |
| align=center bgcolor=#c0b0e0 colspan=2 | Duration (hr:mn:sc) | |
| align=center bgcolor=#b0a0e0 | Totality | 01:24:16 |
| align=center bgcolor=#c0a0e0 | Partial | 03:46:11 |
| align=center bgcolor=#d0d0e0 | Penumbral | 06:08:07 |
| align=center bgcolor=#a0d0e0 colspan=2 | Contacts | |
| align=center bgcolor=#d0d0e0 | P1 | 06:03:38 UTC |
| align=center bgcolor=#c0a0e0 | U1 | 07:14:38 UTC |
| align=center bgcolor=#b0a0e0 | U2 | 08:25:35 UTC |
| align=center bgcolor=#a0a0e0 | Greatest | 09:07:43 UTC |
| align=center bgcolor=#b0a0e0 | U3 | 09:49:42 UTC |
| align=center bgcolor=#c0a0e0 | U4 | 11:00:49 UTC |
| align=center bgcolor=#d0d0e0 | P4 | 12:11:45 UTC |
The eclipse occurs in the constellation Libra at the ascending node of the moon's orbit. | ||
It is the first of two total lunar eclipses in 2069, the second occurring at the descending node of the Moon's orbit will be on October 30, which will also be a central total eclipse.
It is the third of an almost tetrad, the others being 17 May 2068 (P), 9 Nov 2068 (T) and 30 October 2069 (T).
The eclipse will be visible after sunset over Australia and begin before sunset over far eastern Asia, and be seen in the predawn hours over western North and South America.
The Moon will also occult the bright star Alpha Librae as seen from the southern hemisphere a few hours before greatest eclipse.[1]
Lunar eclipses are related by many different eclipse cycles. The Saros cycle (18 years and 10 days) repeats the most consistently due three coinciding periods, and continue over 70 events (1200+ years). Eclipses are identified by a Saros number and a member index within each series.
The lunar year (354 days) and Metonic cycles (19 years) are short period last only 8 to 10 events. The Metonic cycle is equal to one Saros cycle plus one lunar year, and so the two series progress in parallel.
The Inex cycle (29 years minus 20 days) can last tens of thousands of years, so long that long perturbations in the Moon's path must be taken into account for prediction. Also the eclipse qualities are less inconsistent because the Moon is at different significantly positions in its elliptical orbit in sequential events. Similarly for the shorter Tritos cycle (10 years and 31 days), repeats less consistently for the same reason.
This eclipse is the third of four lunar year eclipses occurring at the Moon's ascending node.
The lunar year series repeats after 12 lunations or 354 days (Shifting back about 10 days in sequential years). Because of the date shift, the Earth's shadow will be about 11 degrees west in sequential events.
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 139.