The first table outlines times at which the moon's penumbra or umbra attains the specific parameter, and the second table describes various other parameters pertaining to this eclipse.

This eclipse is a part of Saros series 118, repeating every 18 years, 11 days, and containing 72 events.

The longest duration of totality was produced by member 34 at 6 minutes, 59 seconds on May 16, 1398, and the longest duration of annularity was produced by member 59 at 1 minutes, 58 seconds on February 23, 1849.

All eclipses in this series occur at the Moon’s descending node of orbit.

[4] The metonic series repeats eclipses every 19 years (6939.69 days), lasting about 5 cycles.

Their appearance and longitude are irregular due to a lack of synchronization with the anomalistic month (period of perigee).