The entire eclipse will be visible from Africa, Europe, and the western half of Asia. Part or most of the eclipse will be visible from the Americas (except for westernmost North America), the eastern half of Asia, and western Australia.

Tritos series edit

The tritos series repeats 31 days short of 11 years at alternating nodes. Sequential events have incremental Saros cycle indices.

This series produces 23 total eclipses between June 22, 1880 and August 9, 2120.

Inex series edit

The inex series repeats eclipses 20 days short of 29 years, repeating on average every 10571.95 days. This period is equal to 358 lunations (synodic months) and 388.5 draconic months. Saros series increment by one on successive Inex events and repeat at alternate ascending and descending lunar nodes.

This period is 383.6734 anomalistic months (the period of the Moon's elliptical orbital precession). Despite the average 0.05 time-of-day shift between subsequent events, the variation of the Moon in its elliptical orbit at each event causes the actual eclipse time to vary significantly. It is a part of Lunar Inex series 35.

Lunar year series edit

Tzolkinex edit

• Preceded: Lunar eclipse of January 1, 2048

• Followed: Lunar eclipse of March 25, 2062

• List of lunar eclipses and List of 21st-century lunar eclipses

• 2055 Feb 11 chart Eclipse Predictions by Fred Espenak, NASA/GSFC