A penumbral lunar eclipse will occur at the Moon’s ascending node of orbit on Monday, May 17, 2049,[1] with an umbral magnitude of −0.2073.

A penumbral lunar eclipse occurs when part or all of the Moon's near side passes into the Earth's penumbra.

Occurring about 1.9 days before perigee (on May 19, 2049, at 15:25 UTC), the Moon's apparent diameter will be larger.

[2] The eclipse will be completely visible over Australia, Antarctica, and the Pacific Ocean, seen rising over east Asia and setting over much of North and South America.

This eclipse is a part of Saros series 112, repeating every 18 years, 11 days, and containing 72 events.