May_1966_lunar_eclipse

May 1966 lunar eclipse

May 1966 lunar eclipse

Penumbral lunar eclipse May 4, 1966


A penumbral lunar eclipse took place on Wednesday, May 4, 1966, the first of two penumbral lunar eclipses in 1966. It was visible from South America, Europe, Africa, Asia, Australia and Antarctica.[1]

Visibility

The penumbral eclipse was visible in South America, Europe, Africa, central Asia and Australia, seen rising over North Atlantic Ocean and South America and setting over Australia, South China Sea and East China Sea as of today.

Lunar year series

More information Lunar eclipse series sets from 1966–1969, Descending node ...

Saros series

Lunar Saros 111, repeating every 18 years and 11 days, has a total of 71 lunar eclipse events including 11 total lunar eclipses. The first total lunar eclipse of this series was on April 19, 1353, and last was on August 4, 1533. The longest occurrence of this series was on June 12, 1443 when the totality lasted 106 minutes.

Metonic series

The metonic cycle repeats nearly exactly every 19 years and represents a Saros cycle plus one lunar year. Because it occurs on the same calendar date, the Earth's shadow will in nearly the same location relative to the background stars.

More information Metonic events: May 4 and October 28, Descending node ...

Half-Saros cycle

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 solar eclipses of Solar Saros 118.

More information April 30, 1957 ...

See also


Notes

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



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