June 2075 lunar eclipse


A partial lunar eclipse will occur at the Moon’s descending node of orbit on Friday, June 28, 2075, with an umbral magnitude of 0.6235. A lunar eclipse occurs when the Moon moves into the Earth's shadow, causing the Moon to be darkened. A partial lunar eclipse occurs when one part of the Moon is in the Earth's umbra, while the other part is in the Earth's penumbra. Unlike a solar eclipse, which can only be viewed from a relatively small area of the world, a lunar eclipse may be viewed from anywhere on the night side of Earth. Occurring only about 5.5 hours after perigee, the Moon's apparent diameter will be larger.

Visibility

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

Eclipse details

Shown below is a table displaying details about this particular solar eclipse. It describes various parameters pertaining to this eclipse.
ParameterValue
Penumbral Magnitude1.56389
Umbral Magnitude0.62349
Gamma0.68971
Sun Right Ascension06h29m58.9s
Sun Declination+23°14'59.1"
Sun Semi-Diameter15'44.0"
Sun Equatorial Horizontal Parallax08.7"
Moon Right Ascension18h30m07.3s
Moon Declination-22°32'40.9"
Moon Semi-Diameter16'43.9"
Moon Equatorial Horizontal Parallax1°01'24.3"
ΔT104.0 s

Eclipse season

This eclipse is part of an eclipse season, a period, roughly every six months, when eclipses occur. Only two eclipse seasons occur each year, and each season lasts about 35 days and repeats just short of six months later; thus two full eclipse seasons always occur each year. Either two or three eclipses happen each eclipse season. In the sequence below, each eclipse is separated by a fortnight.
June 28
Descending node
July 13
Ascending node
Partial lunar eclipse
Lunar Saros 121		Annular solar eclipse
Solar Saros 147

Related eclipses

Eclipses in 2075

This eclipse is a member of a semester series. An eclipse in a semester series of lunar eclipses repeats approximately every 177 days and 4 hours at alternating nodes of the Moon's orbit.
The penumbral lunar eclipses on February 11, 2074 and August 7, 2074 occur in the previous lunar year eclipse set, and the penumbral lunar eclipses on April 27, 2078 and October 21, 2078 occur in the next lunar year eclipse set.

Saros 121

Tritos series

Half-Saros cycle

A lunar eclipse will be preceded and followed by solar eclipses by 9 years and 5.5 days. This lunar eclipse is related to two total solar eclipses of Solar Saros 128.
June 22, 2066July 3, 2084