A total lunar eclipse will occur at the Moon’s descending node of orbit on Sunday, August 28, 2072, with an umbral magnitude of 1.1673. A lunar eclipse occurs when the Moon moves into the Earth's shadow, causing the Moon to be darkened. A total lunar eclipse occurs when the Moon's near side entirely passes into the Earth's umbral shadow. 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. A total lunar eclipse can last up to nearly two hours, while a total solar eclipse lasts only a few minutes at any given place, because the Moon's shadow is smaller. Occurring only about 4.5 hours before apogee (on August 28, 2072, at 20:40 UTC), the Moon's apparent diameter will be smaller.

This lunar eclipse will be the second of a tetrad, with four total lunar eclipses in series, the others being on March 4, 2072; February 22, 2073; and August 17, 2073.

Visibility The eclipse will be completely visible over southeast and east Asia, Australia, and Antarctica, seen rising over Africa, Europe, and west and central Asia and setting over the eastern Pacific Ocean and western North America.

Eclipse details Shown below is a table displaying details about this particular lunar eclipse. It describes various parameters pertaining to this eclipse.

+August 28, 2072 Lunar Eclipse Parameters Parameter Value Penumbral Magnitude 2.24389 Umbral Magnitude 1.16727 Gamma 0.35634 Sun Right Ascension 10h31m55.6s Sun Declination +09°13'37.7" Sun Semi-Diameter 15'50.1" Sun Equatorial Horizontal Parallax 08.7" Moon Right Ascension 22h31m34.3s Moon Declination -08°55'07.7" Moon Semi-Diameter 14'42.5" Moon Equatorial Horizontal Parallax 0°53'58.7" ΔT 101.6 s

Eclipse season

This eclipse is part of an eclipse season, a period, roughly every six months, when eclipses occur. Only two (or occasionally three) eclipse seasons occur each year, and each season lasts about 35 days and repeats just short of six months (173 days) 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.

+ Eclipse season of August–September 2072 August 28Descending node (full moon) September 12Ascending node (new moon) Total lunar eclipseLunar Saros 129 Total solar eclipseSolar Saros 155

Related eclipses Eclipses in 2072 A total lunar eclipse on March 4. A partial solar eclipse on March 19. A total lunar eclipse on August 28. A total solar eclipse on September 12.

Metonic Preceded by: Lunar eclipse of November 9, 2068 Followed by: Lunar eclipse of June 17, 2076

Tzolkinex Preceded by: Lunar eclipse of July 17, 2065 Followed by: Lunar eclipse of October 10, 2079

Half-Saros Preceded by: Solar eclipse of August 24, 2063 Followed by: Solar eclipse of September 3, 2081

Tritos Preceded by: Lunar eclipse of September 29, 2061 Followed by: Lunar eclipse of July 29, 2083

Lunar Saros 129 Preceded by: Lunar eclipse of August 18, 2054 Followed by: Lunar eclipse of September 8, 2090

Inex Preceded by: Lunar eclipse of September 19, 2043 Followed by: Lunar eclipse of August 9, 2101

Triad Preceded by: Lunar eclipse of October 28, 1985 Followed by: Lunar eclipse of June 30, 2159

Lunar eclipses of 2071–2074 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 (a semester) at alternating nodes of the Moon's orbit.

The penumbral lunar eclipse on July 8, 2074 occurs in the next lunar year eclipse set.

Lunar eclipse series sets from 2071 to 2074 Ascending node  Descending node Saros DateViewing TypeChart Gamma Saros DateViewing TypeChart Gamma 114 2071 Mar 16Penumbral −1.0756 119 2071 Sep 09Penumbral 1.0834 1242072 Mar 04Total −0.3430 129 2072 Aug 28Total 0.3563 134 2073 Feb 22Total 0.3388 139 2073 Aug 17Total −0.3998 144 2074 Feb 11Penumbral 1.0611 149 2074 Aug 07Penumbral −1.1291

Saros 129

Tritos series

Inex series

Half-Saros cycle A lunar eclipse will be preceded and followed by solar eclipses by 9 years and 5.5 days (a half saros).Mathematical Astronomy Morsels, Jean Meeus, p.110, Chapter 18, The half-saros This lunar eclipse is related to two total solar eclipses of Solar Saros 136. August 24, 2063September 3, 2081

See also List of lunar eclipses and List of 21st-century lunar eclipses

Notes

External links