June 2058 lunar eclipse

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Template:Short description Template:Infobox lunar eclipse A total lunar eclipse will occur at the Moon’s descending node of orbit on Thursday, June 6, 2058,[1] with an umbral magnitude of 1.6628. It will be a central lunar eclipse, in which part of the Moon will pass through the center of the Earth's shadow. 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 about 1.6 days before perigee (on June 8, 2058, at 9:30 UTC), the Moon's apparent diameter will be larger.[2]

During the eclipse, IC 4634 will be occulted by the Moon over Antarctica. Deep-sky objects are rarely occulted during a total eclipse from any given spot on Earth.[3]Template:Rp

Visibility

The eclipse will be completely visible over east Africa, Antarctica, west, central, and south Asia, and western Australia, seen rising over west Africa, Europe, and eastern South America and setting over east Asia and eastern Australia.[4]

File:Lunar eclipse from moon-2058Jun06.png File:Lunar eclipse chart close-2058Jun06.png

Eclipse details

Shown below is a table displaying details about this particular solar eclipse. It describes various parameters pertaining to this eclipse.[5]

June 6, 2058 Lunar Eclipse Parameters
Parameter Value
Penumbral Magnitude 2.62261
Umbral Magnitude 1.66277
Gamma −0.11810
Sun Right Ascension 05h00m41.7s
Sun Declination +22°43'57.0"
Sun Semi-Diameter 15'45.8"
Sun Equatorial Horizontal Parallax 08.7"
Moon Right Ascension 17h00m35.5s
Moon Declination -22°50'55.4"
Moon Semi-Diameter 16'25.3"
Moon Equatorial Horizontal Parallax 1°00'16.2"
ΔT 90.8 s

Eclipse season

Script error: No such module "Labelled list hatnote". 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. The first and last eclipse in this sequence is separated by one synodic month.

Eclipse season of May–June 2058
May 22
Ascending node (new moon)
June 6
Descending node (full moon)
June 21
Ascending node (new moon)
File:SE2058May22P.png File:Lunar eclipse chart close-2058Jun06.png File:SE2058Jun21P.png
Partial solar eclipse
Solar Saros 119
Total lunar eclipse
Lunar Saros 131
Partial solar eclipse
Solar Saros 157

Related eclipses

Eclipses in 2058

Metonic

Tzolkinex

Half-Saros

Tritos

Lunar Saros 131

Inex

Triad

Lunar eclipses of 2056–2060

Template:Lunar eclipse set 2056-2060

Saros 131

Template:Lunar Saros series 131

Tritos series

Template:Lunar Tritos series November 2003

Inex series

Template:Lunar Inex series July 2000

Half-Saros cycle

A lunar eclipse will be preceded and followed by solar eclipses by 9 years and 5.5 days (a half saros).[6] This lunar eclipse is related to two annular solar eclipses of Solar Saros 138.

May 31, 2049 June 11, 2067
File:SE2049May31A.png File:SE2067Jun11A.png

See also

Notes

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

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External links

Template:Lunar eclipses