June 2010 lunar eclipse

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Template:Short description Template:Use dmy dates Template:Infobox lunar eclipse A partial lunar eclipse occurred at the Moon’s ascending node of orbit on Saturday, June 26, 2010,[1] with an umbral magnitude of 0.5383. 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 about 4.7 days before apogee (on July 1, 2010, at 6:10 UTC), the Moon's apparent diameter was smaller.[2]

Visibility

The eclipse was completely visible over much of Australia and the Pacific Ocean, seen rising over Asia and setting over North and South America.[3]

File:Lunar eclipse from moon-2010Jun26.png File:Lunar eclipse chart close-2010jun26.png
Hourly motion shown right to left
File:Lunar eclipse chart-10jun26.png
The Moon's hourly motion across the Earth's shadow in the constellation of Sagittarius.
File:Visibility Lunar Eclipse 2010-06-26.png
Visibility map

Images

File:2010-06-26 Lunar Eclipse Sketch.png
NASA chart of the eclipse

Gallery

Timing

The eclipse was seen before sunrise on Saturday morning setting over western North and South America.

Times of over North America
Event PDT
(UTC−7)
MDT
(UTC−6)
CDT
(UTC−5)
EDT
(UTC−4)
UTC
Start penumbral (P1) 1:57 a.m. 2:57 a.m. 3:57 a.m. 4:57 a.m. 8:57 a.m.
Start umbral (U1) 3:17 a.m. 4:17 a.m. 5:17 a.m. 6:17 a.m. 10:17 a.m.
Greatest eclipse 4:38 a.m. 5:38 a.m. Set Set 11:38 a.m.
End umbral (U4) Set Set Set Set 1:00 p.m.
End penumbral (P4) Set Set Set Set 2:20 p.m.

Eclipse details

Shown below is a table displaying details about this particular solar eclipse. It describes various parameters pertaining to this eclipse.[4]

June 26, 2010 Lunar Eclipse Parameters
Parameter Value
Penumbral Magnitude 1.57888
Umbral Magnitude 0.53830
Gamma −0.70911
Sun Right Ascension 06h20m48.6s
Sun Declination +23°21'07.6"
Sun Semi-Diameter 15'44.1"
Sun Equatorial Horizontal Parallax 08.7"
Moon Right Ascension 18h21m11.8s
Moon Declination -24°00'06.9"
Moon Semi-Diameter 15'07.3"
Moon Equatorial Horizontal Parallax 0°55'29.7"
ΔT 66.2 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.

Eclipse season of June–July 2010
June 26
Ascending node (full moon)
July 11
Descending node (new moon)
File:Lunar eclipse chart close-2010jun26.png File:SE2010Jul11T.png
Partial lunar eclipse
Lunar Saros 120
Total solar eclipse
Solar Saros 146

Related eclipses

Eclipses in 2010

Metonic

Tzolkinex

Half-Saros

Tritos

Lunar Saros 120

Inex

Triad

Lunar eclipses of 2009–2013

Template:Lunar eclipse set 2009-2013

Metonic series

Template:Metonic lunar eclipse 1991-2048

Saros 120

Template:Lunar Saros series 120

Tritos series

Template:Lunar Tritos series June 2010

Inex series

Template:Lunar Inex series June 2010

Half-Saros cycle

A lunar eclipse will be preceded and followed by solar eclipses by 9 years and 5.5 days (a half saros).[5] This lunar eclipse is related to two total solar eclipses of Solar Saros 127.

June 21, 2001 July 2, 2019
File:SE2001Jun21T.png File:SE2019Jul02T.png

See also

Notes

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

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External links

Template:Sister project

Photos:

Template:Lunar eclipses