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June 2010 lunar eclipse

June 2010 lunar eclipse
Partial eclipse
Partiality as viewed from Canberra, Australia, 11:31 UTC
DateJune 26, 2010
Gamma−0.7091
Magnitude0.5383
Saros cycle120 (58 of 84)
Partiality162 minutes, 52 seconds
Penumbral322 minutes, 7 seconds
Contacts (UTC)
P18:57:24
U110:16:58
Greatest11:38:27
U412:59:50
P414:19:31

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]


Hourly motion shown right to left

The Moon's hourly motion across the Earth's shadow in the constellation of Sagittarius.

Visibility map

Images

NASA chart of the eclipse

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

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)
Partial lunar eclipse
Lunar Saros 120
Total solar eclipse
Solar Saros 146

Eclipses in 2010

Metonic

Tzolkinex

Half-Saros

Tritos

Lunar Saros 120

Inex

Triad

Lunar eclipses of 2009–2013

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.[5]

The penumbral lunar eclipses on February 9, 2009 and August 6, 2009 occur in the previous lunar year eclipse set, and the lunar eclipses on April 25, 2013 (partial) and October 18, 2013 (penumbral) occur in the next lunar year eclipse set.

Lunar eclipse series sets from 2009 to 2013
Ascending node   Descending node
Saros Date
Viewing
Type
Chart
Gamma Saros Date
Viewing
Type
Chart
Gamma
110 2009 Jul 07
Penumbral
−1.4916 115
2009 Dec 31
Partial
0.9766
120
2010 Jun 26
Partial
−0.7091 125
2010 Dec 21
Total
0.3214
130
2011 Jun 15
Total
0.0897 135
2011 Dec 10
Total
−0.3882
140
2012 Jun 04
Partial
0.8248 145 2012 Nov 28
Penumbral
−1.0869
150 2013 May 25
Penumbral
1.5351

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 be in nearly the same location relative to the background stars.

Ascending node Descending node
  1. 1991 Jun 27 - penumbral (110)
  2. 2010 Jun 26 - partial (120)
  3. 2029 Jun 26 - total (130)
  4. 2048 Jun 26 - partial (140)
  5. 2067 Jun 27 - penumbral (150)
  1. 1991 Dec 21 - partial (115)
  2. 2010 Dec 21 - total (125)
  3. 2029 Dec 20 - total (135)
  4. 2048 Dec 20 - partial (145)

Saros 120

This eclipse is a part of Saros series 120, repeating every 18 years, 11 days, and containing 83 events. The series started with a penumbral lunar eclipse on October 16, 1000. It contains partial eclipses from May 31, 1379 through August 4, 1487; total eclipses from August 14, 1505 through May 14, 1938; and a second set of partial eclipses from May 24, 1956 through July 28, 2064. The series ends at member 83 as a penumbral eclipse on April 7, 2479.

The longest duration of totality was produced by member 43 at 104 minutes, 55 seconds on January 24, 1758. All eclipses in this series occur at the Moon’s ascending node of orbit.[6]

Greatest First
The greatest eclipse of the series occurred on 1758 Jan 24, lasting 104 minutes, 55 seconds.[7] Penumbral Partial Total Central
1000 Oct 16
1379 May 31
1505 Aug 14
1559 Sep 16
Last
Central Total Partial Penumbral
1902 Apr 22
1938 May 14
2064 Jul 28
2479 Apr 07

Eclipses are tabulated in three columns; every third eclipse in the same column is one exeligmos apart, so they all cast shadows over approximately the same parts of the Earth.

Half-Saros cycle

A lunar eclipse will be preceded and followed by solar eclipses by 9 years and 5.5 days (a half saros).[8] This lunar eclipse is related to two total solar eclipses of Solar Saros 127.

June 21, 2001 July 2, 2019

See also

Notes

  1. ^ "June 25–26, 2010 Partial Lunar Eclipse". timeanddate. Retrieved 15 November 2024.
  2. ^ "Moon Distances for London, United Kingdom, England". timeanddate. Retrieved 15 November 2024.
  3. ^ "Partial Lunar Eclipse of 2010 Jun 26" (PDF). NASA. Retrieved 15 November 2024.
  4. ^ "Partial Lunar Eclipse of 2010 Jun 26". EclipseWise.com. Retrieved 15 November 2024.
  5. ^ van Gent, R.H. "Solar- and Lunar-Eclipse Predictions from Antiquity to the Present". A Catalogue of Eclipse Cycles. Utrecht University. Retrieved 6 October 2018.
  6. ^ "NASA - Catalog of Lunar Eclipses of Saros 120". eclipse.gsfc.nasa.gov.
  7. ^ Listing of Eclipses of series 120
  8. ^ Mathematical Astronomy Morsels, Jean Meeus, p.110, Chapter 18, The half-saros

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