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Solar eclipse of June 1, 2011

From Wikipedia, the free encyclopedia
21st-century partial solar eclipse
Solar eclipse of June 1, 2011
Partial eclipse
Partial fromTromsø, Norway
Map
Gamma1.213
Magnitude0.601
Maximum eclipse
Coordinates67°48′N46°48′E / 67.8°N 46.8°E /67.8; 46.8
Times (UTC)
(P1) Partial begin19:25:17
Greatest eclipse21:17:18
(P4) Partial end23:06:57
References
Saros118 (68 of 72)
Catalog # (SE5000)9532

A partialsolar eclipse occurred at the Moon’sdescending node of orbit on Wednesday, June 1, 2011,[1][2][3][4][5][6][7][8][9] with amagnitude of 0.601. Asolar eclipse occurs when theMoon passes betweenEarth and theSun, thereby totally or partly obscuring the image of the Sun for a viewer on Earth. A partial solar eclipse occurs in the polar regions of the Earth when the center of the Moon's shadow misses the Earth.

This eclipse was the second of four partial solar eclipses in 2011, with the others occurring onJanuary 4,July 1, andNovember 25.

A partial eclipse was visible for parts ofNortheast Asia,Alaska, northernCanada,Greenland, northernScandinavia, andIceland.

Visibility

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Animated path

Gallery

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Eclipse timing

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Places experiencing partial eclipse

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Solar Eclipse of June 1, 2011
(Local Times)
Country or territoryCity or placeStart of partial eclipseMaximum eclipseEnd of partial eclipseDuration of eclipse (hr:min)Maximum coverage
 JapanSapporo[a]04:27:0304:50:2405:14:310:472.94%
 ChinaHarbin[a]03:47:11 (sunrise)04:01:2504:37:210:5012.46%
 ChinaQiqihar[a]03:51:37 (sunrise)04:05:0204:43:140:5215.52%
 ChinaHulunbuir[a]04:00:23 (sunrise)04:09:5904:50:340:5019.69%
 ChinaMohe[a]03:32:1304:13:3204:56:361:2622.15%
 South KoreaSeoul[a]05:12:25 (sunrise)05:13:4505:15:040:030.12%
 North KoreaPyongyang[a]05:13:06 (sunrise)05:16:1305:20:550:080.92%
 RussiaMagadan[a]07:36:3108:17:4409:00:511:2413.71%
 RussiaYakutsk[a]05:39:0506:25:1207:13:151:3426.48%
 MongoliaChoibalsan[a]04:26:12 (sunrise)04:30:0304:52:190:2614.05%
 RussiaAnadyr[a]07:57:5308:36:4409:16:551:197.49%
 FinlandRovaniemi23:41:3400:00:39[b]00:21:23 (sunset)[b]0:4019.26%
 United StatesWainwright12:19:4913:02:3613:46:031:268.94%
 United StatesAtqasuk12:22:2213:04:2913:47:111:258.31%
 United StatesUtqiagvik12:22:2613:05:4913:49:451:279.33%
 RussiaBelushya Guba[a]00:23:3201:13:4502:04:131:4149.55%
 FinlandUtsjoki23:38:3600:28:24[b]01:17:54[b]1:3948.81%
 FinlandIvalo23:39:0300:28:27[b]01:17:33[b]1:3948.92%
 Svalbard and Jan MayenLongyearbyen22:37:3623:29:4900:21:37[b]1:4444.98%
 FinlandKittilä23:41:2000:30:26[b]01:19:09[b]1:3848.57%
 NorwayTromsø22:43:2923:33:1600:22:34[b]1:3947.73%
 SwedenKiruna22:44:0823:33:2000:22:03[b]1:3847.89%
 CanadaAlert16:42:5317:36:0918:28:361:4631.71%
 GreenlandDanmarkshavn20:50:2521:42:3322:33:431:4339.31%
 GreenlandPituffik17:56:4118:48:1219:38:241:4225.88%
 Faroe IslandsTórshavn22:07:4822:48:3422:56:24 (sunset)0:4937.58%
 CanadaPond Inlet17:05:4117:54:4418:42:171:3719.45%
 IcelandReykjavík21:13:3422:01:2622:47:541:3434.63%
 GreenlandNuuk19:26:0920:12:1820:56:391:3121.54%
 CanadaSt. John's19:41:1820:09:2820:36:420:555.08%
References:[1]

Eclipse details

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Shown below are two tables displaying details about this particular solar eclipse. The first table outlines times at which the Moon's penumbra or umbra attains the specific parameter, and the second table describes various other parameters pertaining to this eclipse.[10]

June 1, 2011 Solar Eclipse Times
EventTime (UTC)
First Penumbral External Contact2011 June 01 at 19:26:25.5 UTC
Ecliptic Conjunction2011 June 01 at 21:03:42.9 UTC
Greatest Eclipse2011 June 01 at 21:17:18.4 UTC
Equatorial Conjunction2011 June 01 at 21:23:06.3 UTC
Last Penumbral External Contact2011 June 01 at 23:08:03.6 UTC
June 1, 2011 Solar Eclipse Parameters
ParameterValue
Eclipse Magnitude0.60107
Eclipse Obscuration0.50014
Gamma1.21300
Sun Right Ascension04h37m53.4s
Sun Declination+22°05'47.3"
Sun Semi-Diameter15'46.3"
Sun Equatorial Horizontal Parallax08.7"
Moon Right Ascension04h37m41.0s
Moon Declination+23°13'19.4"
Moon Semi-Diameter15'13.4"
Moon Equatorial Horizontal Parallax0°55'52.1"
ΔT66.4 s

Eclipse season

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See also:Eclipse cycle

This eclipse is part of aneclipse 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 afortnight. The first and last eclipse in this sequence is separated by onesynodic month.

Eclipse season of June–July 2011
June 1
Descending node (new moon)
June 15
Ascending node (full moon)
July 1
Descending node (new moon)
Partial solar eclipse
Solar Saros 118
Total lunar eclipse
Lunar Saros 130
Partial solar eclipse
Solar Saros 156

Related eclipses

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Eclipses in 2011

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Metonic

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Tzolkinex

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Half-Saros

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Tritos

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Solar Saros 118

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Inex

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Triad

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Solar eclipses of 2011–2014

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This eclipse is a member of asemester series. An eclipse in a semester series of solar eclipses repeats approximately every 177 days and 4 hours (a semester) at alternatingnodes of the Moon's orbit.[11]

The partial solar eclipses onJanuary 4, 2011 andJuly 1, 2011 occur in the previous lunar year eclipse set.

Solar eclipse series sets from 2011 to 2014
Descending node Ascending node
SarosMapGammaSarosMapGamma
118

Partial inTromsø,Norway
June 1, 2011

Partial
1.21300123

Hinode XRT footage
November 25, 2011

Partial
−1.05359
128

Annularity inRed Bluff, CA, USA
May 20, 2012

Annular
0.48279133

Totality inMount Carbine,Queensland,Australia
November 13, 2012

Total
−0.37189
138

Annularity inChurchills Head,Australia
May 10, 2013

Annular
−0.26937143

Partial inLibreville,Gabon
November 3, 2013

Hybrid
0.32715
148

Partial inAdelaide,Australia
April 29, 2014

Annular (non-central)
−0.99996153

Partial inMinneapolis, MN, USA
October 23, 2014

Partial
1.09078

Saros 118

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This eclipse is a part ofSaros series 118, repeating every 18 years, 11 days, and containing 72 events. The series started with a partial solar eclipse on May 24, 803 AD. It contains total eclipses from August 19, 947 AD through October 25, 1650; hybrid eclipses on November 4, 1668 and November 15, 1686; and annular eclipses from November 27, 1704 throughApril 30, 1957. The series ends at member 72 as a partial eclipse onJuly 15, 2083. Its eclipses are tabulated in three columns; every third eclipse in the same column is oneexeligmos apart, so they all cast shadows over approximately the same parts of the Earth.

The longest duration of totality was produced by member 34 at 6 minutes, 59 seconds on May 16, 1398, and the longest duration of annularity was produced by member 59 at 1 minutes, 58 seconds on February 23, 1849. All eclipses in this series occur at the Moon’sdescending node of orbit.[12]

Series members 57–72 occur between 1801 and 2083:
575859

February 1, 1813

February 12, 1831

February 23, 1849
606162

March 6, 1867

March 16, 1885

March 29, 1903
636465

April 8, 1921

April 19, 1939

April 30, 1957
666768

May 11, 1975

May 21, 1993

June 1, 2011
697071

June 12, 2029

June 23, 2047

July 3, 2065
72

July 15, 2083

Metonic series

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Themetonic series repeats eclipses every 19 years (6939.69 days), lasting about 5 cycles. Eclipses occur in nearly the same calendar date. In addition, the octon subseries repeats 1/5 of that or every 3.8 years (1387.94 days). All eclipses in this table occur at the Moon's descending node.

22 eclipse events between June 1, 2011 and October 24, 2098
May 31–June 1March 19–20January 5–6October 24–25August 12–13
118120122124126

June 1, 2011

March 20, 2015

January 6, 2019

October 25, 2022

August 12, 2026
128130132134136

June 1, 2030

March 20, 2034

January 5, 2038

October 25, 2041

August 12, 2045
138140142144146

May 31, 2049

March 20, 2053

January 5, 2057

October 24, 2060

August 12, 2064
148150152154156

May 31, 2068

March 19, 2072

January 6, 2076

October 24, 2079

August 13, 2083
158160162164

June 1, 2087

October 24, 2098

Tritos series

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This eclipse is a part of atritos cycle, repeating at alternating nodes every 135synodic months (≈ 3986.63 days, or 11 years minus 1 month). Their appearance and longitude are irregular due to a lack of synchronization with theanomalistic month (period of perigee), but groupings of 3 tritos cycles (≈ 33 years minus 3 months) come close (≈ 434.044 anomalistic months), so eclipses are similar in these groupings.

The partial solar eclipses onApril 8, 1902 (part of Saros 108) andJanuary 5, 1935 (part of Saros 111) are also a part of this series but are not included in the table below.

Series members between 2000 and 2200

July 1, 2000
(Saros 117)

June 1, 2011
(Saros 118)

April 30, 2022
(Saros 119)

March 30, 2033
(Saros 120)

February 28, 2044
(Saros 121)

January 27, 2055
(Saros 122)

December 27, 2065
(Saros 123)

November 26, 2076
(Saros 124)

October 26, 2087
(Saros 125)

September 25, 2098
(Saros 126)

August 26, 2109
(Saros 127)

July 25, 2120
(Saros 128)

June 25, 2131
(Saros 129)

May 25, 2142
(Saros 130)

April 23, 2153
(Saros 131)

March 23, 2164
(Saros 132)

February 21, 2175
(Saros 133)

January 20, 2186
(Saros 134)

December 19, 2196
(Saros 135)

Inex series

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This eclipse is a part of the long periodinex cycle, repeating at alternating nodes, every 358synodic months (≈ 10,571.95 days, or 29 years minus 20 days). Their appearance and longitude are irregular due to a lack of synchronization with theanomalistic month (period of perigee). However, groupings of 3 inex cycles (≈ 87 years minus 2 months) comes close (≈ 1,151.02 anomalistic months), so eclipses are similar in these groupings.

Series members between 1801 and 2200

October 19, 1808
(Saros 111)

August 20, 1895
(Saros 114)

July 31, 1924
(Saros 115)

July 11, 1953
(Saros 116)

June 21, 1982
(Saros 117)

June 1, 2011
(Saros 118)

May 11, 2040
(Saros 119)

April 21, 2069
(Saros 120)

April 1, 2098
(Saros 121)

March 13, 2127
(Saros 122)

February 21, 2156
(Saros 123)

January 31, 2185
(Saros 124)

Notes

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  1. ^abcdefghijklThe times listed for this location occur on June 2, 2011, local time.
  2. ^abcdefghijkThe time listed here for this location occurs on June 2, 2011, local time.

References

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  1. ^ab"June 1, 2011 Partial Solar Eclipse". timeanddate. Retrieved11 August 2024.
  2. ^Malik, Tariq (2011-06-02)."Rare 'Midnight' Partial Solar Eclipse Amazes Northern Skywatchers".Space.com.
  3. ^Peralta, Eyder (2011-06-03)."Stunning: A Solar Eclipse At Midnight".NPR.
  4. ^Fazekas, Andrew (2011-06-02)."Solar Eclipse at Midnight? Sun Smiles on Arctic Tonight".National Geographic. Archived fromthe original on March 3, 2021.
  5. ^Grossman, Lisa (2011-06-03)."Rare Midnight Solar Eclipse Caught in Arctic" – via Wired.
  6. ^"Looking skyward".News-Journal. Mansfield, Ohio. 2011-06-01. p. 2. Retrieved2023-10-18 – via Newspapers.com.
  7. ^"Skywatch data".The Bangor Daily News. Bangor, Maine. 2011-06-01. p. 14. Retrieved2023-10-18 – via Newspapers.com.
  8. ^"Weather Report".Poughkeepsie Journal. Poughkeepsie, New York. 2011-06-01. p. 10. Retrieved2023-10-18 – via Newspapers.com.
  9. ^"Plenty to see even with shorter nights".Kent County News. Chestertown, Maryland. 2011-06-02. p. 7. Retrieved2023-10-18 – via Newspapers.com.
  10. ^"Partial Solar Eclipse of 2011 Jun 01". EclipseWise.com. Retrieved11 August 2024.
  11. ^van Gent, R.H."Solar- and Lunar-Eclipse Predictions from Antiquity to the Present".A Catalogue of Eclipse Cycles. Utrecht University. Retrieved6 October 2018.
  12. ^"NASA - Catalog of Solar Eclipses of Saros 118".eclipse.gsfc.nasa.gov.

External links

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Wikimedia Commons has media related toSolar eclipse of 2011 June 1.
Features
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Saros series (list)
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21 August 2017 total solar eclipse
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23 October 2014 partial eclipse
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