Solar eclipse of June 11, 2067

Last updated
Solar eclipse of June 11, 2067
SE2067Jun11A.png
Map
Type of eclipse
NatureAnnular
Gamma −0.0387
Magnitude 0.967
Maximum eclipse
Duration245 s (4 min 5 s)
Coordinates 21°00′N130°12′W / 21°N 130.2°W / 21; -130.2
Max. width of band119 km (74 mi)
Times (UTC)
Greatest eclipse20:42:26
References
Saros 138 (34 of 70)
Catalog # (SE5000) 9658

An annular solar eclipse will occur at the Moon's descending node of orbit on Saturday, June 11, 2067, [1] with a magnitude of 0.967. A solar eclipse occurs when the Moon passes between Earth and the Sun, thereby totally or partly obscuring the image of the Sun for a viewer on Earth. An annular solar eclipse occurs when the Moon's apparent diameter is smaller than the Sun's, blocking most of the Sun's light and causing the Sun to look like an annulus (ring). An annular eclipse appears as a partial eclipse over a region of the Earth thousands of kilometres wide. Occurring about 4.3 days before apogee (on June 16, 2067, at 4:05 UTC), the Moon's apparent diameter will be smaller. [2]

Contents

The path of annularity will be visible from parts of Kiribati, Ecuador, northern Peru, extreme southern Colombia, and extreme western Brazil. A partial solar eclipse will also be visible for parts of Oceania, Hawaii, southern North America, Central America, the Caribbean, and western South America.

Eclipse details

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. [3]

June 11, 2067 Solar Eclipse Times
EventTime (UTC)
First Penumbral External Contact2067 June 11 at 17:41:42.1 UTC
First Umbral External Contact2067 June 11 at 18:45:02.0 UTC
First Central Line2067 June 11 at 18:46:37.3 UTC
First Umbral Internal Contact2067 June 11 at 18:48:12.5 UTC
First Penumbral Internal Contact2067 June 11 at 19:51:38.7 UTC
Greatest Eclipse2067 June 11 at 20:42:26.4 UTC
Equatorial Conjunction2067 June 11 at 20:42:35.2 UTC
Ecliptic Conjunction2067 June 11 at 20:42:53.4 UTC
Greatest Duration2067 June 11 at 20:43:57.1 UTC
Last Penumbral Internal Contact2067 June 11 at 21:33:13.1 UTC
Last Umbral Internal Contact2067 June 11 at 22:36:38.6 UTC
Last Central Line2067 June 11 at 22:38:16.2 UTC
Last Umbral External Contact2067 June 11 at 22:39:53.8 UTC
Last Penumbral External Contact2067 June 11 at 23:43:15.9 UTC
June 11, 2067 Solar Eclipse Parameters
ParameterValue
Eclipse Magnitude0.96702
Eclipse Obscuration0.93513
Gamma−0.03865
Sun Right Ascension05h20m58.3s
Sun Declination+23°07'36.6"
Sun Semi-Diameter15'45.1"
Sun Equatorial Horizontal Parallax08.7"
Moon Right Ascension05h20m58.0s
Moon Declination+23°05'29.3"
Moon Semi-Diameter15'00.0"
Moon Equatorial Horizontal Parallax0°55'03.2"
ΔT95.6 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. The first and last eclipse in this sequence is separated by one synodic month.

Eclipse season of May–June 2067
May 28
Ascending node (full moon)
 June 11
Descending node (new moon)
 June 27
Ascending node (full moon)
Lunar eclipse chart close-2067May28.png SE2067Jun11A.png
Penumbral lunar eclipse
Lunar Saros 112		 Annular solar eclipse
Solar Saros 138		 Penumbral lunar eclipse
Lunar Saros 150

Eclipses in 2067

Metonic

Tzolkinex

Half-Saros

Tritos

Solar Saros 138

Inex

Triad

Solar eclipses of 2065–2069

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

The partial solar eclipses on February 5, 2065 and August 2, 2065 occur in the previous lunar year eclipse set, and the partial solar eclipses on April 21, 2069 and October 15, 2069 occur in the next lunar year eclipse set.

Solar eclipse series sets from 2065 to 2069
Descending node Ascending node
SarosMapGammaSarosMapGamma
118 July 3, 2065
SE2065Jul03P.png
Partial		1.4619123 December 27, 2065
SE2065Dec27P.png
Partial		−1.0688
128 June 22, 2066
SE2066Jun22A.png
Annular		0.733133 December 17, 2066
SE2066Dec17T.png
Total		−0.4043
138 June 11, 2067
SE2067Jun11A.png
Annular		−0.0387143 December 6, 2067
SE2067Dec06H.png
Hybrid		0.2845
148 May 31, 2068
SE2068May31T.png
Total		−0.797153 November 24, 2068
SE2068Nov24P.png
Partial		1.0299
158 May 20, 2069
SE2069May20P.png
Partial		−1.4852

Saros 138

This eclipse is a part of Saros series 138, repeating every 18 years, 11 days, and containing 70 events. The series started with a partial solar eclipse on June 6, 1472. It contains annular eclipses from August 31, 1598 through February 18, 2482; a hybrid eclipse on March 1, 2500; and total eclipses from March 12, 2518 through April 3, 2554. The series ends at member 70 as a partial eclipse on July 11, 2716. Its 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.

The longest duration of annularity was produced by member 23 at 8 minutes, 2 seconds on February 11, 1869, and the longest duration of totality will be produced by member 61 at 56 seconds on April 3, 2554. All eclipses in this series occur at the Moon’s descending node of orbit. [5]

Series members 20–41 occur between 1801 and 2200:
202122
SE1815Jan10A.png
January 10, 1815		 SE1833Jan20A.png
January 20, 1833		 SE1851Feb01A.png
February 1, 1851
232425
SE1869Feb11A.png
February 11, 1869		 SE1887Feb22A.png
February 22, 1887		 SE1905Mar06A.png
March 6, 1905
262728
SE1923Mar17A.png
March 17, 1923 		SE1941Mar27A.png
March 27, 1941 		SE1959Apr08A.png
April 8, 1959
293031
SE1977Apr18A.png
April 18, 1977 		SE1995Apr29A.png
April 29, 1995 		SE2013May10A.png
May 10, 2013
323334
SE2031May21A.png
May 21, 2031 		SE2049May31A.png
May 31, 2049 		SE2067Jun11A.png
June 11, 2067
353637
SE2085Jun22A.png
June 22, 2085 		SE2103Jul04A.png
July 4, 2103		 SE2121Jul14A.png
July 14, 2121
383940
SE2139Jul25A.png
July 25, 2139		 SE2157Aug05A.png
August 5, 2157		 SE2175Aug16A.png
August 16, 2175
41
SE2193Aug26A.png
August 26, 2193

Metonic series

The metonic 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 12, 2029 and November 4, 2116
June 11–12March 30–31January 16November 4–5August 23–24
118120122124126
SE2029Jun12P.png
June 12, 2029 		SE2033Mar30T.png
March 30, 2033 		SE2037Jan16P.png
January 16, 2037 		SE2040Nov04P.png
November 4, 2040 		SE2044Aug23T.png
August 23, 2044
128130132134136
SE2048Jun11A.png
June 11, 2048 		SE2052Mar30T.png
March 30, 2052 		SE2056Jan16A.png
January 16, 2056 		SE2059Nov05A.png
November 5, 2059 		SE2063Aug24T.png
August 24, 2063
138140142144146
SE2067Jun11A.png
June 11, 2067 		SE2071Mar31A.png
March 31, 2071 		SE2075Jan16T.png
January 16, 2075 		SE2078Nov04A.png
November 4, 2078 		SE2082Aug24T.png
August 24, 2082
148150152154156
SE2086Jun11T.png
June 11, 2086 		SE2090Mar31P.png
March 31, 2090 		SE2094Jan16T.png
January 16, 2094 		SE2097Nov04A.png
November 4, 2097 		Saros156 06van69 SE2101Aug24P.jpg
August 24, 2101
158160162164
Saros158 03van70 SE2105Jun12P.jpg
June 12, 2105		 Saros164 02van80 SE2116Nov04P.jpg
November 4, 2116

Tritos series

This eclipse is a part of a tritos cycle, repeating at alternating nodes every 135 synodic months (≈ 3986.63 days, or 11 years minus 1 month). Their appearance and longitude are irregular due to a lack of synchronization with the anomalistic 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.

Series members between 1801 and 2200
SE1805Jun26P.gif
June 26, 1805
(Saros 114)		 SE1816May27A.gif
May 27, 1816
(Saros 115)		 SE1827Apr26A.gif
April 26, 1827
(Saros 116)		 SE1838Mar25T.gif
March 25, 1838
(Saros 117)		 SE1849Feb23A.gif
February 23, 1849
(Saros 118)
SE1860Jan23A.png
January 23, 1860
(Saros 119)		 SE1870Dec22T.png
December 22, 1870
(Saros 120)		 SE1881Nov21A.gif
November 21, 1881
(Saros 121)		 SE1892Oct20P.gif
October 20, 1892
(Saros 122)		 SE1903Sep21T.png
September 21, 1903
(Saros 123)
SE1914Aug21T.png
August 21, 1914
(Saros 124)		 SE1925Jul20A.png
July 20, 1925
(Saros 125)		 SE1936Jun19T.png
June 19, 1936
(Saros 126)		 SE1947May20T.png
May 20, 1947
(Saros 127)		 SE1958Apr19A.png
April 19, 1958
(Saros 128)
SE1969Mar18A.png
March 18, 1969
(Saros 129)		 SE1980Feb16T.png
February 16, 1980
(Saros 130)		 SE1991Jan15A.png
January 15, 1991
(Saros 131)		 SE2001Dec14A.png
December 14, 2001
(Saros 132)		 SE2012Nov13T.png
November 13, 2012
(Saros 133)
SE2023Oct14A.png
October 14, 2023
(Saros 134)		 SE2034Sep12A.png
September 12, 2034
(Saros 135)		 SE2045Aug12T.png
August 12, 2045
(Saros 136)		 SE2056Jul12A.png
July 12, 2056
(Saros 137)		 SE2067Jun11A.png
June 11, 2067
(Saros 138)
SE2078May11T.png
May 11, 2078
(Saros 139)		 SE2089Apr10A.png
April 10, 2089
(Saros 140)		 SE2100Mar10A.png
March 10, 2100
(Saros 141)		 SE2111Feb08T.png
February 8, 2111
(Saros 142)		 SE2122Jan08A.png
January 8, 2122
(Saros 143)
SE2132Dec07A.png
December 7, 2132
(Saros 144)		 SE2143Nov07T.png
November 7, 2143
(Saros 145)		 SE2154Oct07T.png
October 7, 2154
(Saros 146)		 Saros147 31van80 SE2165Sep05A.jpg
September 5, 2165
(Saros 147)		 Saros148 30van75 SE2176Aug04T.jpg
August 4, 2176
(Saros 148)
Saros149 30van71 SE2187Jul06T.jpg
July 6, 2187
(Saros 149)		 Saros150 27van71 SE2198Jun04A.jpg
June 4, 2198
(Saros 150)

Inex series

This eclipse is a part of the long period inex cycle, repeating at alternating nodes, every 358 synodic months (≈ 10,571.95 days, or 29 years minus 20 days). Their appearance and longitude are irregular due to a lack of synchronization with the anomalistic 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
SE1806Dec10A.gif
December 10, 1806
(Saros 129)		 SE1835Nov20T.gif
November 20, 1835
(Saros 130)		 SE1864Oct30A.gif
October 30, 1864
(Saros 131)
SE1893Oct09A.png
October 9, 1893
(Saros 132)		 SE1922Sep21T.png
September 21, 1922
(Saros 133)		 SE1951Sep01A.png
September 1, 1951
(Saros 134)
SE1980Aug10A.png
August 10, 1980
(Saros 135)		 SE2009Jul22T.png
July 22, 2009
(Saros 136)		 SE2038Jul02A.png
July 2, 2038
(Saros 137)
SE2067Jun11A.png
June 11, 2067
(Saros 138)		 SE2096May22T.png
May 22, 2096
(Saros 139)		 SE2125May03A.png
May 3, 2125
(Saros 140)
SE2154Apr12A.png
April 12, 2154
(Saros 141)		 SE2183Mar23T.png
March 23, 2183
(Saros 142)

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<span class="mw-page-title-main">Solar eclipse of July 9, 1926</span> 20th-century annular solar eclipse

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References

  1. ↑ "June 11, 2067 Annular Solar Eclipse". timeanddate. Retrieved 19 August 2024.
  2. ↑ "Moon Distances for London, United Kingdom, England". timeanddate. Retrieved 19 August 2024.
  3. ↑ "Annular Solar Eclipse of 2067 Jun 11". EclipseWise.com. Retrieved 19 August 2024.
  4. ↑ 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.
  5. ↑ "NASA - Catalog of Solar Eclipses of Saros 138". eclipse.gsfc.nasa.gov.
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