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Solar eclipse of June 1, 2076

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Solar eclipse of June 1, 2076
Map
Type of eclipse
NaturePartial
Gamma−1.3897
Magnitude0.2897
Maximum eclipse
Coordinates64°24′S 51°12′W / 64.4°S 51.2°W / -64.4; -51.2
Times (UTC)
Greatest eclipse17:31:22
References
Saros119 (69 of 71)
Catalog # (SE5000)9679

A partial solar eclipse will occur at the Moon's ascending node of orbit on Monday, June 1, 2076,[1] with a magnitude of 0.2897. 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. A partial solar eclipse occurs in the polar regions of the Earth when the center of the Moon's shadow misses the Earth.

This will be the second of four solar eclipses in 2076, with the others occurring on January 6, July 1, and November 26.

The partial solar eclipse will be visible for parts of southern South America and the Antarctic Peninsula.

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.[2]

June 1, 2076 Solar Eclipse Times
Event Time (UTC)
First Penumbral External Contact 2076 June 01 at 16:11:56.2 UTC
Equatorial Conjunction 2076 June 01 at 16:54:32.2 UTC
Ecliptic Conjunction 2076 June 01 at 17:16:09.9 UTC
Greatest Eclipse 2076 June 01 at 17:31:21.9 UTC
Last Penumbral External Contact 2076 June 01 at 18:51:07.6 UTC
June 1, 2076 Solar Eclipse Parameters
Parameter Value
Eclipse Magnitude 0.28972
Eclipse Obscuration 0.17696
Gamma −1.38966
Sun Right Ascension 04h42m27.8s
Sun Declination +22°14'01.6"
Sun Semi-Diameter 15'46.3"
Sun Equatorial Horizontal Parallax 08.7"
Moon Right Ascension 04h43m42.6s
Moon Declination +20°58'42.6"
Moon Semi-Diameter 15'11.7"
Moon Equatorial Horizontal Parallax 0°55'45.9"
ΔT 102.5 s

Eclipse season

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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 June–July 2076
June 1
Ascending node (new moon)
June 17
Descending node (full moon)
July 1
Ascending node (new moon)
Partial solar eclipse
Solar Saros 119
Total lunar eclipse
Lunar Saros 131
Partial solar eclipse
Solar Saros 157
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Eclipses in 2076

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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 119

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Inex

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Triad

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Solar eclipses of 2076–2079

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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.[3]

The partial solar eclipses on January 6, 2076 and July 1, 2076 occur in the previous lunar year eclipse set.

Solar eclipse series sets from 2076 to 2079
Ascending node   Descending node
Saros Map Gamma Saros Map Gamma
119 June 1, 2076

Partial
−1.3897 124 November 26, 2076

Partial
1.1401
129 May 22, 2077

Total
−0.5725 134 November 15, 2077

Annular
0.4705
139 May 11, 2078

Total
0.1838 144 November 4, 2078

Annular
−0.2285
149 May 1, 2079

Total
0.9081 154 October 24, 2079

Annular
−0.9243

Saros 119

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This eclipse is a part of Saros series 119, repeating every 18 years, 11 days, and containing 71 events. The series started with a partial solar eclipse on May 15, 850 AD. It contains total eclipses on August 9, 994 AD and August 20, 1012; a hybrid eclipse on August 31, 1030; and annular eclipses from September 10, 1048 through March 18, 1950. The series ends at member 71 as a partial eclipse on June 24, 2112. 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 totality was produced by member 10 at 32 seconds on August 20, 1012, and the longest duration of annularity was produced by member 44 at 7 minutes, 37 seconds on September 1, 1625. All eclipses in this series occur at the Moon’s ascending node of orbit.[4]

Metonic series

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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 ascending node.

22 eclipse events between June 1, 2076 and October 27, 2163
June 1–3 March 21–22 January 7–8 October 26–27 August 14–15
119 121 123 125 127

June 1, 2076

March 21, 2080

January 7, 2084

October 26, 2087

August 15, 2091
129 131 133 135 137

June 2, 2095

March 21, 2099

January 8, 2103

October 26, 2106

August 15, 2110
139 141 143 145 147

June 3, 2114

March 22, 2118

January 8, 2122

October 26, 2125

August 15, 2129
149 151 153 155 157

June 3, 2133

March 21, 2137

January 8, 2141

October 26, 2144

August 14, 2148
159 161 163 165

June 3, 2152

October 27, 2163

Tritos series

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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 2054 and 2200

August 3, 2054
(Saros 117)

July 3, 2065
(Saros 118)

June 1, 2076
(Saros 119)

May 2, 2087
(Saros 120)

April 1, 2098
(Saros 121)

March 1, 2109
(Saros 122)

January 30, 2120
(Saros 123)

December 30, 2130
(Saros 124)

November 28, 2141
(Saros 125)

October 28, 2152
(Saros 126)

September 28, 2163
(Saros 127)

August 27, 2174
(Saros 128)

July 26, 2185
(Saros 129)

June 26, 2196
(Saros 130)

Inex series

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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 1844 and 2200

November 10, 1844
(Saros 111)

September 12, 1931
(Saros 114)

July 13, 2018
(Saros 117)

June 23, 2047
(Saros 118)

June 1, 2076
(Saros 119)

May 14, 2105
(Saros 120)

April 24, 2134
(Saros 121)

April 3, 2163
(Saros 122)

March 13, 2192
(Saros 123)

References

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  1. ^ "June 1, 2076 Partial Solar Eclipse". timeanddate. Retrieved 22 August 2024.
  2. ^ "Partial Solar Eclipse of 2076 Jun 01". EclipseWise.com. Retrieved 22 August 2024.
  3. ^ 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.
  4. ^ "NASA - Catalog of Solar Eclipses of Saros 119". eclipse.gsfc.nasa.gov.
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