Solar eclipse of June 1, 2076

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Template:Short description Script error: No such module "Solar eclipse". 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

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 1 at 16:11:56.2 UTC
Equatorial Conjunction 2076 June 1 at 16:54:32.2 UTC
Ecliptic Conjunction 2076 June 1 at 17:16:09.9 UTC
Greatest Eclipse 2076 June 1 at 17:31:21.9 UTC
Last Penumbral External Contact 2076 June 1 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

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. 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)
File:SE2076Jun01P.png File:Lunar eclipse chart close-2076Jun17.png File:SE2076Jul01P.png
Partial solar eclipse
Solar Saros 119
Total lunar eclipse
Lunar Saros 131
Partial solar eclipse
Solar Saros 157

Related eclipses

Eclipses in 2076

Metonic

Tzolkinex

Half-Saros

Tritos

Solar Saros 119

Inex

Triad

Solar eclipses of 2076–2079

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
File:SE2076Jun01P.png
Partial
−1.3897 124 November 26, 2076
File:SE2076Nov26P.png
Partial
1.1401
129 May 22, 2077
File:SE2077May22T.png
Total
−0.5725 134 November 15, 2077
File:SE2077Nov15A.png
Annular
0.4705
139 May 11, 2078
File:SE2078May11T.png
Total
0.1838 144 November 4, 2078
File:SE2078Nov04A.png
Annular
−0.2285
149 May 1, 2079
File:SE2079May01T.png
Total
0.9081 154 October 24, 2079
File:SE2079Oct24A.png
Annular
−0.9243

Saros 119

Template:Solar Saros series 119

Metonic series

Template:Solar Metonic series 2076–2163

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 2054 and 2200
File:SE2054Aug03P.png
August 3, 2054
(Saros 117)
File:SE2065Jul03P.png
July 3, 2065
(Saros 118)
File:SE2076Jun01P.png
June 1, 2076
(Saros 119)
File:SE2087May02P.png
May 2, 2087
(Saros 120)
File:SE2098Apr01P.png
April 1, 2098
(Saros 121)
File:SE2109Mar01P.png
March 1, 2109
(Saros 122)
File:Saros123 59van70 SE2120Jan30P.jpg
January 30, 2120
(Saros 123)
File:Saros124 61van73 SE2130Dec30P.jpg
December 30, 2130
(Saros 124)
File:Saros125 61van73 SE2141Nov28P.jpg
November 28, 2141
(Saros 125)
File:Saros126 55van72 SE2152Oct28P.jpg
October 28, 2152
(Saros 126)
File:Saros127 66van82 SE2163Sep28P.jpg
September 28, 2163
(Saros 127)
File:Saros128 67van73 SE2174Aug27P.jpg
August 27, 2174
(Saros 128)
File:Saros129 61van80 SE2185Jul26T.jpg
July 26, 2185
(Saros 129)
File:SE2196Jun26T.png
June 26, 2196
(Saros 130)

Inex series

Template:Solar Inex series 2018 July 13

References

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External links


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