Solar eclipse of July 1, 2076

Last updated
Solar eclipse of July 1, 2076
SE2076Jul01P.png
Map
Type of eclipse
NaturePartial
Gamma 1.4005
Magnitude 0.2746
Maximum eclipse
Coordinates 67°00′N98°06′W / 67°N 98.1°W / 67; -98.1
Times (UTC)
Greatest eclipse6:50:43
References
Saros 157 (2 of 70)
Catalog # (SE5000) 9678

A partial solar eclipse will occur at the Moon's ascending node of orbit on Wednesday, July 1, 2076, [1] with a magnitude of 0.2746. 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.

Contents

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

The partial solar eclipse will be visible for parts of Greenland, northern Canada, Alaska, and the Russian Far East.

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]

July 1, 2076 Solar Eclipse Times
EventTime (UTC)
First Penumbral External Contact2076 July 01 at 05:30:23.1 UTC
Greatest Eclipse2076 July 01 at 06:50:43.3 UTC
Equatorial Conjunction2076 July 01 at 06:53:58.3 UTC
Ecliptic Conjunction2076 July 01 at 07:06:45.0 UTC
Last Penumbral External Contact2076 July 01 at 08:11:05.4 UTC
July 1, 2076 Solar Eclipse Parameters
ParameterValue
Eclipse Magnitude0.27461
Eclipse Obscuration0.16287
Gamma1.40052
Sun Right Ascension06h44m59.8s
Sun Declination+23°01'35.5"
Sun Semi-Diameter15'43.9"
Sun Equatorial Horizontal Parallax08.6"
Moon Right Ascension06h44m53.2s
Moon Declination+24°17'50.8"
Moon Semi-Diameter14'52.7"
Moon Equatorial Horizontal Parallax0°54'36.1"
ΔT102.6 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 June–July 2076
June 1
Ascending node (new moon)
June 17
Descending node (full moon)
July 1
Ascending node (new moon)
SE2076Jun01P.png Lunar eclipse chart close-2076Jun17.png SE2076Jul01P.png
Partial solar eclipse
Solar Saros 119
Total lunar eclipse
Lunar Saros 131
Partial solar eclipse
Solar Saros 157

Eclipses in 2076

Metonic

Tzolkinex

Half-Saros

Tritos

Solar Saros 157

Inex

Triad

Solar eclipses of 2073–2076

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 June 1, 2076 and November 26, 2076 occur in the next lunar year eclipse set.

Solar eclipse series sets from 2073 to 2076
Descending node Ascending node
SarosMapGammaSarosMapGamma
122 February 7, 2073
SE2073Feb07P.png
Partial
1.1651127 August 3, 2073
SE2073Aug03T.png
Total
−0.8763
132 January 27, 2074
SE2074Jan27A.png
Annular
0.4251137 July 24, 2074
SE2074Jul24A.png
Annular
−0.1242
142 January 16, 2075
SE2075Jan16T.png
Total
−0.2799147 July 13, 2075
SE2075Jul13A.png
Annular
0.6583
152 January 6, 2076
SE2076Jan06T.png
Total
−0.9373157 July 1, 2076
SE2076Jul01P.png
Partial
1.4005

Saros 157

This eclipse is a part of Saros series 157, repeating every 18 years, 11 days, and containing 70 events. The series will start with a partial solar eclipse on June 21, 2058. It contains annular eclipses from August 25, 2166 through March 10, 2491; hybrid eclipses from March 22, 2509 through April 12, 2545; and total eclipses from April 24, 2563 through April 21, 3158. The series ends at member 70 as a partial eclipse on July 17, 3302. 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 will be produced by member 15 at 4 minutes, 16 seconds on November 22, 2310, and the longest duration of totality will be produced by member 38 at 5 minutes, 57 seconds on July 31, 2725. All eclipses in this series occur at the Moon’s ascending node of orbit. [4]

Series members 1–8 occur between 2058 and 2200:
123
SE2058Jun21P.png
June 21, 2058
SE2076Jul01P.png
July 1, 2076
SE2094Jul12P.png
July 12, 2094
456
Saros157 04van70 SE2112Jul23P.jpg
July 23, 2112
Saros157 05van70 SE2130Aug04P.jpg
August 4, 2130
Saros157 06van70 SE2148Aug14P.jpg
August 14, 2148
78
Saros157 07van70 SE2166Aug25A.jpg
August 25, 2166
Saros157 08van70 SE2184Sep04A.jpg
September 4, 2184

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 ascending node.

21 eclipse events between July 1, 2000 and July 1, 2076
July 1–2April 19–20February 5–7November 24–25September 12–13
117119121123125
SE2000Jul01P.png
July 1, 2000
SE2004Apr19P.png
April 19, 2004
SE2008Feb07A.png
February 7, 2008
SE2011Nov25P.png
November 25, 2011
SE2015Sep13P.png
September 13, 2015
127129131133135
SE2019Jul02T.png
July 2, 2019
SE2023Apr20H.png
April 20, 2023
SE2027Feb06A.png
February 6, 2027
SE2030Nov25T.png
November 25, 2030
SE2034Sep12A.png
September 12, 2034
137139141143145
SE2038Jul02A.png
July 2, 2038
SE2042Apr20T.png
April 20, 2042
SE2046Feb05A.png
February 5, 2046
SE2049Nov25H.png
November 25, 2049
SE2053Sep12T.png
September 12, 2053
147149151153155
SE2057Jul01A.png
July 1, 2057
SE2061Apr20T.png
April 20, 2061
SE2065Feb05P.png
February 5, 2065
SE2068Nov24P.png
November 24, 2068
SE2072Sep12T.png
September 12, 2072
157
SE2076Jul01P.png
July 1, 2076

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 2087
SE1803Aug17A.png
August 17, 1803
(Saros 132)
SE1814Jul17T.png
July 17, 1814
(Saros 133)
SE1825Jun16H.png
June 16, 1825
(Saros 134)
SE1836May15A.png
May 15, 1836
(Saros 135)
SE1847Apr15T.png
April 15, 1847
(Saros 136)
SE1858Mar15A.png
March 15, 1858
(Saros 137)
SE1869Feb11A.png
February 11, 1869
(Saros 138)
SE1880Jan11T.png
January 11, 1880
(Saros 139)
SE1890Dec12H.png
December 12, 1890
(Saros 140)
SE1901Nov11A.png
November 11, 1901
(Saros 141)
SE1912Oct10T.png
October 10, 1912
(Saros 142)
SE1923Sep10T.png
September 10, 1923
(Saros 143)
SE1934Aug10A.png
August 10, 1934
(Saros 144)
SE1945Jul09T.png
July 9, 1945
(Saros 145)
SE1956Jun08T.png
June 8, 1956
(Saros 146)
SE1967May09P.png
May 9, 1967
(Saros 147)
SE1978Apr07P.png
April 7, 1978
(Saros 148)
SE1989Mar07P.png
March 7, 1989
(Saros 149)
SE2000Feb05P.png
February 5, 2000
(Saros 150)
SE2011Jan04P.png
January 4, 2011
(Saros 151)
SE2021Dec04T.png
December 4, 2021
(Saros 152)
SE2032Nov03P.png
November 3, 2032
(Saros 153)
SE2043Oct03A.png
October 3, 2043
(Saros 154)
SE2054Sep02P.png
September 2, 2054
(Saros 155)
SE2065Aug02P.png
August 2, 2065
(Saros 156)
SE2076Jul01P.png
July 1, 2076
(Saros 157)
SE2087Jun01P.png
June 1, 2087
(Saros 158)

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
SE1815Dec30P.gif
December 30, 1815
(Saros 148)
SE1844Dec09P.gif
December 9, 1844
(Saros 149)
SE1873Nov20P.png
November 20, 1873
(Saros 150)
SE1902Oct31P.png
October 31, 1902
(Saros 151)
SE1931Oct11P.png
October 11, 1931
(Saros 152)
SE1960Sep20P.png
September 20, 1960
(Saros 153)
SE1989Aug31P.png
August 31, 1989
(Saros 154)
SE2018Aug11P.png
August 11, 2018
(Saros 155)
SE2047Jul22P.png
July 22, 2047
(Saros 156)
SE2076Jul01P.png
July 1, 2076
(Saros 157)
Saros158 03van70 SE2105Jun12P.jpg
June 12, 2105
(Saros 158)
Saros159 01van70 SE2134May23P.jpg
May 23, 2134
(Saros 159)
Saros161 02van72 SE2192Apr12P.jpg
April 12, 2192
(Saros 161)

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References

  1. "July 1, 2076 Partial Solar Eclipse". timeanddate. Retrieved 22 August 2024.
  2. "Partial Solar Eclipse of 2076 Jul 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 157". eclipse.gsfc.nasa.gov.