Solar eclipse of July 24, 2074

Last updated
Solar eclipse of July 24, 2074
SE2074Jul24A.png
Map
Type of eclipse
NatureAnnular
Gamma −0.1242
Magnitude 0.9838
Maximum eclipse
Duration117 s (1 min 57 s)
Coordinates 12°48′N133°42′E / 12.8°N 133.7°E / 12.8; 133.7
Max. width of band58 km (36 mi)
Times (UTC)
Greatest eclipse3:10:32
References
Saros 137 (39 of 70)
Catalog # (SE5000) 9674

An annular solar eclipse will occur at the Moon's ascending node of orbit on Tuesday, July 24, 2074, with a magnitude of 0.9838. 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.

Contents

Eclipses in 2074

Metonic

Tzolkinex

Half-Saros

Tritos

Solar Saros 137

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. [1]

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 137

This eclipse is a part of Saros series 137, repeating every 18 years, 11 days, and containing 70 events. The series started with a partial solar eclipse on May 25, 1389. It contains total eclipses from August 20, 1533 through December 6, 1695; the first set of hybrid eclipses from December 17, 1713 through February 11, 1804; the first set of annular eclipses from February 21, 1822 through March 25, 1876; the second set of hybrid eclipses from April 6, 1894 through April 28, 1930; and the second set of annular eclipses from May 9, 1948 through April 13, 2507. The series ends at member 70 as a partial eclipse on June 28, 2633. 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 11 at 2 minutes, 55 seconds on September 10, 1569, and the longest duration of annularity will be produced by member 59 at 7 minutes, 5 seconds on February 28, 2435. All eclipses in this series occur at the Moon’s ascending node of orbit. [2]

Series members 24–46 occur between 1801 and 2200:
242526
SE1804Feb11H.png
February 11, 1804
SE1822Feb21A.png
February 21, 1822
SE1840Mar04A.png
March 4, 1840
272829
SE1858Mar15A.png
March 15, 1858
SE1876Mar25A.png
March 25, 1876
SE1894Apr06H.png
April 6, 1894
303132
SE1912Apr17H.png
April 17, 1912
SE1930Apr28H.png
April 28, 1930
SE1948May09A.png
May 9, 1948
333435
SE1966May20A.png
May 20, 1966
SE1984May30A.png
May 30, 1984
SE2002Jun10A.png
June 10, 2002
363738
SE2020Jun21A.png
June 21, 2020
SE2038Jul02A.png
July 2, 2038
SE2056Jul12A.png
July 12, 2056
394041
SE2074Jul24A.png
July 24, 2074
SE2092Aug03A.png
August 3, 2092
SE2110Aug15A.png
August 15, 2110
424344
SE2128Aug25A.png
August 25, 2128
SE2146Sep06A.png
September 6, 2146
SE2164Sep16A.png
September 16, 2164
4546
SE2182Sep27A.png
September 27, 2182
SE2200Oct09A.png
October 9, 2200

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
SE1801Sep08P.png
September 8, 1801
(Saros 112)
SE1812Aug07P.gif
August 7, 1812
(Saros 113)
SE1823Jul08P.gif
July 8, 1823
(Saros 114)
SE1834Jun07P.gif
June 7, 1834
(Saros 115)
SE1845May06An.gif
May 6, 1845
(Saros 116)
SE1856Apr05T.gif
April 5, 1856
(Saros 117)
SE1867Mar06A.gif
March 6, 1867
(Saros 118)
SE1878Feb02A.gif
February 2, 1878
(Saros 119)
SE1889Jan01T.png
January 1, 1889
(Saros 120)
SE1899Dec03A.png
December 3, 1899
(Saros 121)
SE1910Nov02P.png
November 2, 1910
(Saros 122)
SE1921Oct01T.png
October 1, 1921
(Saros 123)
SE1932Aug31T.png
August 31, 1932
(Saros 124)
SE1943Aug01A.png
August 1, 1943
(Saros 125)
SE1954Jun30T.png
June 30, 1954
(Saros 126)
SE1965May30T.png
May 30, 1965
(Saros 127)
SE1976Apr29A.png
April 29, 1976
(Saros 128)
SE1987Mar29H.png
March 29, 1987
(Saros 129)
SE1998Feb26T.png
February 26, 1998
(Saros 130)
SE2009Jan26A.png
January 26, 2009
(Saros 131)
SE2019Dec26A.png
December 26, 2019
(Saros 132)
SE2030Nov25T.png
November 25, 2030
(Saros 133)
SE2041Oct25A.png
October 25, 2041
(Saros 134)
SE2052Sep22A.png
September 22, 2052
(Saros 135)
SE2063Aug24T.png
August 24, 2063
(Saros 136)
SE2074Jul24A.png
July 24, 2074
(Saros 137)
SE2085Jun22A.png
June 22, 2085
(Saros 138)
SE2096May22T.png
May 22, 2096
(Saros 139)
SE2107Apr23A.png
April 23, 2107
(Saros 140)
SE2118Mar22A.png
March 22, 2118
(Saros 141)
SE2129Feb18T.png
February 18, 2129
(Saros 142)
SE2140Jan20A.png
January 20, 2140
(Saros 143)
SE2150Dec19A.png
December 19, 2150
(Saros 144)
SE2161Nov17T.png
November 17, 2161
(Saros 145)
SE2172Oct17H.png
October 17, 2172
(Saros 146)
Saros147 32van80 SE2183Sep16A.jpg
September 16, 2183
(Saros 147)
Saros148 31van75 SE2194Aug16T.jpg
August 16, 2194
(Saros 148)

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 23, 2036 and July 23, 2112
July 23–24May 11February 27–28December 16–17October 4–5
117119121123125
SE2036Jul23P.png
July 23, 2036
SE2040May11P.png
May 11, 2040
SE2044Feb28A.png
February 28, 2044
SE2047Dec16P.png
December 16, 2047
SE2051Oct04P.png
October 4, 2051
127129131133135
SE2055Jul24T.png
July 24, 2055
SE2059May11T.png
May 11, 2059
SE2063Feb28A.png
February 28, 2063
SE2066Dec17T.png
December 17, 2066
SE2070Oct04A.png
October 4, 2070
137139141143145
SE2074Jul24A.png
July 24, 2074
SE2078May11T.png
May 11, 2078
SE2082Feb27A.png
February 27, 2082
SE2085Dec16A.png
December 16, 2085
SE2089Oct04T.png
October 4, 2089
147149151153155
SE2093Jul23A.png
July 23, 2093
SE2097May11T.png
May 11, 2097
SE2101Feb28A.png
February 28, 2101
Saros153 14van70 SE2104Dec17A.jpg
December 17, 2104
Saros155 11van71 SE2108Oct05T.jpg
October 5, 2108
157
Saros157 04van70 SE2112Jul23P.jpg
July 23, 2112

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References

  1. 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.
  2. "NASA - Catalog of Solar Eclipses of Saros 137". eclipse.gsfc.nasa.gov.