Solar eclipse of August 3, 2092

Last updated
Solar eclipse of August 3, 2092
SE2092Aug03A.png
Map
Type of eclipse
NatureAnnular
Gamma −0.2044
Magnitude 0.9794
Maximum eclipse
Duration151 s (2 min 31 s)
Coordinates 5°36′N30°18′E / 5.6°N 30.3°E / 5.6; 30.3
Max. width of band75 km (47 mi)
Times (UTC)
Greatest eclipse9:59:33
References
Saros 137 (40 of 70)
Catalog # (SE5000) 9715

An annular solar eclipse will occur at the Moon's ascending node of orbit on Sunday, August 3, 2092, [1] with a magnitude of 0.9794. 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 kilometers wide. Occurring about 5.3 days after apogee (on July 29, 2092, at 2:00 UTC), the Moon's apparent diameter will be smaller. [2]

Contents

The path of annularity will be visible from parts of Liberia, Côte d'Ivoire, Ghana, Togo, Benin, Nigeria, Cameroon, Chad, the Central African Republic, South Sudan, Uganda, Kenya, Somalia, and the Seychelles. A partial solar eclipse will also be visible for parts of eastern Brazil, Africa, Southern Europe, the Middle East, and South Asia.

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]

August 3, 2092 Solar Eclipse Times
EventTime (UTC)
First Penumbral External Contact2092 August 03 at 07:03:23.5 UTC
First Umbral External Contact2092 August 03 at 08:06:36.3 UTC
First Central Line2092 August 03 at 08:07:48.9 UTC
First Umbral Internal Contact2092 August 03 at 08:09:01.6 UTC
First Penumbral Internal Contact2092 August 03 at 09:14:39.6 UTC
Greatest Duration2092 August 03 at 09:18:10.6 UTC
Ecliptic Conjunction2092 August 03 at 09:57:12.6 UTC
Greatest Eclipse2092 August 03 at 09:59:32.8 UTC
Equatorial Conjunction2092 August 03 at 10:03:51.7 UTC
Last Penumbral Internal Contact2092 August 03 at 10:44:20.1 UTC
Last Umbral Internal Contact2092 August 03 at 11:50:02.9 UTC
Last Central Line2092 August 03 at 11:51:12.9 UTC
Last Umbral External Contact2092 August 03 at 11:52:22.8 UTC
Last Penumbral External Contact2092 August 03 at 12:55:34.2 UTC
August 3, 2092 Solar Eclipse Parameters
ParameterValue
Eclipse Magnitude0.97942
Eclipse Obscuration0.95927
Gamma−0.20443
Sun Right Ascension08h58m14.3s
Sun Declination+17°09'21.7"
Sun Semi-Diameter15'45.7"
Sun Equatorial Horizontal Parallax08.7"
Moon Right Ascension08h58m05.6s
Moon Declination+16°58'10.4"
Moon Semi-Diameter15'12.2"
Moon Equatorial Horizontal Parallax0°55'47.9"
ΔT116.5 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 July–August 2092
July 19
Descending node (full moon)
August 3
Ascending node (new moon)
August 17
Descending node (full moon)
SE2092Aug03A.png
Penumbral lunar eclipse
Lunar Saros 111
Annular solar eclipse
Solar Saros 137
Penumbral lunar eclipse
Lunar Saros 149

Eclipses in 2092

Metonic

Tzolkinex

Half-Saros

Tritos

Solar Saros 137

Inex

Triad

Solar eclipses of 2091–2094

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 June 13, 2094 and December 7, 2094 occur in the next lunar year eclipse set.

Solar eclipse series sets from 2091 to 2094
Descending node Ascending node
SarosMapGammaSarosMapGamma
122 February 18, 2091
SE2091Feb18P.png
Partial
1.1779127 August 15, 2091
SE2091Aug15T.png
Total
−0.949
132 February 7, 2092
SE2092Feb07A.png
Annular
0.4322137 August 3, 2092
SE2092Aug03A.png
Annular
−0.2044
142 January 27, 2093
SE2093Jan27T.png
Total
−0.2737147 July 23, 2093
SE2093Jul23A.png
Annular
0.5717
152 January 16, 2094
SE2094Jan16T.png
Total
−0.9333157 July 12, 2094
SE2094Jul12P.png
Partial
1.3150

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. [5]

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

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.

23 eclipse events between August 3, 2054 and October 16, 2145
August 3–4May 22–24March 10–11December 27–29October 14–16
117119121123125
SE2054Aug03P.png
August 3, 2054
SE2058May22P.png
May 22, 2058
SE2062Mar11P.png
March 11, 2062
SE2065Dec27P.png
December 27, 2065
SE2069Oct15P.png
October 15, 2069
127129131133135
SE2073Aug03T.png
August 3, 2073
SE2077May22T.png
May 22, 2077
SE2081Mar10A.png
March 10, 2081
SE2084Dec27T.png
December 27, 2084
SE2088Oct14A.png
October 14, 2088
137139141143145
SE2092Aug03A.png
August 3, 2092
SE2096May22T.png
May 22, 2096
SE2100Mar10A.png
March 10, 2100
SE2103Dec29A.png
December 29, 2103
SE2107Oct16T.png
October 16, 2107
147149151153155
SE2111Aug04A.png
August 4, 2111
SE2115May24T.png
May 24, 2115
Saros151 20van72 SE2119Mar11A.jpg
March 11, 2119
Saros153 15van70 SE2122Dec28A.jpg
December 28, 2122
SE2126Oct16T.png
October 16, 2126
157159161163165
Saros157 05van70 SE2130Aug04P.jpg
August 4, 2130
Saros159 01van70 SE2134May23P.jpg
May 23, 2134
Saros165 01van72 SE2145Oct16P.jpg
October 16, 2145

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
SE1808Oct19P.gif
October 19, 1808
(Saros 111)
SE1819Sep19Pe.gif
September 19, 1819
(Saros 112)
SE1830Aug18P.gif
August 18, 1830
(Saros 113)
SE1841Jul18P.gif
July 18, 1841
(Saros 114)
SE1852Jun17P.gif
June 17, 1852
(Saros 115)
SE1863May17P.gif
May 17, 1863
(Saros 116)
SE1874Apr16T.png
April 16, 1874
(Saros 117)
SE1885Mar16A.gif
March 16, 1885
(Saros 118)
SE1896Feb13A.png
February 13, 1896
(Saros 119)
SE1907Jan14T.png
January 14, 1907
(Saros 120)
SE1917Dec14A.png
December 14, 1917
(Saros 121)
SE1928Nov12P.png
November 12, 1928
(Saros 122)
SE1939Oct12T.png
October 12, 1939
(Saros 123)
SE1950Sep12T.png
September 12, 1950
(Saros 124)
SE1961Aug11A.png
August 11, 1961
(Saros 125)
SE1972Jul10T.png
July 10, 1972
(Saros 126)
SE1983Jun11T.png
June 11, 1983
(Saros 127)
SE1994May10A.png
May 10, 1994
(Saros 128)
SE2005Apr08H.png
April 8, 2005
(Saros 129)
SE2016Mar09T.png
March 9, 2016
(Saros 130)
SE2027Feb06A.png
February 6, 2027
(Saros 131)
SE2038Jan05A.png
January 5, 2038
(Saros 132)
SE2048Dec05T.png
December 5, 2048
(Saros 133)
SE2059Nov05A.png
November 5, 2059
(Saros 134)
SE2070Oct04A.png
October 4, 2070
(Saros 135)
SE2081Sep03T.png
September 3, 2081
(Saros 136)
SE2092Aug03A.png
August 3, 2092
(Saros 137)
SE2103Jul04A.png
July 4, 2103
(Saros 138)
SE2114Jun03T.png
June 3, 2114
(Saros 139)
SE2125May03A.png
May 3, 2125
(Saros 140)
SE2136Apr01A.png
April 1, 2136
(Saros 141)
SE2147Mar02T.png
March 2, 2147
(Saros 142)
SE2158Jan30A.png
January 30, 2158
(Saros 143)
SE2168Dec29A.png
December 29, 2168
(Saros 144)
SE2179Nov28T.png
November 28, 2179
(Saros 145)
SE2190Oct29H.png
October 29, 2190
(Saros 146)

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
SE1803Feb21T.png
February 21, 1803
(Saros 127)
SE1832Feb01A.gif
February 1, 1832
(Saros 128)
SE1861Jan11A.gif
January 11, 1861
(Saros 129)
SE1889Dec22T.png
December 22, 1889
(Saros 130)
SE1918Dec03A.png
December 3, 1918
(Saros 131)
SE1947Nov12A.png
November 12, 1947
(Saros 132)
SE1976Oct23T.png
October 23, 1976
(Saros 133)
SE2005Oct03A.png
October 3, 2005
(Saros 134)
SE2034Sep12A.png
September 12, 2034
(Saros 135)
SE2063Aug24T.png
August 24, 2063
(Saros 136)
SE2092Aug03A.png
August 3, 2092
(Saros 137)
SE2121Jul14A.png
July 14, 2121
(Saros 138)
SE2150Jun25T.png
June 25, 2150
(Saros 139)
SE2179Jun05A.png
June 5, 2179
(Saros 140)

Notes

  1. "August 3, 2092 Annular Solar Eclipse". timeanddate. Retrieved 24 August 2024.
  2. "Moon Distances for London, United Kingdom, England". timeanddate. Retrieved 24 August 2024.
  3. "Annular Solar Eclipse of 2092 Aug 03". EclipseWise.com. Retrieved 24 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 137". eclipse.gsfc.nasa.gov.

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References