Solar eclipse of November 16, 2058

Last updated
Solar eclipse of November 16, 2058
SE2058Nov16P.png
Map
Type of eclipse
NaturePartial
Gamma 1.1224
Magnitude 0.7644
Maximum eclipse
Coordinates 62°54′N174°12′E / 62.9°N 174.2°E / 62.9; 174.2
Times (UTC)
Greatest eclipse3:23:07
References
Saros 124 (57 of 73)
Catalog # (SE5000) 9639

A partial solar eclipse will occur at the Moon's descending node of orbit on Saturday, November 16, 2058, [1] with a magnitude of 0.7644. 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

The partial solar eclipse will be visible for parts of Northeast 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. [2]

November 16, 2058 Solar Eclipse Times
EventTime (UTC)
First Penumbral External Contact2058 November 16 at 01:25:37.0 UTC
Equatorial Conjunction2058 November 16 at 02:38:28.2 UTC
Ecliptic Conjunction2058 November 16 at 03:10:59.7 UTC
Greatest Eclipse2058 November 16 at 03:23:07.3 UTC
Last Penumbral External Contact2058 November 16 at 05:20:50.7 UTC
November 16, 2058 Solar Eclipse Parameters
ParameterValue
Eclipse Magnitude0.76445
Eclipse Obscuration0.69696
Gamma1.12238
Sun Right Ascension15h26m32.8s
Sun Declination-18°46'09.8"
Sun Semi-Diameter16'10.2"
Sun Equatorial Horizontal Parallax08.9"
Moon Right Ascension15h28m05.5s
Moon Declination-17°45'10.1"
Moon Semi-Diameter15'47.0"
Moon Equatorial Horizontal Parallax0°57'55.4"
ΔT89.7 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.

Eclipse season of November 2058
November 16
Descending node (new moon)
November 30
Ascending node (full moon)
SE2058Nov16P.png Lunar eclipse chart close-2058Nov30.png
Partial solar eclipse
Solar Saros 124
Total lunar eclipse
Lunar Saros 136

Eclipses in 2058

Metonic

Tzolkinex

Half-Saros

Tritos

Solar Saros 124

Inex

Triad

Solar eclipses of 2058–2061

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 eclipse on June 21, 2058 occurs in the previous lunar year eclipse set.

Solar eclipse series sets from 2058 to 2061
Ascending node Descending node
SarosMapGammaSarosMapGamma
119 May 22, 2058
SE2058May22P.png
Partial
−1.3194124 November 16, 2058
SE2058Nov16P.png
Partial
1.1224
129 May 11, 2059
SE2059May11T.png
Total
−0.508134 November 5, 2059
SE2059Nov05A.png
Annular
0.4454
139 April 30, 2060
SE2060Apr30T.png
Total
0.2422144 October 24, 2060
SE2060Oct24A.png
Annular
−0.2625
149 April 20, 2061
SE2061Apr20T.png
Total
0.9578154 October 13, 2061
SE2061Oct13A.png
Annular
−0.9639

Saros 124

This eclipse is a part of Saros series 124, repeating every 18 years, 11 days, and containing 73 events. The series started with a partial solar eclipse on March 6, 1049. It contains total eclipses from June 12, 1211 through September 22, 1968, and a hybrid eclipse on October 3, 1986. There are no annular eclipses in this set. The series ends at member 73 as a partial eclipse on May 11, 2347. 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 39 at 5 minutes, 46 seconds on May 3, 1734. All eclipses in this series occur at the Moon’s descending node of orbit. [4]

Series members 43–64 occur between 1801 and 2200:
434445
SE1806Jun16T.png
June 16, 1806
SE1824Jun26T.png
June 26, 1824
SE1842Jul08T.png
July 8, 1842
464748
SE1860Jul18T.png
July 18, 1860
SE1878Jul29T.png
July 29, 1878
SE1896Aug09T.png
August 9, 1896
495051
SE1914Aug21T.png
August 21, 1914
SE1932Aug31T.png
August 31, 1932
SE1950Sep12T.png
September 12, 1950
525354
SE1968Sep22T.png
September 22, 1968
SE1986Oct03H.png
October 3, 1986
SE2004Oct14P.png
October 14, 2004
555657
SE2022Oct25P.png
October 25, 2022
SE2040Nov04P.png
November 4, 2040
SE2058Nov16P.png
November 16, 2058
585960
SE2076Nov26P.png
November 26, 2076
SE2094Dec07P.png
December 7, 2094
Saros124 60van73 SE2112Dec19P.jpg
December 19, 2112
616263
Saros124 61van73 SE2130Dec30P.jpg
December 30, 2130
Saros124 62van73 SE2149Jan09P.jpg
January 9, 2149
Saros124 63van73 SE2167Jan21P.jpg
January 21, 2167
64
Saros124 64van73 SE2185Jan31P.jpg
January 31, 2185

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 descending node.

22 eclipse events between June 23, 2047 and November 16, 2134
June 22–23April 10–11January 27–29November 15–16September 3–5
118120122124126
SE2047Jun23P.png
June 23, 2047
SE2051Apr11P.png
April 11, 2051
SE2055Jan27P.png
January 27, 2055
SE2058Nov16P.png
November 16, 2058
SE2062Sep03P.png
September 3, 2062
128130132134136
SE2066Jun22A.png
June 22, 2066
SE2070Apr11T.png
April 11, 2070
SE2074Jan27A.png
January 27, 2074
SE2077Nov15A.png
November 15, 2077
SE2081Sep03T.png
September 3, 2081
138140142144146
SE2085Jun22A.png
June 22, 2085
SE2089Apr10A.png
April 10, 2089
SE2093Jan27T.png
January 27, 2093
SE2096Nov15A.png
November 15, 2096
SE2100Sep04T.png
September 4, 2100
148150152154156
SE2104Jun22T.png
June 22, 2104
SE2108Apr11P.gif
April 11, 2108
Saros152 18van70 SE2112Jan29T.jpg
January 29, 2112
SE2115Nov16A.png
November 16, 2115
Saros156 07van69 SE2119Sep05P.jpg
September 5, 2119
158160162164
Saros158 04van70 SE2123Jun23P.jpg
June 23, 2123
Saros164 03van80 SE2134Nov16P.jpg
November 16, 2134

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.

The partial solar eclipses on March 27, 1884 (part of Saros 108) and December 24, 1916 (part of Saros 111) are also a part of this series but are not included in the table below.

Series members between 1971 and 2200
SE1971Jul22P.png
July 22, 1971
(Saros 116)
SE1982Jun21P.png
June 21, 1982
(Saros 117)
SE1993May21P.png
May 21, 1993
(Saros 118)
SE2004Apr19P.png
April 19, 2004
(Saros 119)
SE2015Mar20T.png
March 20, 2015
(Saros 120)
SE2026Feb17A.png
February 17, 2026
(Saros 121)
SE2037Jan16P.png
January 16, 2037
(Saros 122)
SE2047Dec16P.png
December 16, 2047
(Saros 123)
SE2058Nov16P.png
November 16, 2058
(Saros 124)
SE2069Oct15P.png
October 15, 2069
(Saros 125)
SE2080Sep13P.png
September 13, 2080
(Saros 126)
SE2091Aug15T.png
August 15, 2091
(Saros 127)
SE2102Jul15A.png
July 15, 2102
(Saros 128)
SE2113Jun13T.png
June 13, 2113
(Saros 129)
SE2124May14T.png
May 14, 2124
(Saros 130)
SE2135Apr13A.png
April 13, 2135
(Saros 131)
SE2146Mar12A.png
March 12, 2146
(Saros 132)
SE2157Feb09T.png
February 9, 2157
(Saros 133)
SE2168Jan10A.png
January 10, 2168
(Saros 134)
SE2178Dec09A.png
December 9, 2178
(Saros 135)
SE2189Nov08T.png
November 8, 2189
(Saros 136)
SE2200Oct09A.png
October 9, 2200
(Saros 137)

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
SE1827Apr26A.gif
April 26, 1827
(Saros 116)
SE1856Apr05T.gif
April 5, 1856
(Saros 117)
SE1885Mar16A.gif
March 16, 1885
(Saros 118)
SE1914Feb25A.png
February 25, 1914
(Saros 119)
SE1943Feb04T.png
February 4, 1943
(Saros 120)
SE1972Jan16A.png
January 16, 1972
(Saros 121)
SE2000Dec25P.png
December 25, 2000
(Saros 122)
SE2029Dec05P.png
December 5, 2029
(Saros 123)
SE2058Nov16P.png
November 16, 2058
(Saros 124)
SE2087Oct26P.png
October 26, 2087
(Saros 125)
Saros126 53van72 SE2116Oct06P.jpg
October 6, 2116
(Saros 126)
Saros127 65van82 SE2145Sep16P.jpg
September 16, 2145
(Saros 127)
Saros128 67van73 SE2174Aug27P.jpg
August 27, 2174
(Saros 128)

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References

  1. "November 16, 2058 Partial Solar Eclipse". timeanddate. Retrieved 17 August 2024.
  2. "Partial Solar Eclipse of 2058 Nov 16". EclipseWise.com. Retrieved 17 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 124". eclipse.gsfc.nasa.gov.