A partial solar eclipse will occur at the Moon's descending node of orbit on Saturday, November 16, 2058, 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.

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.

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)
Partial solar eclipse Solar Saros 124Total lunar eclipse Lunar Saros 136

Related eclipses

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.

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 nodeDescending node
SarosMapGammaSarosMapGamma
119May 22, 2058 Partial−1.3194124November 16, 2058 Partial1.1224
129May 11, 2059 Total−0.508134November 5, 2059 Annular0.4454
139April 30, 2060 Total0.2422144October 24, 2060 Annular−0.2625
149April 20, 2061 Total0.9578154October 13, 2061 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.

Series members 43–64 occur between 1801 and 2200:
434445
June 16, 1806June 26, 1824July 8, 1842
464748
July 18, 1860July 29, 1878August 9, 1896
495051
August 21, 1914August 31, 1932September 12, 1950
525354
September 22, 1968October 3, 1986October 14, 2004
555657
October 25, 2022November 4, 2040November 16, 2058
585960
November 26, 2076December 7, 2094December 19, 2112
616263
December 30, 2130January 9, 2149January 21, 2167
64
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
June 23, 2047April 11, 2051January 27, 2055November 16, 2058September 3, 2062
128130132134136
June 22, 2066April 11, 2070January 27, 2074November 15, 2077September 3, 2081
138140142144146
June 22, 2085April 10, 2089January 27, 2093November 15, 2096September 4, 2100
148150152154156
June 22, 2104April 11, 2108January 29, 2112November 16, 2115September 5, 2119
158160162164
June 23, 2123November 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
July 22, 1971 (Saros 116)June 21, 1982 (Saros 117)May 21, 1993 (Saros 118)April 19, 2004 (Saros 119)March 20, 2015 (Saros 120)
February 17, 2026 (Saros 121)January 16, 2037 (Saros 122)December 16, 2047 (Saros 123)November 16, 2058 (Saros 124)October 15, 2069 (Saros 125)
September 13, 2080 (Saros 126)August 15, 2091 (Saros 127)July 15, 2102 (Saros 128)June 13, 2113 (Saros 129)May 14, 2124 (Saros 130)
April 13, 2135 (Saros 131)March 12, 2146 (Saros 132)February 9, 2157 (Saros 133)January 10, 2168 (Saros 134)December 9, 2178 (Saros 135)
November 8, 2189 (Saros 136)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
April 26, 1827 (Saros 116)April 5, 1856 (Saros 117)March 16, 1885 (Saros 118)
February 25, 1914 (Saros 119)February 4, 1943 (Saros 120)January 16, 1972 (Saros 121)
December 25, 2000 (Saros 122)December 5, 2029 (Saros 123)November 16, 2058 (Saros 124)
October 26, 2087 (Saros 125)October 6, 2116 (Saros 126)September 16, 2145 (Saros 127)
August 27, 2174 (Saros 128)

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