| Partial eclipse | |
 Map | |
| 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 eclipse | 3:23:07 |
| References | |
| Saros | 124 (57 of 73) |
| Catalog # (SE5000) | 9639 |
A partialsolar eclipse will occur at the Moon'sdescending node of orbit on Saturday, November 16, 2058,[1] with amagnitude of 0.7644. Asolar eclipse occurs when theMoon passes betweenEarth and theSun, 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 ofNortheast Asia.
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]
| Event | Time (UTC) |
|---|---|
| First Penumbral External Contact | 2058 November 16 at 01:25:37.0 UTC |
| Equatorial Conjunction | 2058 November 16 at 02:38:28.2 UTC |
| Ecliptic Conjunction | 2058 November 16 at 03:10:59.7 UTC |
| Greatest Eclipse | 2058 November 16 at 03:23:07.3 UTC |
| Last Penumbral External Contact | 2058 November 16 at 05:20:50.7 UTC |
| Parameter | Value |
|---|---|
| Eclipse Magnitude | 0.76445 |
| Eclipse Obscuration | 0.69696 |
| Gamma | 1.12238 |
| Sun Right Ascension | 15h26m32.8s |
| Sun Declination | -18°46'09.8" |
| Sun Semi-Diameter | 16'10.2" |
| Sun Equatorial Horizontal Parallax | 08.9" |
| Moon Right Ascension | 15h28m05.5s |
| Moon Declination | -17°45'10.1" |
| Moon Semi-Diameter | 15'47.0" |
| Moon Equatorial Horizontal Parallax | 0°57'55.4" |
| ΔT | 89.7 s |
This eclipse is part of aneclipse 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 afortnight.
| November 16 Descending node (new moon) | November 30 Ascending node (full moon) |
|---|---|
|  |
| Partial solar eclipse Solar Saros 124 | Total lunar eclipse Lunar Saros 136 |
This eclipse is a member of asemester series. An eclipse in a semester series of solar eclipses repeats approximately every 177 days and 4 hours (a semester) at alternatingnodes of the Moon's orbit.[3]
The partial solar eclipse onJune 21, 2058 occurs in the previous lunar year eclipse set.
| Solar eclipse series sets from 2058 to 2061 | ||||||
|---|---|---|---|---|---|---|
| Ascending node | Descending node | |||||
| Saros | Map | Gamma | Saros | Map | Gamma | |
| 119 | May 22, 2058 Partial | −1.3194 | 124 | November 16, 2058 Partial | 1.1224 | |
| 129 | May 11, 2059 Total | −0.508 | 134 | November 5, 2059 Annular | 0.4454 | |
| 139 | April 30, 2060 Total | 0.2422 | 144 | October 24, 2060 Annular | −0.2625 | |
| 149 | April 20, 2061 Total | 0.9578 | 154 | October 13, 2061 Annular | −0.9639 | |
This eclipse is a part ofSaros 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 throughSeptember 22, 1968, and a hybrid eclipse onOctober 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 oneexeligmos 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’sdescending node of orbit.[4]
| Series members 43–64 occur between 1801 and 2200: | ||
|---|---|---|
| 43 | 44 | 45 |
 June 16, 1806 |  June 26, 1824 |  July 8, 1842 |
| 46 | 47 | 48 |
 July 18, 1860 |  July 29, 1878 |  August 9, 1896 |
| 49 | 50 | 51 |
 August 21, 1914 |  August 31, 1932 |  September 12, 1950 |
| 52 | 53 | 54 |
 September 22, 1968 |  October 3, 1986 |  October 14, 2004 |
| 55 | 56 | 57 |
 October 25, 2022 |  November 4, 2040 | November 16, 2058 |
| 58 | 59 | 60 |
 November 26, 2076 |  December 7, 2094 |  December 19, 2112 |
| 61 | 62 | 63 |
 December 30, 2130 |  January 9, 2149 |  January 21, 2167 |
| 64 | ||
 January 31, 2185 | ||
Themetonic 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 22–23 | April 10–11 | January 27–29 | November 15–16 | September 3–5 |
| 118 | 120 | 122 | 124 | 126 |
 June 23, 2047 |  April 11, 2051 |  January 27, 2055 | November 16, 2058 |  September 3, 2062 |
| 128 | 130 | 132 | 134 | 136 |
 June 22, 2066 |  April 11, 2070 |  January 27, 2074 |  November 15, 2077 |  September 3, 2081 |
| 138 | 140 | 142 | 144 | 146 |
 June 22, 2085 |  April 10, 2089 |  January 27, 2093 |  November 15, 2096 |  September 4, 2100 |
| 148 | 150 | 152 | 154 | 156 |
 June 22, 2104 |  April 11, 2108 |  January 29, 2112 |  November 16, 2115 |  September 5, 2119 |
| 158 | 160 | 162 | 164 | |
 June 23, 2123 |  November 16, 2134 | |||
This eclipse is a part of atritos cycle, repeating at alternating nodes every 135synodic months (≈ 3986.63 days, or 11 years minus 1 month). Their appearance and longitude are irregular due to a lack of synchronization with theanomalistic 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) andDecember 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) | |||
This eclipse is a part of the long periodinex cycle, repeating at alternating nodes, every 358synodic months (≈ 10,571.95 days, or 29 years minus 20 days). Their appearance and longitude are irregular due to a lack of synchronization with theanomalistic 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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