A partial solar eclipse will occur at the Moon's ascending node of orbit on Wednesday, May 22, 2058, with a magnitude of 0.4141. 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.
Solar eclipse of May 22, 2058 | |
---|---|
Type of eclipse | |
Nature | Partial |
Gamma | −1.3194 |
Magnitude | 0.4141 |
Maximum eclipse | |
Coordinates | 63°30′S 61°06′E / 63.5°S 61.1°E |
Times (UTC) | |
Greatest eclipse | 10:39:25 |
References | |
Saros | 119 (68 of 71) |
Catalog # (SE5000) | 9638 |
Related eclipses
editEclipses in 2058
edit- A partial solar eclipse on May 22.
- A total lunar eclipse on June 6.
- A partial solar eclipse on June 21.
- A partial solar eclipse on November 16.
- A total lunar eclipse on November 30.
Metonic
edit- Preceded by: Solar eclipse of August 3, 2054
- Followed by: Solar eclipse of March 11, 2062
Tzolkinex
edit- Preceded by: Solar eclipse of April 11, 2051
- Followed by: Solar eclipse of July 3, 2065
Half-Saros
edit- Preceded by: Lunar eclipse of May 17, 2049
- Followed by: Lunar eclipse of May 28, 2067
Tritos
edit- Preceded by: Solar eclipse of June 23, 2047
- Followed by: Solar eclipse of April 21, 2069
Solar Saros 119
edit- Preceded by: Solar eclipse of May 11, 2040
- Followed by: Solar eclipse of June 1, 2076
Inex
edit- Preceded by: Solar eclipse of June 12, 2029
- Followed by: Solar eclipse of May 2, 2087
Triad
edit- Preceded by: Solar eclipse of July 22, 1971
- Followed by: Solar eclipse of March 23, 2145
Solar eclipses of 2058–2061
editThis 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 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 | |||||
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 |
Saros 119
editThis eclipse is a part of Saros series 119, repeating every 18 years, 11 days, and containing 71 events. The series started with a partial solar eclipse on May 15, 850 AD. It contains total eclipses on August 9, 994 AD and August 20, 1012; a hybrid eclipse on August 31, 1030; and annular eclipses from September 10, 1048 through March 18, 1950. The series ends at member 71 as a partial eclipse on June 24, 2112. 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 10 at 32 seconds on August 20, 1012, and the longest duration of annularity was produced by member 44 at 7 minutes, 37 seconds on September 1, 1625. All eclipses in this series occur at the Moon’s ascending node of orbit.[2]
Series members 54–71 occur between 1801 and 2112: | ||
---|---|---|
54 | 55 | 56 |
December 21, 1805 |
January 1, 1824 |
January 11, 1842 |
57 | 58 | 59 |
January 23, 1860 |
February 2, 1878 |
February 13, 1896 |
60 | 61 | 62 |
February 25, 1914 |
March 7, 1932 |
March 18, 1950 |
63 | 64 | 65 |
March 28, 1968 |
April 9, 1986 |
April 19, 2004 |
66 | 67 | 68 |
April 30, 2022 |
May 11, 2040 |
May 22, 2058 |
69 | 70 | 71 |
June 1, 2076 |
June 13, 2094 |
June 24, 2112 |
Metonic series
editThe 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 3–4 | May 22–24 | March 10–11 | December 27–29 | October 14–16 |
117 | 119 | 121 | 123 | 125 |
August 3, 2054 |
May 22, 2058 |
March 11, 2062 |
December 27, 2065 |
October 15, 2069 |
127 | 129 | 131 | 133 | 135 |
August 3, 2073 |
May 22, 2077 |
March 10, 2081 |
December 27, 2084 |
October 14, 2088 |
137 | 139 | 141 | 143 | 145 |
August 3, 2092 |
May 22, 2096 |
March 10, 2100 |
December 29, 2103 |
October 16, 2107 |
147 | 149 | 151 | 153 | 155 |
August 4, 2111 |
May 24, 2115 |
March 11, 2119 |
December 28, 2122 |
October 16, 2126 |
157 | 159 | 161 | 163 | 165 |
August 4, 2130 |
May 23, 2134 |
October 16, 2145 |
Tritos series
editThis 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 2036 and 2200 | ||||
---|---|---|---|---|
July 23, 2036 (Saros 117) |
June 23, 2047 (Saros 118) |
May 22, 2058 (Saros 119) |
April 21, 2069 (Saros 120) |
March 21, 2080 (Saros 121) |
February 18, 2091 (Saros 122) |
January 19, 2102 (Saros 123) |
December 19, 2112 (Saros 124) |
November 18, 2123 (Saros 125) |
October 17, 2134 (Saros 126) |
September 16, 2145 (Saros 127) |
August 16, 2156 (Saros 128) |
July 16, 2167 (Saros 129) |
June 16, 2178 (Saros 130) |
May 15, 2189 (Saros 131) |
April 14, 2200 (Saros 132) |
Inex series
editThis 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 | ||
---|---|---|
October 31, 1826 (Saros 111) |
||
August 31, 1913 (Saros 114) |
August 12, 1942 (Saros 115) |
July 22, 1971 (Saros 116) |
July 1, 2000 (Saros 117) |
June 12, 2029 (Saros 118) |
May 22, 2058 (Saros 119) |
May 2, 2087 (Saros 120) |
April 13, 2116 (Saros 121) |
March 23, 2145 (Saros 122) |
March 3, 2174 (Saros 123) |
References
edit- ^ 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.
- ^ "NASA - Catalog of Solar Eclipses of Saros 119". eclipse.gsfc.nasa.gov.
External links
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