Solar eclipse of January 26, 2028 | |
---|---|
Type of eclipse | |
Nature | Annular |
Gamma | 0.3901 |
Magnitude | 0.9208 |
Maximum eclipse | |
Duration | 627 s (10 min 27 s) |
Coordinates | 3°00′N51°30′W / 3°N 51.5°W |
Max. width of band | 323 km (201 mi) |
Times (UTC) | |
Greatest eclipse | 15:08:59 |
References | |
Saros | 141 (24 of 70) |
Catalog # (SE5000) | 9569 |
An annular solar eclipse will occur on Wednesday, January 26, 2028. 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 kilometres wide.
On January 26, 2028, the path of totality will pass through Ecuador, Peru, and northern Brazil. It will then travel across the Atlantic Ocean and end in Spain. A partial eclipse will be visible over much of Central and South America and Western Europe, as well as in northwestern Africa.
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. [1]
Ascending node | Descending node | |||||
---|---|---|---|---|---|---|
Saros | Map | Gamma | Saros | Map | Gamma | |
121 | 2026 February 17 Annular | −0.97427 | 126 | 2026 August 12 Total | 0.89774 | |
131 | 2027 February 6 Annular | −0.29515 | 136 | 2027 August 2 Total | 0.14209 | |
141 | 2028 January 26 Annular | 0.39014 | 146 | 2028 July 22 Total | −0.60557 | |
151 | 2029 January 14 Partial | 1.05532 | 156 | 2029 July 11 Partial | −1.41908 |
Partial solar eclipses on June 12, 2029, and December 5, 2029, occur in the next lunar year eclipse set.
Solar saros 141, repeating every about 18 years, 11 days, and 8 hours, contains 70 events. The series started with partial solar eclipse on May 19, 1613. It contains 41 annular eclipses from August 4, 1739, to October 14, 2460. There are no total eclipses in this series. The series ends at member 70 as a partial eclipse on June 13, 2857. The longest annular eclipse occurred on December 14, 1955, with maximum duration of annularity at 12 minutes and 9 seconds. All eclipses in this series occur at the Moon’s ascending node. [2]
Series members 17–36 occur between 1901 and 2259 | ||
---|---|---|
17 | 18 | 19 |
November 11, 1901 | November 22, 1919 | December 2, 1937 |
20 | 21 | 22 |
December 14, 1955 | December 24, 1973 | January 4, 1992 |
23 | 24 | 25 |
January 15, 2010 | January 26, 2028 | February 5, 2046 |
26 | 27 | 28 |
February 17, 2064 | February 27, 2082 | March 10, 2100 |
29 | 30 | 31 |
March 22, 2118 | April 1, 2136 | April 12, 2154 |
32 | 33 | 34 |
April 23, 2172 | May 4, 2190 | May 15, 2208 |
35 | 36 | |
May 27, 2226 | June 6, 2244 |
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.
21 eclipse events between June 21, 1982, and June 21, 2058 | ||||
---|---|---|---|---|
June 21 | April 8–9 | January 26 | November 13–14 | September 1–2 |
107 | 109 | 111 | 113 | 115 |
June 21, 1963 | April 9, 1967 | January 26, 1971 | November 14, 1974 | September 2, 1978 |
117 | 119 | 121 | 123 | 125 |
June 21, 1982 | April 9, 1986 | January 26, 1990 | November 13, 1993 | September 2, 1997 |
127 | 129 | 131 | 133 | 135 |
June 21, 2001 | April 8, 2005 | January 26, 2009 | November 13, 2012 | September 1, 2016 |
137 | 139 | 141 | 143 | 145 |
June 21, 2020 | April 8, 2024 | January 26, 2028 | November 14, 2031 | September 2, 2035 |
147 | 149 | 151 | 153 | 155 |
June 21, 2039 | April 9, 2043 | January 26, 2047 | November 14, 2050 | September 2, 2054 |
157 | ||||
June 21, 2058 |
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