Solar eclipse of January 16, 2075 | |
---|---|
Type of eclipse | |
Nature | Total |
Gamma | −0.2799 |
Magnitude | 1.0311 |
Maximum eclipse | |
Duration | 162 s (2 min 42 s) |
Coordinates | 37°12′S94°06′W / 37.2°S 94.1°W |
Max. width of band | 110 km (68 mi) |
Times (UTC) | |
Greatest eclipse | 18:36:04 |
References | |
Saros | 142 (26 of 72) |
Catalog # (SE5000) | 9675 |
A total solar eclipse will occur on Wednesday, January 16, 2075. 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 total solar eclipse occurs when the Moon's apparent diameter is larger than the Sun's, blocking all direct sunlight, turning day into darkness. Totality occurs in a narrow path across Earth's surface, with the partial solar eclipse visible over a surrounding region thousands of kilometres wide.
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]
122 | February 7, 2073 Partial | 127 | August 3, 2073 Total |
132 | January 27, 2074 Annular | 137 | July 24, 2074 Annular |
142 | January 16, 2075 Total | 147 | July 13, 2075 Annular |
152 | January 6, 2076 Total | 157 | July 1, 2076 Partial |
It is a part of Saros cycle 142, repeating every 18 years, 11 days, containing 72 events. The series started with partial solar eclipse on April 17, 1624. It contains one hybrid eclipse on July 14, 1768, and total eclipses from July 25, 1786 through October 29, 2543. The series ends at member 72 as a partial eclipse on June 5, 2904. The longest duration of totality will be 6 minutes, 34 seconds on May 28, 2291. All eclipses in this series occurs at the Moon’s descending node. [2]
Series members 17–41 occur between 1901 and 2359 | ||
---|---|---|
17 | 18 | 19 |
October 10, 1912 | October 21, 1930 | November 1, 1948 |
20 | 21 | 22 |
November 12, 1966 | November 22, 1984 | December 4, 2002 |
23 | 24 | 25 |
December 14, 2020 | December 26, 2038 | January 5, 2057 |
26 | 27 | 28 |
January 16, 2075 | January 27, 2093 | February 8, 2111 |
29 | 30 | 31 |
February 18, 2129 | March 2, 2147 | March 12, 2165 |
32 | 33 | 34 |
March 23, 2183 | April 4, 2201 | April 15, 2219 |
35 | 36 | 37 |
April 25, 2237 | May 7, 2255 | May 17, 2273 |
38 | 39 | 40 |
May 28, 2291 | June 9, 2309 | June 20, 2327 |
41 | ||
June 30, 2345 |
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.
Inex series members between 1901 and 2100: | ||
---|---|---|
May 18, 1901 (Saros 136) | April 28, 1930 (Saros 137) | April 8, 1959 (Saros 138) |
March 18, 1988 (Saros 139) | February 26, 2017 (Saros 140) | February 5, 2046 (Saros 141) |
January 16, 2075 (Saros 142) |
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).
21 eclipse events between June 12, 2029 and June 12, 2105 | ||||
---|---|---|---|---|
June 11–12 | March 30–31 | January 16 | November 4–5 | August 23–24 |
118 | 120 | 122 | 124 | 126 |
June 12, 2029 | March 30, 2033 | January 16, 2037 | November 4, 2040 | August 23, 2044 |
128 | 130 | 132 | 134 | 136 |
June 11, 2048 | March 30, 2052 | January 16, 2056 | November 5, 2059 | August 24, 2063 |
138 | 140 | 142 | 144 | 146 |
June 11, 2067 | March 31, 2071 | January 16, 2075 | November 4, 2078 | August 24, 2082 |
148 | 150 | 152 | 154 | |
June 11, 2086 | March 31, 2090 | January 16, 2094 | November 4, 2097 |
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