Solar eclipse of January 16, 2075
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′S 94°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 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.
Related eclipses
Solar eclipses 2073–2076
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]
The partial solar eclipses on June 1, 2076 and November 26, 2076 occur in the next lunar year eclipse set.
Solar eclipse series sets from 2073 to 2076 | ||||||
---|---|---|---|---|---|---|
Descending node | Ascending node | |||||
Saros | Map | Gamma | Saros | Map | Gamma | |
122 | February 7, 2073 Partial |
1.1651 | 127 | August 3, 2073 Total |
−0.8763 | |
132 | January 27, 2074 Annular |
0.4251 | 137 | July 24, 2074 Annular |
−0.1242 | |
142 | January 16, 2075 Total |
−0.2799 | 147 | July 13, 2075 Annular |
0.6583 | |
152 | January 6, 2076 Total |
−0.9373 | 157 | July 1, 2076 Partial |
1.4005 |
Saros series 142
This eclipse is a part of Saros series 142, repeating every 18 years, 11 days, and containing 72 events. The series started with a partial solar eclipse on April 17, 1624. It contains a hybrid eclipse on July 14, 1768, and total eclipses from July 25, 1786 through October 29, 2543. There are no annular eclipses in this set. The series ends at member 72 as a partial eclipse on June 5, 2904. 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 will be produced by member 38 at 6 minutes, 34 seconds on May 28, 2291. All eclipses in this series occur at the Moon’s descending node of orbit.[2]
Series members 11–32 occur between 1801 and 2200: | ||
---|---|---|
11 | 12 | 13 |
August 5, 1804 |
August 16, 1822 |
August 27, 1840 |
14 | 15 | 16 |
September 7, 1858 |
September 17, 1876 |
September 29, 1894 |
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 | ||
March 23, 2183 |
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.
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) |
Metonic cycle
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 |
Notes
- ^ 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 142". eclipse.gsfc.nasa.gov.
References
- Earth visibility chart and eclipse statistics Eclipse Predictions by Fred Espenak, NASA/GSFC