Solar eclipse of January 16, 2075
A total solar eclipse will occur at the Moon's descending node of orbit on Wednesday, January 16, 2075, with a magnitude of 1.0311. 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
Eclipses in 2075
- A penumbral lunar eclipse on January 2, 2075.
- A total solar eclipse on January 16, 2075.
- A partial lunar eclipse on June 28, 2075.
- An annular solar eclipse on July 13, 2075.
- A partial lunar eclipse on December 22, 2075.
Metonic
- Preceded by: Solar eclipse of March 31, 2071
- Followed by: Solar eclipse of November 4, 2078
Tzolkinex
- Preceded by: Solar eclipse of December 6, 2067
- Followed by: Solar eclipse of February 27, 2082
Half-Saros
- Preceded by: Lunar eclipse of January 11, 2066
- Followed by: Lunar eclipse of January 22, 2084
Tritos
- Preceded by: Solar eclipse of February 17, 2064
- Followed by: Solar eclipse of December 16, 2085
Solar Saros 142
- Preceded by: Solar eclipse of January 5, 2057
- Followed by: Solar eclipse of January 27, 2093
Inex
- Preceded by: Solar eclipse of February 5, 2046
- Followed by: Solar eclipse of December 29, 2103
Triad
- Preceded by: Solar eclipse of March 18, 1988
- Followed by: Solar eclipse of November 17, 2161
Solar eclipses of 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]
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 |
Saros 142
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 |
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 series
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
References
- Earth visibility chart and eclipse statistics Eclipse Predictions by Fred Espenak, NASA/GSFC
- Google interactive map
- Besselian elements
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By era | |
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Saros series (list) | |
Visibility | |
Historical |
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![21 August 2017 total solar eclipse](http://upload.wikimedia.org/wikipedia/commons/thumb/4/42/Solar_eclipse%2C_Miles_Landing_8-21-17_%2836842678271%29.jpg/80px-Solar_eclipse%2C_Miles_Landing_8-21-17_%2836842678271%29.jpg)
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Annular eclipses
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- 1820
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- 2030
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- Jan. 2038
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![23 October 2014 partial eclipse](http://upload.wikimedia.org/wikipedia/commons/thumb/0/09/Partial_solar_eclipse_Oct_23_2014_Minneapolis_5-36pm_Ruen1.png/80px-Partial_solar_eclipse_Oct_23_2014_Minneapolis_5-36pm_Ruen1.png)
Partial eclipses
→ next partial
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