Solar eclipse of April 10, 2089
An annular solar eclipse will occur at the Moon's descending node of orbit on Sunday, April 10, 2089, with a magnitude of 0.9919. 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.
Related eclipses
Eclipses in 2089
- A penumbral lunar eclipse on March 26, 2089.
- An annular solar eclipse on April 10, 2089.
- A penumbral lunar eclipse on September 19, 2089.
- A total solar eclipse on October 4, 2089.
Metonic
- Preceded by: Solar eclipse of June 22, 2085
- Followed by: Solar eclipse of January 27, 2093
Tzolkinex
- Preceded by: Solar eclipse of February 27, 2082
- Followed by: Solar eclipse of May 22, 2096
Half-Saros
- Preceded by: Lunar eclipse of April 4, 2080
- Followed by: Lunar eclipse of April 15, 2098
Tritos
- Preceded by: Solar eclipse of May 11, 2078
- Followed by: Solar eclipse of March 10, 2100
Solar Saros 140
- Preceded by: Solar eclipse of March 31, 2071
- Followed by: Solar eclipse of April 23, 2107
Inex
- Preceded by: Solar eclipse of April 30, 2060
- Followed by: Solar eclipse of March 22, 2118
Triad
- Preceded by: Solar eclipse of June 10, 2002
- Followed by: Solar eclipse of February 10, 2176
Solar eclipses of 2087–2090
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]
120 | May 2, 2087![]() Partial | 125 | October 26, 2087![]() Partial |
130 | April 21, 2088![]() Total | 135 | October 14, 2088![]() Annular |
140 | April 10, 2089![]() Annular | 145 | October 4, 2089![]() Total |
150 | March 31, 2090![]() Partial | 155 | September 23, 2090![]() Total |
Saros 140
It is a part of Saros cycle 140, repeating every 18 years, 11 days, containing 71 events. The series started with partial solar eclipse on April 16, 1512. It contains total eclipses from July 21, 1656, through November 9, 1836, hybrid eclipses from November 20, 1854, through December 23, 1908, and annular eclipses from January 3, 1927, through December 7, 2485. The series ends at member 71 as a partial eclipse on June 1, 2774. The longest duration of totality was 4 minutes, 10 seconds on August 12, 1692.
Series members 23–53 occur between 1901 and 2450: | ||
---|---|---|
23 | 24 | 25 |
![]() December 23, 1908 | ![]() January 3, 1927 | ![]() January 14, 1945 |
26 | 27 | 28 |
![]() January 25, 1963 | ![]() February 4, 1981 | ![]() February 16, 1999 |
29 | 30 | 31 |
![]() February 26, 2017 | ![]() March 9, 2035 | ![]() March 20, 2053 |
32 | 33 | 34 |
![]() March 31, 2071 | ![]() April 10, 2089 | ![]() April 23, 2107 |
35 | 36 | 37 |
![]() May 3, 2125 | ![]() May 14, 2143 | ![]() May 25, 2161 |
38 | 39 | 40 |
![]() June 5, 2179 | ![]() June 15, 2197 | ![]() June 28, 2215 |
41 | 42 | 43 |
![]() July 8, 2233 | ![]() July 19, 2251 | ![]() July 29, 2269 |
44 | 45 | 46 |
![]() August 10, 2287 | ![]() August 21, 2305 | ![]() September 1, 2323 |
47 | 48 | 49 |
![]() September 12, 2341 | ![]() September 23, 2359 | ![]() October 3, 2377 |
50 | 51 | 52 |
![]() October 14, 2395 | ![]() October 25, 2413 | ![]() November 5, 2431 |
53 | ||
![]() November 15, 2449 |
Tritos series
This 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 1901 and 2100 | |||
---|---|---|---|
![]() September 21, 1903 (Saros 123) | ![]() August 21, 1914 (Saros 124) | ![]() July 20, 1925 (Saros 125) | |
![]() June 19, 1936 (Saros 126) | ![]() May 20, 1947 (Saros 127) | ![]() April 19, 1958 (Saros 128) | |
![]() March 18, 1969 (Saros 129) | ![]() February 16, 1980 (Saros 130) | ![]() January 15, 1991 (Saros 131) | |
![]() December 14, 2001 (Saros 132) | ![]() November 13, 2012 (Saros 133) | ![]() October 14, 2023 (Saros 134) | |
![]() September 12, 2034 (Saros 135) | ![]() August 12, 2045 (Saros 136) | ![]() July 12, 2056 (Saros 137) | |
![]() June 11, 2067 (Saros 138) | ![]() May 11, 2078 (Saros 139) | ![]() April 10, 2089 (Saros 140) | |
![]() March 10, 2100 (Saros 141) |
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.
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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![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)
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