| Solar eclipse of April 10, 2089 | |
|---|---|
 Map | |
| Type of eclipse | |
| Nature | Annular |
| Gamma | −0.3319 |
| Magnitude | 0.9919 |
| Maximum eclipse | |
| Duration | 53 sec (0 m 53 s) |
| Coordinates | 10°12′S 154°48′W / 10.2°S 154.8°W |
| Max. width of band | 30 km (19 mi) |
| Times (UTC) | |
| Greatest eclipse | 22:44:42 |
| References | |
| Saros | 140 (33 of 71) |
| Catalog # (SE5000) | 9708 |
An annular solar eclipse will occur on April 10, 2089. 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.
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 |
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 |
 Dec 23, 1908 |
 Jan 3, 1927 |
 Jan 14, 1945 |
| 26 | 27 | 28 |
 Jan 25, 1963 |
 Feb 4, 1981 |
 Feb 16, 1999 |
| 29 | 30 | 31 |
 Feb 26, 2017 |
 Mar 9, 2035 |
 Mar 20, 2053 |
| 32 | 33 | 34 |
 Mar 31, 2071 |
Apr 10, 2089 |
 Apr 23, 2107 |
| 35 | 36 | 37 |
 May 3, 2125 |
 May 14, 2143 |
 May 25, 2161 |
| 38 | 39 | 40 |
 Jun 5, 2179 |
 Jun 15, 2197 |
 Jun 28, 2215 |
| 41 | 42 | 43 |
 Jul 8, 2233 |
 Jul 19, 2251 |
 Jul 29, 2269 |
| 44 | 45 | 46 |
 Aug 10, 2287 |
 Aug 21, 2305 |
 Sep 1, 2323 |
| 47 | 48 | 49 |
 Sep 12, 2341 |
 Sep 23, 2359 |
 Oct 3, 2377 |
| 50 | 51 | 52 |
 Oct 14, 2395 |
 Oct 25, 2413 |
 Nov 5, 2431 |
| 53 | ||
 Nov 15, 2449 | ||
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) |
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