Solar eclipse of April 10, 2089: Difference between revisions
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{{Solar eclipse set 2087-2090}} |
{{Solar eclipse set 2087-2090}} |
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=== Saros 140 === |
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=== Saros 140 === |
=== Saros 140 === |
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Revision as of 23:13, 30 May 2019
Solar eclipse of April 10, 2089 | |
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Type of eclipse | |
Nature | Annular |
Gamma | −0.3319 |
Magnitude | 0.9919 |
Maximum eclipse | |
Duration | 53 s (0 min 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.
Related eclipses
Solar eclipses 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 |
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 |
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