Solar eclipse of April 10, 2089

Future annular solar eclipse
10°12′S 154°48′W / 10.2°S 154.8°W / -10.2; -154.8Max. width of band30 km (19 mi)Times (UTC)Greatest eclipse22:44:42ReferencesSaros140 (33 of 71)Catalog # (SE5000)9708

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

Metonic

Tzolkinex

Half-Saros

  • Preceded by: Lunar eclipse of April 4, 2080
  • Followed by: Lunar eclipse of April 15, 2098

Tritos

Solar Saros 140

Inex

Triad

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

  1. ^ 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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