Solar eclipse of April 10, 2089: Difference between revisions
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=== Saros 140 === |
=== Saros 140 === |
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{{Solar Saros series 140}} |
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It is a part of [[Solar Saros 140|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. |
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{| class="wikitable collapsible collapsed" |
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!colspan=3|Series members 23–53 occur between 1901 and 2450: |
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|- |
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!23 |
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!24 |
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!25 |
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|- style="text-align:center;" |
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|[[File:SE1908Dec23H.png|150px]]<br />[[solar eclipse of December 23, 1908|December 23, 1908]] |
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|[[File:SE1927Jan03A.png|150px]]<br />[[solar eclipse of January 3, 1927|January 3, 1927]] |
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|[[File:SE1945Jan14A.png|150px]]<br />[[solar eclipse of January 14, 1945|January 14, 1945]] |
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|- |
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!26 |
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!27 |
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!28 |
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|- style="text-align:center;" |
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|[[File:SE1963Jan25A.png|150px]]<br />[[solar eclipse of January 25, 1963|January 25, 1963]] |
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|[[File:SE1981Feb04A.png|150px]]<br />[[solar eclipse of February 4, 1981|February 4, 1981]] |
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|[[File:SE1999Feb16A.png|150px]]<br />[[solar eclipse of February 16, 1999|February 16, 1999]] |
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|- |
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!29 |
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!30 |
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!31 |
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|- style="text-align:center;" |
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|[[File:SE2017Feb26A.png|150px]]<br />[[solar eclipse of February 26, 2017|February 26, 2017]] |
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|[[File:SE2035Mar09A.png|150px]]<br />[[solar eclipse of March 9, 2035|March 9, 2035]] |
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|[[File:SE2053Mar20A.png|150px]]<br />[[solar eclipse of March 20, 2053|March 20, 2053]] |
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|- |
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!32 |
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!33 |
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!34 |
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|- style="text-align:center;" |
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|[[File:SE2071Mar31A.png|150px]]<br />[[solar eclipse of March 31, 2071|March 31, 2071]] |
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|[[File:SE2089Apr10A.png|150px]]<br />[[solar eclipse of April 10, 2089|April 10, 2089]] |
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|[[File:SE2107Apr23A.png|150px]]<br />April 23, 2107 |
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|- |
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!35 |
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!36 |
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!37 |
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|- style="text-align:center;" |
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|[[File:SE2125May03A.png|150px]]<br />May 3, 2125 |
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|[[File:SE2143May14A.png|150px]]<br />May 14, 2143 |
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|[[File:SE2161May25A.png|150px]]<br />May 25, 2161 |
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|- |
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!38 |
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!39 |
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!40 |
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|- style="text-align:center;" |
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|[[File:SE2179Jun05A.png|150px]]<br />June 5, 2179 |
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|[[File:SE2197Jun15A.png|150px]]<br />June 15, 2197 |
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|[[File:SE2215Jun28A.png|150px]]<br />June 28, 2215 |
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|- |
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!41 |
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!42 |
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!43 |
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|- style="text-align:center;" |
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|[[File:SE2233Jul08A.png|150px]]<br />July 8, 2233 |
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|[[File:SE2251Jul19A.png|150px]]<br />July 19, 2251 |
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|[[File:SE2269Jul29A.png|150px]] <br />July 29, 2269 |
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|- |
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!44 |
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!45 |
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!46 |
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|- style="text-align:center;" |
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|[[File:SE2287Aug10A.png|150px]]<br />August 10, 2287 |
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|[[File:SE2305Aug21A.png|150px]]<br />August 21, 2305 |
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|[[File:SE2323Sep01A.png|150px]]<br />September 1, 2323 |
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|- |
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!47 |
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!48 |
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!49 |
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|- style="text-align:center;" |
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|[[File:SE2341Sep12A.png|150px]]<br />September 12, 2341 |
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|[[File:SE2359Sep23A.png|150px]]<br />September 23, 2359 |
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|[[File:SE2377Oct03A.png|150px]] <br />October 3, 2377 |
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|- |
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!50 |
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!51 |
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!52 |
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|- style="text-align:center;" |
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|[[File:SE2395Oct14A.png|150px]]<br />October 14, 2395 |
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|[[File:SE2413Oct25A.png|150px]]<br />October 25, 2413 |
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|[[File:SE2431Nov05A.png|150px]] <br />November 5, 2431 |
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|- |
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!53 |
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|- style="text-align:center;" |
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|[[File:SE2449Nov15A.png|150px]] <br />November 15, 2449 |
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|} |
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=== Tritos series === |
=== Tritos series === |
Revision as of 20:21, 13 July 2024
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 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]
The partial solar eclipse on June 1, 2087 occurs in the previous lunar year eclipse set.
Solar eclipse series sets from 2087 to 2090 | ||||||
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Descending node | Ascending node | |||||
Saros | Map | Gamma | Saros | Map | Gamma | |
120 | May 2, 2087 Partial |
1.1139 | 125 | October 26, 2087 Partial |
−1.2882 | |
130 | April 21, 2088 Total |
0.4135 | 135 | October 14, 2088 Annular |
−0.5349 | |
140 | April 10, 2089 Annular |
−0.3319 | 145 | October 4, 2089 Total |
0.2167 | |
150 | March 31, 2090 Partial |
−1.1028 | 155 | September 23, 2090 Total |
0.9157 |
Saros 140
This eclipse is a part of Saros series 140, repeating every 18 years, 11 days, and containing 71 events. The series started with a 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. Its eclipses are tabulated in three columns; every third eclipse in the same column is one exeligmos apart, so they all cast shadows over approximately the same parts of the Earth.
The longest duration of totality was produced by member 11 at 4 minutes, 10 seconds on August 12, 1692, and the longest duration of annularity will be produced by member 53 at 7 minutes, 35 seconds on November 15, 2449. All eclipses in this series occur at the Moon’s descending node of orbit.[2]
Series members 18–39 occur between 1801 and 2200: | ||
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18 | 19 | 20 |
October 29, 1818 |
November 9, 1836 |
November 20, 1854 |
21 | 22 | 23 |
November 30, 1872 |
December 12, 1890 |
December 23, 1908 |
24 | 25 | 26 |
January 3, 1927 |
January 14, 1945 |
January 25, 1963 |
27 | 28 | 29 |
February 4, 1981 |
February 16, 1999 |
February 26, 2017 |
30 | 31 | 32 |
March 9, 2035 |
March 20, 2053 |
March 31, 2071 |
33 | 34 | 35 |
April 10, 2089 |
April 23, 2107 |
May 3, 2125 |
36 | 37 | 38 |
May 14, 2143 |
May 25, 2161 |
June 5, 2179 |
39 | ||
June 15, 2197 |
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.
- ^ "NASA - Catalog of Solar Eclipses of Saros 140". eclipse.gsfc.nasa.gov.
References
- Earth visibility chart and eclipse statistics Eclipse Predictions by Fred Espenak, NASA/GSFC