Template:Solar Saros series 142: Difference between revisions
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This eclipse is a part of [[Solar Saros 142|Saros series 142]], repeating every 18 years, 11 days, and containing 72 events. The series started with a partial solar eclipse on April 17, 1624. It contains a hybrid eclipse on July 14, 1768, and total eclipses from July 25, 1786 through October 29, 2543. There are no annular eclipses in this set. The series ends at member 72 as a partial eclipse on June 5, 2904. 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. |
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The longest duration of totality will be produced by member 38 at 6 minutes, 34 seconds on May 28, 2291. All eclipses in this series occur at the Moon’s [[Lunar node|descending node]] of orbit.<ref>{{Cite web|url=https://eclipse.gsfc.nasa.gov/SEsaros/SEsaros142.html|title=NASA - Catalog of Solar Eclipses of Saros 142|website=eclipse.gsfc.nasa.gov}}</ref> |
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!colspan=3|Series members |
!colspan=3|Series members 11–32 occur between 1801 and 2200: |
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!14 |
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!15 |
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!16 |
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|[[File:SE1858Sep07T.png|150px]]<br />[[solar eclipse of September 7, 1858|September 7, 1858]] |
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!17 |
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|[[File:SE2183Mar23T.png|150px]]<br />March 23, 2183 |
|[[File:SE2183Mar23T.png|150px]]<br />March 23, 2183 |
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!37 |
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!38 |
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!40 |
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|[[File:SE2291May28T.png|150px]]<br />May 28, 2291 |
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|[[File:SE2309Jun09T.png|150px]]<br />June 9, 2309 |
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|[[File:SE2327Jun20T.png|150px]]<br />June 20, 2327 |
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!41 |
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|- style="text-align:center;" |
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|[[File:SE2345Jun30T.png|150px]]<br />June 30, 2345 |
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[[Category:Solar eclipse templates]] |
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Latest revision as of 01:43, 14 July 2024
This eclipse is a part of Saros series 142, repeating every 18 years, 11 days, and containing 72 events. The series started with a partial solar eclipse on April 17, 1624. It contains a hybrid eclipse on July 14, 1768, and total eclipses from July 25, 1786 through October 29, 2543. There are no annular eclipses in this set. The series ends at member 72 as a partial eclipse on June 5, 2904. 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 will be produced by member 38 at 6 minutes, 34 seconds on May 28, 2291. All eclipses in this series occur at the Moon’s descending node of orbit.[1]
Series members 11–32 occur between 1801 and 2200: | ||
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11 | 12 | 13 |
August 5, 1804 |
August 16, 1822 |
August 27, 1840 |
14 | 15 | 16 |
September 7, 1858 |
September 17, 1876 |
September 29, 1894 |
17 | 18 | 19 |
October 10, 1912 |
October 21, 1930 |
November 1, 1948 |
20 | 21 | 22 |
November 12, 1966 |
November 22, 1984 |
December 4, 2002 |
23 | 24 | 25 |
December 14, 2020 |
December 26, 2038 |
January 5, 2057 |
26 | 27 | 28 |
January 16, 2075 |
January 27, 2093 |
February 8, 2111 |
29 | 30 | 31 |
February 18, 2129 |
March 2, 2147 |
March 12, 2165 |
32 | ||
March 23, 2183 |
References
- ^ "NASA - Catalog of Solar Eclipses of Saros 142". eclipse.gsfc.nasa.gov.