Solar eclipse of October 14, 2042: Difference between revisions
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=== Saros 144 === |
=== Saros 144 === |
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{{Solar Saros series 144}} |
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It is a part of [[Solar Saros 144|Saros cycle 144]], repeating every 18 years, 11 days, containing 70 events. The series started with partial solar eclipse on April 11, 1736. It contains annular eclipses from July 7, 1880 through August 27, 2565. There are no total eclipses in the series. The series ends at member 70 as a partial eclipse on May 5, 2980. The longest duration of annularity will be 9 minutes, 52 seconds on December 29, 2168. |
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{| class="wikitable collapsible collapsed" |
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!colspan=3|Series members 11–21 occur between 1901 and 2100: |
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|- |
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!11 |
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!12 |
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!13 |
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|- style="text-align:center;" |
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|[[File:SE1916Jul30A.png|150px]]<br />[[solar eclipse of July 30, 1916|July 30, 1916]] |
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|[[File:SE1934Aug10A.png|150px]]<br />[[solar eclipse of August 10, 1934|August 10, 1934]] |
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|[[File:SE1952Aug20A.png|150px]]<br />[[solar eclipse of August 20, 1952|August 20, 1952]] |
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|- |
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!14 |
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!15 |
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!16 |
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|- style="text-align:center;" |
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|[[File:SE1970Aug31A.png|150px]]<br />[[solar eclipse of August 31, 1970|August 31, 1970]] |
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|[[File:SE1988Sep11A.png|150px]]<br />[[solar eclipse of September 11, 1988|September 11, 1988]] |
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|[[File:SE2006Sep22A.png|150px]]<br />[[solar eclipse of September 22, 2006|September 22, 2006]] |
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|- |
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!17 |
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!18 |
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!19 |
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|- style="text-align:center;" |
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|[[File:SE2024Oct02A.png|150px]]<br />[[solar eclipse of October 2, 2024|October 2, 2024]] |
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|[[File:SE2042Oct14A.png|150px]]<br />[[solar eclipse of October 14, 2042|October 14, 2042]] |
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|[[File:SE2060Oct24A.png|150px]]<br />[[solar eclipse of October 24, 2060|October 24, 2060]] |
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|- |
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!20 |
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!21 |
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|- style="text-align:center;" |
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|[[File:SE2078Nov04A.png|150px]]<br />[[solar eclipse of November 4, 2078|November 4, 2078]] |
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|[[File:SE2096Nov15A.png|150px]]<br />[[solar eclipse of November 15, 2096|November 15, 2096]] |
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|}<noinclude> |
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=== Inex series === |
=== Inex series === |
Revision as of 02:00, 14 July 2024
Solar eclipse of October 14, 2042 | |
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Type of eclipse | |
Nature | Annular |
Gamma | −0.303 |
Magnitude | 0.93 |
Maximum eclipse | |
Duration | 464 s (7 min 44 s) |
Coordinates | 23°42′S 137°48′E / 23.7°S 137.8°E |
Max. width of band | 273 km (170 mi) |
Times (UTC) | |
Greatest eclipse | 2:00:42 |
References | |
Saros | 144 (18 of 70) |
Catalog # (SE5000) | 9602 |
An annular solar eclipse will occur at the Moon's descending node of orbit on Tuesday, October 14, 2042, with a magnitude of 0.93. 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 will be the second eclipse to cross Southeast Asia in 2042 after the total solar eclipse of April 20, 2042.
Images
Related eclipses
Eclipses in 2042
- A penumbral lunar eclipse on April 5, 2042.
- A total solar eclipse on April 20, 2042.
- A penumbral lunar eclipse on September 29, 2042.
- An annular solar eclipse on October 14, 2042.
Metonic
- Preceded by: Solar eclipse of December 26, 2038
- Followed by: Solar eclipse of August 2, 2046
Tzolkinex
- Preceded by: Solar eclipse of September 2, 2035
- Followed by: Solar eclipse of November 25, 2049
Half-Saros
- Preceded by: Lunar eclipse of October 8, 2033
- Followed by: Lunar eclipse of October 19, 2051
Tritos
- Preceded by: Solar eclipse of November 14, 2031
- Followed by: Solar eclipse of September 12, 2053
Solar Saros 144
- Preceded by: Solar eclipse of October 2, 2024
- Followed by: Solar eclipse of October 24, 2060
Inex
- Preceded by: Solar eclipse of November 3, 2013
- Followed by: Solar eclipse of September 23, 2071
Triad
- Preceded by: Solar eclipse of December 14, 1955
- Followed by: Solar eclipse of August 15, 2129
Solar eclipses of 2040–2043
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]
Solar eclipse series sets from 2040 to 2043 | ||||||
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Ascending node | Descending node | |||||
Saros | Map | Gamma | Saros | Map | Gamma | |
119 | May 11, 2040 Partial |
−1.2529 | 124 | November 4, 2040 Partial |
1.0993 | |
129 | April 30, 2041 Total |
−0.4492 | 134 | October 25, 2041 Annular |
0.4133 | |
139 | April 20, 2042 Total |
0.2956 | 144 | October 14, 2042 Annular |
−0.303 | |
149 | April 9, 2043 Total (non-central) |
1.0031 | 154 | October 3, 2043 Annular (non-central) |
1.0102 |
Saros 144
This eclipse is a part of Saros series 144, repeating every 18 years, 11 days, and containing 70 events. The series started with a partial solar eclipse on April 11, 1736. It contains annular eclipses from July 7, 1880 through August 27, 2565. There are no hybrid or total eclipses in this set. The series ends at member 70 as a partial eclipse on May 5, 2980. 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 annularity will be produced by member 51 at 9 minutes, 52 seconds on December 29, 2168. All eclipses in this series occur at the Moon’s descending node of orbit.[2]
Series members 5–26 occur between 1801 and 2200: | ||
---|---|---|
5 | 6 | 7 |
May 25, 1808 |
June 5, 1826 |
June 16, 1844 |
8 | 9 | 10 |
June 27, 1862 |
July 7, 1880 |
July 18, 1898 |
11 | 12 | 13 |
July 30, 1916 |
August 10, 1934 |
August 20, 1952 |
14 | 15 | 16 |
August 31, 1970 |
September 11, 1988 |
September 22, 2006 |
17 | 18 | 19 |
October 2, 2024 |
October 14, 2042 |
October 24, 2060 |
20 | 21 | 22 |
November 4, 2078 |
November 15, 2096 |
November 27, 2114 |
23 | 24 | 25 |
December 7, 2132 |
December 19, 2150 |
December 29, 2168 |
26 | ||
January 9, 2187 |
Inex series
This eclipse is a part of the long period inex cycle, repeating at alternating nodes, every 358 synodic months (≈ 10,571.95 days, or 29 years minus 20 days). Their appearance and longitude are irregular due to a lack of synchronization with the anomalistic month (period of perigee). However, groupings of 3 inex cycles (≈ 87 years minus 2 months) comes close (≈ 1,151.02 anomalistic months), so eclipses are similar in these groupings.
Inex series members between 1901 and 2100: | ||
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January 3, 1927 (Saros 140) |
December 14, 1955 (Saros 141) |
November 22, 1984 (Saros 142) |
November 3, 2013 (Saros 143) |
October 14, 2042 (Saros 144) |
September 23, 2071 (Saros 145) |
September 4, 2100 (Saros 146) |
Metonic series
The metonic series repeats eclipses every 19 years (6939.69 days), lasting about 5 cycles. Eclipses occur in nearly the same calendar date. In addition, the octon subseries repeats 1/5 of that or every 3.8 years (1387.94 days). All eclipses in this table occur at the Moon's descending node.
21 eclipse events between May 21, 1993 and May 20, 2069 | ||||
---|---|---|---|---|
May 20–21 | March 9 | December 25–26 | October 13–14 | August 1–2 |
118 | 120 | 122 | 124 | 126 |
May 21, 1993 |
March 9, 1997 |
December 25, 2000 |
October 14, 2004 |
August 1, 2008 |
128 | 130 | 132 | 134 | 136 |
May 20, 2012 |
March 9, 2016 |
December 26, 2019 |
October 14, 2023 |
August 2, 2027 |
138 | 140 | 142 | 144 | 146 |
May 21, 2031 |
March 9, 2035 |
December 26, 2038 |
October 14, 2042 |
August 2, 2046 |
148 | 150 | 152 | 154 | 156 |
May 20, 2050 |
March 9, 2054 |
December 26, 2057 |
October 13, 2061 |
August 2, 2065 |
158 | ||||
May 20, 2069 |
References
- ^ 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 144". eclipse.gsfc.nasa.gov.