Solar eclipse of August 24, 2082
Solar eclipse of August 24, 2082 | |
---|---|
Type of eclipse | |
Nature | Total |
Gamma | −0.4004 |
Magnitude | 1.0452 |
Maximum eclipse | |
Duration | 241 s (4 min 1 s) |
Coordinates | 10°18′S 151°48′E / 10.3°S 151.8°E |
Max. width of band | 163 km (101 mi) |
Times (UTC) | |
Greatest eclipse | 1:16:21 |
References | |
Saros | 146 (31 of 76) |
Catalog # (SE5000) | 9692 |
A total solar eclipse will occur at the Moon's descending node of orbit on Monday, August 24, 2082, with a magnitude of 1.0452. 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. A total solar eclipse occurs when the Moon's apparent diameter is larger than the Sun's, blocking all direct sunlight, turning day into darkness. Totality occurs in a narrow path across Earth's surface, with the partial solar eclipse visible over a surrounding region thousands of kilometres wide.
Related eclipses[edit]
Eclipses in 2082[edit]
- A partial lunar eclipse on February 13, 2082.
- An annular solar eclipse on February 27, 2082.
- A penumbral lunar eclipse on August 8, 2082.
- A total solar eclipse on August 24, 2082.
Metonic[edit]
- Preceded by: Solar eclipse of November 4, 2078
- Followed by: Solar eclipse of June 11, 2086
Tzolkinex[edit]
- Preceded by: Solar eclipse of July 13, 2075
- Followed by: Solar eclipse of October 4, 2089
Half-Saros[edit]
- Preceded by: Lunar eclipse of August 17, 2073
- Followed by: Lunar eclipse of August 29, 2091
Tritos[edit]
- Preceded by: Solar eclipse of September 23, 2071
- Followed by: Solar eclipse of July 23, 2093
Solar Saros 146[edit]
- Preceded by: Solar eclipse of August 12, 2064
- Followed by: Solar eclipse of September 4, 2100
Inex[edit]
- Preceded by: Solar eclipse of September 12, 2053
- Followed by: Solar eclipse of August 4, 2111
Triad[edit]
- Preceded by: Solar eclipse of October 24, 1995
- Followed by: Solar eclipse of June 24, 2169
Solar eclipses of 2080–2083[edit]
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 July 15, 2083 occurs in the next lunar year eclipse set.
Solar eclipse series sets from 2080 to 2083 | ||||||
---|---|---|---|---|---|---|
Ascending node | Descending node | |||||
Saros | Map | Gamma | Saros | Map | Gamma | |
121 | March 21, 2080![]() Partial |
−1.0578 | 126 | September 13, 2080![]() Partial |
1.0723 | |
131 | March 10, 2081![]() Annular |
−0.3653 | 136 | September 3, 2081![]() Total |
0.3378 | |
141 | February 27, 2082![]() Annular |
0.3361 | 146 | August 24, 2082![]() Total |
−0.4004 | |
151 | February 16, 2083![]() Partial |
1.017 | 156 | August 13, 2083![]() Partial |
−1.2064 |
Saros 146[edit]
This eclipse is a part of Saros series 146, repeating every 18 years, 11 days, and containing 76 events. The series started with a partial solar eclipse on September 19, 1541. It contains total eclipses from May 29, 1938 through October 7, 2154; hybrid eclipses from October 17, 2172 through November 20, 2226; and annular eclipses from November 30, 2244 through August 10, 2659. The series ends at member 76 as a partial eclipse on December 29, 2893. 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 26 at 5 minutes, 21 seconds on June 30, 1992, and the longest duration of annularity will be produced by member 63 at 3 minutes, 30 seconds on August 10, 2659. All eclipses in this series occur at the Moon’s descending node of orbit.[2]
Series members 16–37 occur between 1801 and 2200: | ||
---|---|---|
16 | 17 | 18 |
![]() March 13, 1812 |
![]() March 24, 1830 |
![]() April 3, 1848 |
19 | 20 | 21 |
![]() April 15, 1866 |
![]() April 25, 1884 |
![]() May 7, 1902 |
22 | 23 | 24 |
![]() May 18, 1920 |
![]() May 29, 1938 |
![]() June 8, 1956 |
25 | 26 | 27 |
![]() June 20, 1974 |
![]() June 30, 1992 |
![]() July 11, 2010 |
28 | 29 | 30 |
![]() July 22, 2028 |
![]() August 2, 2046 |
![]() August 12, 2064 |
31 | 32 | 33 |
![]() August 24, 2082 |
![]() September 4, 2100 |
![]() September 15, 2118 |
34 | 35 | 36 |
![]() September 26, 2136 |
![]() October 7, 2154 |
![]() October 17, 2172 |
37 | ||
![]() October 29, 2190 |
Metonic series[edit]
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).
21 eclipse events between June 12, 2029, and June 12, 2105 | ||||
---|---|---|---|---|
June 11–12 | March 30–31 | January 16 | November 4–5 | August 23–24 |
118 | 120 | 122 | 124 | 126 |
![]() June 12, 2029 |
![]() March 30, 2033 |
![]() January 16, 2037 |
![]() November 4, 2040 |
![]() August 23, 2044 |
128 | 130 | 132 | 134 | 136 |
![]() June 11, 2048 |
![]() March 30, 2052 |
![]() January 16, 2056 |
![]() November 5, 2059 |
![]() August 24, 2063 |
138 | 140 | 142 | 144 | 146 |
![]() June 11, 2067 |
![]() March 31, 2071 |
![]() January 16, 2075 |
![]() November 4, 2078 |
![]() August 24, 2082 |
148 | 150 | 152 | 154 | |
![]() June 11, 2086 |
![]() March 31, 2090 |
![]() January 16, 2094 |
![]() November 4, 2097 |
Notes[edit]
- ^ 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 146". eclipse.gsfc.nasa.gov.
References[edit]
- Earth visibility chart and eclipse statistics Eclipse Predictions by Fred Espenak, NASA/GSFC