Solar eclipse of June 11, 2086
Solar eclipse of June 11, 2086 | |
---|---|
Type of eclipse | |
Nature | Total |
Gamma | −0.7215 |
Magnitude | 1.0174 |
Maximum eclipse | |
Duration | 108 s (1 min 48 s) |
Coordinates | 23°12′S 12°30′E / 23.2°S 12.5°E |
Max. width of band | 86 km (53 mi) |
Times (UTC) | |
Greatest eclipse | 11:07:14 |
References | |
Saros | 148 (25 of 75) |
Catalog # (SE5000) | 9701 |
A total solar eclipse will occur at the Moon's descending node of orbit on Tuesday, June 11, 2086, with a magnitude of 1.0174. 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 2086[edit]
- A partial lunar eclipse on May 28, 2086.
- A total solar eclipse on June 11, 2086.
- A partial lunar eclipse on November 20, 2086.
- A partial solar eclipse on December 6, 2086.
Metonic[edit]
- Preceded by: Solar eclipse of August 24, 2082
- Followed by: Solar eclipse of March 31, 2090
Tzolkinex[edit]
- Preceded by: Solar eclipse of May 1, 2079
- Followed by: Solar eclipse of July 23, 2093
Half-Saros[edit]
- Preceded by: Lunar eclipse of June 6, 2077
- Followed by: Lunar eclipse of June 17, 2095
Tritos[edit]
- Preceded by: Solar eclipse of July 13, 2075
- Followed by: Solar eclipse of May 11, 2097
Solar Saros 148[edit]
- Preceded by: Solar eclipse of May 31, 2068
- Followed by: Solar eclipse of June 22, 2104
Inex[edit]
- Preceded by: Solar eclipse of July 1, 2057
- Followed by: Solar eclipse of May 24, 2115
Triad[edit]
- Preceded by: Solar eclipse of August 11, 1999
- Followed by: Solar eclipse of April 12, 2173
Solar eclipses of 2083–2087[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 eclipses on February 16, 2083 and August 13, 2083 occur in the previous lunar year eclipse set, and the partial solar eclipses on May 2, 2087 and October 26, 2087 occur in the next lunar year eclipse set.
Solar eclipse series sets from 2083 to 2087 | ||||||
---|---|---|---|---|---|---|
Descending node | Ascending node | |||||
Saros | Map | Gamma | Saros | Map | Gamma | |
118 | July 15, 2083![]() Partial |
1.5465 | 123 | January 7, 2084![]() Partial |
−1.0715 | |
128 | July 3, 2084![]() Annular |
0.8208 | 133 | December 27, 2084![]() Total |
−0.4094 | |
138 | June 22, 2085![]() Annular |
0.0452 | 143 | December 16, 2085![]() Annular |
0.2786 | |
148 | June 11, 2086![]() Total |
−0.7215 | 153 | December 6, 2086![]() Partial |
1.0194 | |
158 | June 1, 2087![]() Partial |
−1.4186 |
Saros 148[edit]
This eclipse is a part of Saros series 148, repeating every 18 years, 11 days, and containing 75 events. The series started with a partial solar eclipse on September 21, 1653. It contains annular eclipses on April 29, 2014 and May 9, 2032; a hybrid eclipse on May 20, 2050; and total eclipses from May 31, 2068 through August 3, 2771. The series ends at member 75 as a partial eclipse on December 12, 2987. 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 22 at 22 seconds (by default) on May 9, 2032, and the longest duration of totality will be produced by member 54 at 5 minutes, 23 seconds on April 26, 2609. All eclipses in this series occur at the Moon’s descending node of orbit.[2]
Series members 10–31 occur between 1801 and 2200: | ||
---|---|---|
10 | 11 | 12 |
![]() December 30, 1815 |
![]() January 9, 1834 |
![]() January 21, 1852 |
13 | 14 | 15 |
![]() January 31, 1870 |
![]() February 11, 1888 |
![]() February 23, 1906 |
16 | 17 | 18 |
![]() March 5, 1924 |
![]() March 16, 1942 |
![]() March 27, 1960 |
19 | 20 | 21 |
![]() April 7, 1978 |
![]() April 17, 1996 |
![]() April 29, 2014 |
22 | 23 | 24 |
![]() May 9, 2032 |
![]() May 20, 2050 |
![]() May 31, 2068 |
25 | 26 | 27 |
![]() June 11, 2086 |
![]() June 22, 2104 |
![]() July 4, 2122 |
28 | 29 | 30 |
![]() July 14, 2140 |
![]() July 25, 2158 |
![]() August 4, 2176 |
31 | ||
![]() August 16, 2194 |
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 148". eclipse.gsfc.nasa.gov.
References[edit]
- Earth visibility chart and eclipse statistics Eclipse Predictions by Fred Espenak, NASA/GSFC