Solar eclipse of June 22, 2085
| Solar eclipse of June 22, 2085 | |
|---|---|
 Map | |
| Type of eclipse | |
| Nature | Annular |
| Gamma | 0.0452 |
| Magnitude | 0.9704 |
| Maximum eclipse | |
| Duration | 209 s (3 min 29 s) |
| Coordinates | 26°12′N 131°18′E / 26.2°N 131.3°E |
| Max. width of band | 106 km (66 mi) |
| Times (UTC) | |
| Greatest eclipse | 3:21:16 |
| References | |
| Saros | 138 (35 of 70) |
| Catalog # (SE5000) | 9699 |
An annular solar eclipse will occur on June 22, 2085. 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[edit]
Solar eclipses 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]
| Solar eclipse series sets from 2083 to 2087 | ||||
|---|---|---|---|---|
| Descending node | Ascending node | |||
| 118 | July 15, 2083 Partial |
123 | January 7, 2084 Partial | |
| 128 | July 3, 2084 Annular |
133 | December 27, 2084 Total | |
| 138 | June 22, 2085 Annular |
143 | December 16, 2085 Annular | |
| 148 | June 11, 2086 Total |
153 | December 6, 2086 Partial | |
| 158 | June 1, 2087 Partial | |||
Saros 138[edit]
It is a part of Saros cycle 138, repeating every 18 years, 11 days, containing 70 events. The series started with partial solar eclipse on June 6, 1472. It contains annular eclipses from August 31, 1598 through February 18, 2482 with a hybrid eclipse on March 1, 2500. It has total eclipses from March 12, 2518 through April 3, 2554. The series ends at member 70 as a partial eclipse on July 11, 2716. The longest duration of totality will be only 56 seconds on April 3, 2554.
| Series members 25–35 occur between 1901 and 2100: | ||
|---|---|---|
| 25 | 26 | 27 |
 March 6, 1905 |
 March 17, 1923 |
 March 27, 1941 |
| 28 | 29 | 30 |
 April 8, 1959 |
 April 18, 1977 |
 April 29, 1995 |
| 31 | 32 | 33 |
 May 10, 2013 |
 May 21, 2031 |
 May 31, 2049 |
| 34 | 35 | |
 June 11, 2067 |
June 22, 2085 | |
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.
References[edit]
- Earth visibility chart and eclipse statistics Eclipse Predictions by Fred Espenak, NASA/GSFC
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