Solar eclipse of June 13, 2094
| Solar eclipse of June 13, 2094 | |
|---|---|
| Type of eclipse | |
| Nature | Partial |
| Gamma | -1.4613 |
| Magnitude | 0.1618 |
| Maximum eclipse | |
| Coordinates | 10°30′S 39°00′E / 10.5°S 39°E Fatal error: The format of the coordinate could not be determined. Parsing failed. |
| Max. width of band | 142 km (88 mi) |
| Times (UTC) | |
| Greatest eclipse | 0:22:11 |
| References | |
| Saros | 119 (70 of 71) |
| Catalog # (SE5000) | 9719 |
A partial solar eclipse will occur on June 12–13, 2094. 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 partial solar eclipse occurs in the polar regions of the Earth when the center of the Moon's shadow misses the Earth. In the west of the International Date Line it is June 12 local time.
Related eclipses
Solar eclipses 2094–2098
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]
| 119 | June 13, 2094 File:SE2094Jun13P.png Partial |
124 | December 7, 2094 File:SE2094Dec07P.png Partial |
| 129 | June 2, 2095 File:SE2095Jun02T.png Total |
134 | November 27, 2095 File:SE2095Nov27A.png Annular |
| 139 | May 22, 2096 File:SE2096May22T.png Total |
144 | November 15, 2096 File:SE2096Nov15A.png Annular |
| 149 | May 11, 2097 File:SE2097May11T.png Total |
154 | November 4, 2097 File:SE2097Nov04A.png Annular |
| 164 | October 24, 2098 File:SE2098Oct24P.png Partial |
Saros 119
It is a part of Saros cycle 119, repeating every 18 years, 11 days, containing 71 events. The series started with a partial solar eclipse on May 15, 850 AD. It contains total eclipses on August 9, 994 AD and August 20, 1012, with a hybrid eclipse on August 31, 1030. It has annular eclipses from September 10, 1048 through March 18, 1950. The series ends at member 71 as a partial eclipse on June 24, 2112. The longest duration of totality was only 32 seconds on August 20, 1012. The longest duration of annularity was 7 minutes, 37 seconds on September 1, 1625. The longest duration of hybridity was only 18 seconds on August 31, 1030.
| Series members 54–70 occur between 1801 and 2100: | ||
|---|---|---|
| 54 | 55 | 56 |
| File:SE1805Dec21A.gif December 21, 1805 |
File:SE1824Jan01A.gif January 1, 1824 |
File:SE1842Jan11A.gif January 11, 1842 |
| 57 | 58 | 59 |
| File:SE1860Jan23A.gif January 23, 1860 |
File:SE1878Feb02A.gif February 2, 1878 |
February 13, 1896 |
| 60 | 61 | 62 |
| File:SE1914Feb25A.png February 25, 1914 |
File:SE1932Mar07A.png March 7, 1932 |
File:SE1950Mar18A.png March 18, 1950 |
| 63 | 64 | 65 |
| File:SE1968Mar28P.png March 28, 1968 |
File:SE1986Apr09P.png April 9, 1986 |
File:SE2004Apr19P.png April 19, 2004 |
| 66 | 67 | 68 |
| File:SE2022Apr30P.png April 30, 2022 |
File:SE2040May11P.png May 11, 2040 |
File:SE2058May22P.png May 22, 2058 |
| 69 | 70 | |
| File:SE2076Jun01P.png June 1, 2076 |
File:SE2094Jun13P.png June 13, 2094 | |
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.
External links
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