Solar eclipse of January 16, 2094
A total solar eclipse will occur on January 16, 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 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.
| Solar eclipse of January 16, 2094 | |
|---|---|
![]() Map  | |
| Type of eclipse | |
| Nature | Total | 
| Gamma | −0.9333 | 
| Magnitude | 1.0342 | 
| Maximum eclipse | |
| Duration | 111 sec (1 m 51 s) | 
| Coordinates | 84.8°S 10.6°W | 
| Max. width of band | 329 km (204 mi) | 
| Times (UTC) | |
| Greatest eclipse | 18:59:03 | 
| References | |
| Saros | 152 (17 of 70) | 
| Catalog # (SE5000) | 9718 | 
This total eclipse is notable in that the path of totality passes over the South Pole.
Related eclipses
    
    Solar eclipses 2091–2094
    
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 eclipses 2091–2094 | |||||
|---|---|---|---|---|---|
| 122 | February 18, 2091![]() Partial  | 
127 | August 15, 2091![]() Total  | ||
| 132 | February 7, 2092![]() Annular  | 
137 | August 3, 2092![]() Annular  | ||
| 142 | January 27, 2093![]() Total  | 
147 | July 23, 2093![]() Annular  | ||
| 152 | January 16, 2094![]() Total  | 
157 | July 12, 2094![]() Partial  | ||
Saros 152
    
Solar saros 152, repeating every about 18 years and 11 days, contains 70 events. The series started with a partial solar eclipse on July 26, 1805. It has total eclipses from November 2, 1967, to September 14, 2490; hybrid eclipses from September 26, 2508, to October 17, 2544; and annular eclipses from October 29, 2562, to June 16, 2941. The series ends at member 70 as a partial eclipse on August 20, 3049. The longest total eclipse will occur on June 9, 2328, at 5 minutes and 15 seconds; the longest annular eclipse will occur on February 16, 2743, at 5 minutes and 20 seconds.[2]
| Series members 7–17 occur between 1901 and 2100: | ||
|---|---|---|
| 7 | 8 | 9 | 
  September 30, 1913  | 
  October 11, 1931  | 
  October 21, 1949  | 
| 10 | 11 | 12 | 
  November 2, 1967  | 
  November 12, 1985  | 
  November 23, 2003  | 
| 13 | 14 | 15 | 
  December 4, 2021  | 
  December 15, 2039  | 
  December 26, 2057  | 
| 16 | 17 | |
  January 6, 2076  | 
  January 16, 2094  | |
Metonic cycle
    
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
    
- 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.
 - Saros Series Catalog of Solar Eclipses NASA Eclipse Web Site.
 
References
    
- Earth visibility chart and eclipse statistics Eclipse Predictions by Fred Espenak, NASA/GSFC
 - NASA graphics
 




































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