A total solar eclipse will take place on Monday, January 6, 2076. 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.
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Related eclipses
Solar eclipses 2073–2076
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]
| 122 | February 7, 2073 Partial |
127 | August 3, 2073 Total |
| 132 | January 27, 2074 Annular |
137 | July 24, 2074 Annular |
| 142 | January 16, 2075 Total |
147 | July 13, 2075 Annular |
| 152 | January 6, 2076 Total |
157 | July 1, 2076 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 series
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). All eclipses in this table occur at the Moon's descending node.
| 21 eclipse events between June 1, 2011 and June 1, 2087 | ||||
|---|---|---|---|---|
| May 31 – June 1 | March 19–20 | January 5–6 | October 24–25 | August 12–13 |
| 118 | 120 | 122 | 124 | 126 |
 June 1, 2011 |
 March 20, 2015 |
 January 6, 2019 |
 October 25, 2022 |
 August 12, 2026 |
| 128 | 130 | 132 | 134 | 136 |
 June 1, 2030 |
 March 20, 2034 |
 January 5, 2038 |
 October 25, 2041 |
 August 12, 2045 |
| 138 | 140 | 142 | 144 | 146 |
 May 31, 2049 |
 March 20, 2053 |
 January 5, 2057 |
 October 24, 2060 |
 August 12, 2064 |
| 148 | 150 | 152 | 154 | 156 |
 May 31, 2068 |
 March 19, 2072 |
January 6, 2076 |
 October 24, 2079 |
 August 13, 2083 |
| 158 | 160 | 162 | 164 | 166 |
 June 1, 2087 |
 October 24, 2098 |
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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
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This page was last edited on 1 August 2021, at 12:49