Solar eclipse of September 2, 2035
Solar eclipse of September 2, 2035 | |
---|---|
Map | |
Type of eclipse | |
Nature | Total |
Gamma | 0.3727 |
Magnitude | 1.032 |
Maximum eclipse | |
Duration | 174 sec (2 m 54 s) |
Coordinates | 29°06′N 158°00′E / 29.1°N 158°E |
Max. width of band | 116 km (72 mi) |
Times (UTC) | |
Greatest eclipse | 1:56:46 |
References | |
Saros | 145 (23 of 77) |
Catalog # (SE5000) | 9586 |
A total solar eclipse will occur on September 2, 2035. 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.
Visibility
The path of totality will cross two Asian capital cities, Beijing, China and Pyongyang, North Korea, and will pass north of a third, Tokyo, Japan.[1]
Related eclipses
Solar eclipses of 2033-2036
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.[2]
Solar eclipse series sets from 2033-2036 | ||||||
---|---|---|---|---|---|---|
Descending node | Ascending node | |||||
120 | March 30, 2033 Total |
125 | September 23, 2033 Partial | |||
130 | March 20, 2034 Total |
136 | September 12, 2034 Annular | |||
140 | March 9, 2035 Annular |
145 | September 2, 2035 Total | |||
150 | February 27, 2036 Partial |
155 | August 21, 2036 Partial | |||
A partial solar eclipse on July 23, 2036 occurs in the next lunar year eclipse set. |
Saros 145
This solar eclipse is a part of Saros cycle 145, repeating every 18 years, 11 days, 8 hours, containing 77 events. The series started with a partial solar eclipse on January 4, 1639, and reached a first annular eclipse on June 6, 1891. It was a hybrid event on June 17, 1909, and total eclipses from June 29, 1927, through September 9, 2648. The series ends at member 77 as a partial eclipse on April 17, 3009. The longest eclipse will occur on June 25, 2522, with a maximum duration of totality of 7 minutes, 12 seconds.[3]
Series members 16–26 occur between 1901 and 2100 | ||
---|---|---|
16 | 17 | 18 |
June 17, 1909 |
June 29, 1927 |
July 9, 1945 |
19 | 20 | 21 |
July 20, 1963 |
July 31, 1981 |
August 11, 1999 |
22 | 23 | 24 |
August 21, 2017 |
September 2, 2035 |
September 12, 2053 |
25 | 26 | |
September 23, 2071 |
October 4, 2089 |
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).
21 eclipse events between June 21, 1982, and June 21, 2058 | ||||
---|---|---|---|---|
June 21 | April 8-9 | January 26 | November 13-14 | September 1-2 |
117 | 119 | 121 | 123 | 125 |
June 21, 1982 |
April 9, 1986 |
January 26, 1990 |
November 13, 1993 |
September 2, 1997 |
127 | 129 | 131 | 133 | 135 |
June 21, 2001 |
April 8, 2005 |
January 26, 2009 |
November 13, 2012 |
September 1, 2016 |
137 | 139 | 141 | 143 | 145 |
June 21, 2020 |
April 8, 2024 |
January 26, 2028 |
November 14, 2031 |
September 2, 2035 |
147 | 149 | 151 | 153 | 155 |
June 21, 2039 |
April 9, 2043 |
January 26, 2047 |
November 14, 2050 |
September 2, 2054 |
157 | ||||
June 21, 2058 |
References
- ↑ Kennedy, Kelsey (August 21, 2017). "If You Missed This Year's Eclipse, Chase Another". Atlas Obscura. Retrieved December 12, 2017.
- ↑ 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.
- ↑ Espenak, Fred (September 26, 2009). "Statistics for Solar Eclipses of Saros 145". NASA. Archived from the original on September 30, 2009.
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