Solar_eclipse_of_September_2,_2035
Solar eclipse of September 2, 2035
Total eclipse
A total solar eclipse will occur on Sunday, 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.
| Solar eclipse of September 2, 2035 | |
|---|---|
| Type of eclipse | |
| Nature | Total |
| Gamma | 0.3727 |
| Magnitude | 1.032 |
| Maximum eclipse | |
| Duration | 174 s (2 min 54 s) |
| Coordinates | 29.1°N 158°E / 29.1; 158 |
| Max. width of band | 116 km (72 mi) |
| Times (UTC) | |
| Greatest eclipse | 1:56:46 |
| References | |
| Saros | 145 (23 of 77) |
| Catalog # (SE5000) | 9586 |
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]
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 to 2036 | ||||||
|---|---|---|---|---|---|---|
| Descending node | Ascending node | |||||
| 120 | March 30, 2033 Total |
125 | September 23, 2033 Partial | |||
| 130 | March 20, 2034 Total |
135 | 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. All eclipses in this series occurs at the Moon's ascending node.
| Series members 10–32 occur between 1801 and 2359 | ||
|---|---|---|
| 10 | 11 | 12 |
April 13, 1801 |
April 24, 1819 |
May 4, 1837 |
| 13 | 14 | 15 |
May 16, 1855 |
May 26, 1873 |
June 6, 1891 |
| 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 | 27 |
September 23, 2071 |
October 4, 2089 |
October 16, 2107 |
| 28 | 29 | 30 |
October 26, 2125 |
November 7, 2143 |
November 17, 2161 |
| 31 | 32 | 33 |
November 28, 2179 |
December 9, 2197 |
December 21, 2215 |
| 34 | 35 | 36 |
December 31, 2233 |
January 12, 2252 |
January 22, 2270 |
| 37 | 38 | 39 |
February 2, 2288 |
February 14, 2306 |
February 25, 2324 |
| 40 | ||
March 8, 2342 | ||
Inex series
This eclipse is a part of the long period inex cycle, repeating at alternating nodes, every 358 synodic months (≈ 10,571.95 days, or 29 years minus 20 days). Their appearance and longitude are irregular due to a lack of synchronization with the anomalistic month (period of perigee). However, groupings of 3 inex cycles (≈ 87 years minus 2 months) comes close (≈ 1,151.02 anomalistic months), so eclipses are similar in these groupings.
| Inex series members between 1901 and 2100: | ||
|---|---|---|
November 22, 1919 (Saros 141) |
November 1, 1948 (Saros 142) |
October 12, 1977 (Saros 143) |
September 22, 2006 (Saros 144) |
September 2, 2035 (Saros 145) |
August 12, 2064 (Saros 146) |
July 23, 2093 (Saros 147) |
||
Tritos series
This eclipse is a part of a tritos cycle, repeating at alternating nodes every 135 synodic months (≈ 3986.63 days, or 11 years minus 1 month). Their appearance and longitude are irregular due to a lack of synchronization with the anomalistic month (period of perigee), but groupings of 3 tritos cycles (≈ 33 years minus 3 months) come close (≈ 434.044 anomalistic months), so eclipses are similar in these groupings.
| Series members between 1901 and 2100 | |||
|---|---|---|---|
September 9, 1904 (Saros 133) |
August 10, 1915 (Saros 134) |
July 9, 1926 (Saros 135) | |
June 8, 1937 (Saros 136) |
May 9, 1948 (Saros 137) |
April 8, 1959 (Saros 138) | |
March 7, 1970 (Saros 139) |
February 4, 1981 (Saros 140) |
January 4, 1992 (Saros 141) | |
December 4, 2002 (Saros 142) |
November 3, 2013 (Saros 143) |
October 2, 2024 (Saros 144) | |
September 2, 2035 (Saros 145) |
August 2, 2046 (Saros 146) |
July 1, 2057 (Saros 147) | |
May 31, 2068 (Saros 148) |
May 1, 2079 (Saros 149) |
March 31, 2090 (Saros 150) | |
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 ascending node.
| 21 eclipse events between June 21, 1982, and June 21, 2058 | ||||
|---|---|---|---|---|
| June 21 | April 8–9 | January 26 | November 13–14 | September 1–2 |
| 107 | 109 | 111 | 113 | 115 |
| June 21, 1963 | April 9, 1967 | January 26, 1971 | November 14, 1974 | September 2, 1978 |
| 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 | ||||
The 2035 eclipse is the setting of the 2003 video game Castlevania: Aria of Sorrow. Dracula's castle is located inside the solar eclipse, having been sealed there in 1999.
- 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.
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