title: Solar eclipse of September 2, 2035
text: # Solar eclipse of September 2, 2035
  
  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.
  
  ## 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.
  
  ## 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.
  
  Solar eclipse series sets from 2033–2036 :
  
  | Descending node | Descending node | Ascending 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 |
  