Solar eclipse of November 24, 2068 | |
---|---|
Type of eclipse | |
Nature | Partial |
Gamma | 1.0299 |
Magnitude | 0.9109 |
Maximum eclipse | |
Coordinates | 68°30′N131°06′W / 68.5°N 131.1°W |
Times (UTC) | |
Greatest eclipse | 21:32:30 |
References | |
Saros | 153 (12 of 70) |
Catalog # (SE5000) | 9661 |
A partial solar eclipse will occur on November 24, 2068. 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 partial solar eclipse occurs in the polar regions of the Earth when the center of the Moon's shadow misses the Earth.
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 eclipse series sets from 2065–2069 | ||||
---|---|---|---|---|
Descending node | Ascending node | |||
118 | July 3, 2065 Partial | 123 | December 27, 2065 Partial | |
128 | June 22, 2066 Annular | 133 | December 17, 2066 Total | |
138 | June 11, 2067 Annular | 143 | December 6, 2067 Hybrid | |
148 | May 31, 2068 Total | 153 | November 24, 2068 Partial | |
158 | May 20, 2069 Partial |
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 | |||
---|---|---|---|
March 6, 1905 (Saros 138) | February 3, 1916 (Saros 139) | January 3, 1927 (Saros 140) | |
December 2, 1937 (Saros 141) | November 1, 1948 (Saros 142) | October 2, 1959 (Saros 143) | |
August 31, 1970 (Saros 144) | July 31, 1981 (Saros 145) | June 30, 1992 (Saros 146) | |
May 31, 2003 (Saros 147) | April 29, 2014 (Saros 148) | March 29, 2025 (Saros 149) | |
February 27, 2036 (Saros 150) | January 26, 2047 (Saros 151) | December 26, 2057 (Saros 152) | |
November 24, 2068 (Saros 153) | October 24, 2079 (Saros 154) | September 23, 2090 (Saros 155) |
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, progressing from south to north between July 1, 2000 and July 1, 2076 | ||||
---|---|---|---|---|
July 1–2 | April 19–20 | February 5–7 | November 24–25 | September 12–13 |
117 | 119 | 121 | 123 | 125 |
July 1, 2000 | April 19, 2004 | February 7, 2008 | November 25, 2011 | September 13, 2015 |
127 | 129 | 131 | 133 | 135 |
July 2, 2019 | April 20, 2023 | February 6, 2027 | November 25, 2030 | September 12, 2034 |
137 | 139 | 141 | 143 | 145 |
July 2, 2038 | April 20, 2042 | February 5, 2046 | November 25, 2049 | September 12, 2053 |
147 | 149 | 151 | 153 | 155 |
July 1, 2057 | April 20, 2061 | February 5, 2065 | November 24, 2068 | September 12, 2072 |
157 | 159 | 161 | 163 | 165 |
July 1, 2076 |
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