Solar eclipse of December 17, 2066 | |
---|---|
Type of eclipse | |
Nature | Total |
Gamma | −0.4043 |
Magnitude | 1.0416 |
Maximum eclipse | |
Duration | 194 s (3 min 14 s) |
Coordinates | 47°24′S175°48′E / 47.4°S 175.8°E |
Max. width of band | 152 km (94 mi) |
Times (UTC) | |
Greatest eclipse | 0:23:40 |
References | |
Saros | 133 (48 of 72) |
Catalog # (SE5000) | 9657 |
A total solar eclipse will occur on Friday, December 17, 2066. 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.
This total eclipse follows a similar path to the eclipse on December 25–26, 2038.
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 to 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 |
Solar Saros 133, repeating every 18 years, 11 days, contains 72 events. The series started with a partial solar eclipse on July 13, 1219. It contains annular eclipses from November 20, 1435, through January 13, 1526, with a hybrid eclipse on January 24, 1544. It has total eclipses from February 3, 1562, through June 21, 2373. The series ends at member 72 as a partial eclipse on September 5, 2499. The longest duration of totality was 6 minutes, 49.97 seconds on August 7, 1850. [2] The total eclipses of this saros series are getting shorter and farther south with each iteration. All eclipses in this series occurs at the Moon’s ascending node.
Series members 30–56 occur between 1742 and 2211 | ||
---|---|---|
30 | 31 | 32 |
June 3, 1742 | June 13, 1760 | June 24, 1778 |
33 | 34 | 35 |
July 4, 1796 | July 17, 1814 | July 27, 1832 |
36 | 37 | 38 |
August 7, 1850 | August 18, 1868 | August 29, 1886 |
39 | 40 | 41 |
September 9, 1904 | September 21, 1922 | October 1, 1940 |
42 | 43 | 44 |
October 12, 1958 | October 23, 1976 | November 3, 1994 |
45 | 46 | 47 |
November 13, 2012 | November 25, 2030 | December 5, 2048 |
48 | 49 | 50 |
December 17, 2066 | December 27, 2084 | January 8, 2103 |
51 | 52 | 53 |
January 19, 2121 | January 30, 2139 | February 9, 2157 |
54 | 55 | 56 |
February 21, 2175 | March 3, 2193 | March 15, 2211 |
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 29, 1903 (Saros 118) | February 25, 1914 (Saros 119) | January 24, 1925 (Saros 120) | |
December 25, 1935 (Saros 121) | November 23, 1946 (Saros 122) | October 23, 1957 (Saros 123) | |
September 22, 1968 (Saros 124) | August 22, 1979 (Saros 125) | July 22, 1990 (Saros 126) | |
June 21, 2001 (Saros 127) | May 20, 2012 (Saros 128) | April 20, 2023 (Saros 129) | |
March 20, 2034 (Saros 130) | February 16, 2045 (Saros 131) | January 16, 2056 (Saros 132) | |
December 17, 2066 (Saros 133) | November 15, 2077 (Saros 134) | October 14, 2088 (Saros 135) | |
September 14, 2099 (Saros 136) |
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