Solar eclipse of February 17, 2064 | |
---|---|
Type of eclipse | |
Nature | Annular |
Gamma | 0.3597 |
Magnitude | 0.9262 |
Maximum eclipse | |
Duration | 536 sec (8 m 56 s) |
Coordinates | 7°00′N69°42′E / 7°N 69.7°E |
Max. width of band | 295 km (183 mi) |
Times (UTC) | |
Greatest eclipse | 7:00:23 |
References | |
Saros | 141 (26 of 70) |
Catalog # (SE5000) | 9650 |
An annular solar eclipse will occur on February 17, 2064. 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. An annular solar eclipse occurs when the Moon's apparent diameter is smaller than the Sun's, blocking most of the Sun's light and causing the Sun to look like an annulus (ring). An annular eclipse appears as a partial eclipse over a region of the Earth thousands of kilometres wide.
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]
121 | March 11, 2062 Partial | 126 | September 3, 2062 Partial |
131 | February 28, 2063 Annular | 136 | August 24, 2063 Total |
141 | February 17, 2064 Annular | 146 | August 12, 2064 Total |
151 | February 5, 2065 Partial | 156 | August 2, 2065 Partial |
Solar saros 141, repeating every about 18 years, 11 days, and 8 hours, contains 70 events. The series started with partial solar eclipse on May 19, 1613. It contains 41 annular eclipses from August 4, 1739, to October 14, 2460. There are no total eclipses in this series. The series ends at member 70 as a partial eclipse on June 13, 2857. The longest annular eclipse occurred on December 14, 1955, with maximum duration of annularity at 12 minutes and 9 seconds. All eclipses in this series occur at the Moon’s ascending node. [2]
Series members 17–36 occur between 1901 and 2259 | ||
---|---|---|
17 | 18 | 19 |
November 11, 1901 | November 22, 1919 | December 2, 1937 |
20 | 21 | 22 |
December 14, 1955 | December 24, 1973 | January 4, 1992 |
23 | 24 | 25 |
January 15, 2010 | January 26, 2028 | February 5, 2046 |
26 | 27 | 28 |
February 17, 2064 | February 27, 2082 | March 10, 2100 |
29 | 30 | 31 |
March 22, 2118 | April 1, 2136 | April 12, 2154 |
32 | 33 | 34 |
April 23, 2172 | May 4, 2190 | May 15, 2208 |
35 | 36 | |
May 27, 2226 | June 6, 2244 |
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: | ||
---|---|---|
May 29, 1919 (Saros 136) | May 9, 1948 (Saros 137) | April 18, 1977 (Saros 138) |
March 29, 2006 (Saros 139) | March 9, 2035 (Saros 140) | February 17, 2064 (Saros 141) |
January 27, 2093 (Saros 142) |
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 13, 2018 and July 12, 2094 | ||||
---|---|---|---|---|
July 12–13 | April 30-May 1 | February 16–17 | December 5–6 | September 22–23 |
117 | 119 | 121 | 123 | 125 |
July 13, 2018 | April 30, 2022 | February 17, 2026 | December 5, 2029 | September 23, 2033 |
127 | 129 | 131 | 133 | 135 |
July 13, 2037 | April 30, 2041 | February 16, 2045 | December 5, 2048 | September 22, 2052 |
137 | 139 | 141 | 143 | 145 |
July 12, 2056 | April 30, 2060 | February 17, 2064 | December 6, 2067 | September 23, 2071 |
147 | 149 | 151 | 153 | 155 |
July 13, 2075 | May 1, 2079 | February 16, 2083 | December 6, 2086 | September 23, 2090 |
157 | ||||
July 12, 2094 |
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