Solar eclipse of June 17, 1909 | |
---|---|
Type of eclipse | |
Nature | Hybrid |
Gamma | 0.8957 |
Magnitude | 1.0065 |
Maximum eclipse | |
Duration | 24 s (0 min 24 s) |
Coordinates | 82°54′N123°36′E / 82.9°N 123.6°E |
Max. width of band | 51 km (32 mi) |
Times (UTC) | |
Greatest eclipse | 23:18:38 |
References | |
Saros | 145 (16 of 77) |
Catalog # (SE5000) | 9302 |
A total solar eclipse occurred at the Moon's ascending node of orbit on Thursday, June 17, 1909, [1] [2] [3] with a magnitude of 1.0065. It was a hybrid event, with only a fraction of its path as total, and longer sections at the start and end as an annular eclipse. 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.
The path of totality crossed central Russia, the Arctic Ocean, northeastern Ellesmere Island in Canada, Greenland, and annularity crossed southern Siberia in Russia (now in northeastern Kazakhstan and southern Russia) and southern Greenland.
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. [4]
The partial solar eclipses on February 23, 1906 and August 20, 1906 occur in the previous lunar year eclipse set.
Solar eclipse series sets from 1906 to 1909 | ||||||
---|---|---|---|---|---|---|
Ascending node | Descending node | |||||
Saros | Map | Gamma | Saros | Map | Gamma | |
115 | July 21, 1906 Partial | −1.3637 | 120 | January 14, 1907 Total | 0.8628 | |
125 | July 10, 1907 Annular | −0.6313 | 130 | January 3, 1908 Total | 0.1934 | |
135 | June 28, 1908 Annular | 0.1389 | 140 | December 23, 1908 Hybrid | −0.4985 | |
145 | June 17, 1909 Hybrid | 0.8957 | 150 | December 12, 1909 Partial | −1.2456 |
This eclipse is a part of Saros series 145, repeating every 18 years, 11 days, and containing 77 events. The series started with a partial solar eclipse on January 4, 1639. It contains an annular eclipse on June 6, 1891; a hybrid eclipse 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. Its eclipses are tabulated in three columns; every third eclipse in the same column is one exeligmos apart, so they all cast shadows over approximately the same parts of the Earth.
The longest duration of annularity was produced by member 15 at 6 seconds (by default) on June 6, 1891, and the longest duration of totality will be produced by member 50 at 7 minutes, 12 seconds on June 25, 2522. All eclipses in this series occur at the Moon’s ascending node of orbit. [5]
Series members 10–32 occur between 1801 and 2200: | ||
---|---|---|
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 | |
November 28, 2179 | December 9, 2197 |
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.
The partial solar eclipse on November 4, 2116 (part of Saros 164) is also a part of this series but is not included in the table below.
Series members between 1801 and 2029 | ||||
---|---|---|---|---|
March 24, 1811 (Saros 136) | February 21, 1822 (Saros 137) | January 20, 1833 (Saros 138) | December 21, 1843 (Saros 139) | November 20, 1854 (Saros 140) |
October 19, 1865 (Saros 141) | September 17, 1876 (Saros 142) | August 19, 1887 (Saros 143) | July 18, 1898 (Saros 144) | June 17, 1909 (Saros 145) |
May 18, 1920 (Saros 146) | April 18, 1931 (Saros 147) | March 16, 1942 (Saros 148) | February 14, 1953 (Saros 149) | January 14, 1964 (Saros 150) |
December 13, 1974 (Saros 151) | November 12, 1985 (Saros 152) | October 12, 1996 (Saros 153) | September 11, 2007 (Saros 154) | August 11, 2018 (Saros 155) |
July 11, 2029 (Saros 156) |
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.
25 eclipse events between April 5, 1837 and June 17, 1928 | ||||
---|---|---|---|---|
April 5–6 | January 22–23 | November 10–11 | August 28–30 | June 17–18 |
107 | 109 | 111 | 113 | 115 |
April 5, 1837 | January 22, 1841 | November 10, 1844 | August 28, 1848 | June 17, 1852 |
117 | 119 | 121 | 123 | 125 |
April 5, 1856 | January 23, 1860 | November 11, 1863 | August 29, 1867 | June 18, 1871 |
127 | 129 | 131 | 133 | 135 |
April 6, 1875 | January 22, 1879 | November 10, 1882 | August 29, 1886 | June 17, 1890 |
137 | 139 | 141 | 143 | 145 |
April 6, 1894 | January 22, 1898 | November 11, 1901 | August 30, 1905 | June 17, 1909 |
147 | 149 | 151 | 153 | 155 |
April 6, 1913 | January 23, 1917 | November 10, 1920 | August 30, 1924 | June 17, 1928 |
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