Solar eclipse of June 17, 1909
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′N 123°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.
Related eclipses[edit]
Eclipses in 1909[edit]
- A total lunar eclipse on June 4, 1909.
- A hybrid solar eclipse on June 17, 1909.
- A total lunar eclipse on November 27, 1909.
- A partial solar eclipse on December 12, 1909.
Metonic[edit]
- Preceded by: Solar eclipse of August 30, 1905
- Followed by: Solar eclipse of April 6, 1913
Tzolkinex[edit]
- Preceded by: Solar eclipse of May 7, 1902
- Followed by: Solar eclipse of July 30, 1916
Half-Saros[edit]
- Preceded by: Lunar eclipse of June 13, 1900
- Followed by: Lunar eclipse of June 24, 1918
Tritos[edit]
- Preceded by: Solar eclipse of July 18, 1898
- Followed by: Solar eclipse of May 18, 1920
Solar Saros 145[edit]
- Preceded by: Solar eclipse of June 6, 1891
- Followed by: Solar eclipse of June 29, 1927
Inex[edit]
- Preceded by: Solar eclipse of July 7, 1880
- Followed by: Solar eclipse of May 29, 1938
Triad[edit]
- Preceded by: Solar eclipse of August 16, 1822
- Followed by: Solar eclipse of April 17, 1996
Solar eclipses of 1906–1909[edit]
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 |
Saros 145[edit]
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 |
External links[edit]
- ^ "First eclipse of sun for this year today". Knoxville Sentinel. Knoxville, Tennessee. 1909-06-17. p. 4. Retrieved 2023-11-01 – via Newspapers.com.
- ^ Frederic J. Haskin (1909-06-17). "Eclipse of the sun". The Salt Lake Herald. Salt Lake City, Utah. p. 4. Retrieved 2023-11-01 – via Newspapers.com.
- ^ "Today's shadow of the sun scarcely visible in this region". Daily News-Republican. Lawton, Oklahoma. 1909-06-17. p. 1. Retrieved 2023-11-01 – via Newspapers.com.
- ^ van Gent, R.H. "Solar- and Lunar-Eclipse Predictions from Antiquity to the Present". A Catalogue of Eclipse Cycles. Utrecht University. Retrieved 6 October 2018.
- ^ "NASA - Catalog of Solar Eclipses of Saros 145". eclipse.gsfc.nasa.gov.
- Earth visibility chart and eclipse statistics Eclipse Predictions by Fred Espenak, NASA/GSFC