Solar eclipse of February 14, 1915
| Solar eclipse of February 14, 1915 | |
|---|---|
 Map | |
| Type of eclipse | |
| Nature | Annular |
| Gamma | -0.2024 |
| Magnitude | 0.9789 |
| Maximum eclipse | |
| Duration | 124 sec (2 m 4 s) |
| Coordinates | 24°00′S 120°42′E / 24°S 120.7°E |
| Max. width of band | 77 km (48 mi) |
| Times (UTC) | |
| Greatest eclipse | 4:33:20 |
| References | |
| Saros | 129 (46 of 80) |
| Catalog # (SE5000) | 9315 |
An annular solar eclipse occurred on February 14, 1915. 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.
Related eclipses
Solar eclipses of 1913-1917
Each member 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.
| Descending node | Ascending node | |||
|---|---|---|---|---|
| 114 | August 31, 1913 Partial |
119 | February 25, 1914 Annular | |
| 124 | August 21, 1914 Total |
129 | February 14, 1915 Annular | |
| 134 | August 10, 1915 Annular |
139 | February 3, 1916 Total | |
| 144 | July 30, 1916 Annular |
149 | January 23, 1917 Partial | |
| 154 | July 19, 1917 Partial | |||
Saros 129
It is a part of Saros cycle 129, repeating every 18 years, 11 days, containing 80 events. The series started with partial solar eclipse on October 3, 1103. It contains annular eclipses on May 6, 1464 through March 18, 1969, hybrid eclipses on April 8, 2005 and April 20, 2023 and total eclipses from April 30, 2041 through July 26, 2185. The series ends at member 80 as a partial eclipse on February 21, 2528. The longest duration of totality was 3 minutes, 43 seconds on June 25, 2131 .[1]
| Series members 46-56 occur between 1901 and 2100: | ||
|---|---|---|
| 46 | 47 | 48 |
February 14, 1915 |
 February 24, 1933 |
 March 7, 1951 |
| 49 | 50 | 51 |
 March 18, 1969 |
 March 29, 1987 |
 April 8, 2005 |
| 52 | 53 | 54 |
 April 20, 2023 |
 April 30, 2041 |
 May 11, 2059 |
| 55 | 56 | |
 May 22, 2077 |
 June 2, 2095 | |
Tritos series
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 17, 1904 (Saros 128) |
February 14, 1915 (Saros 129) |
 January 14, 1926 (Saros 130) | |
 December 13, 1936 (Saros 131) |
 November 12, 1947 (Saros 132) |
 October 12, 1958 (Saros 133) | |
 September 11, 1969 (Saros 134) |
 August 10, 1980 (Saros 135) |
 July 11, 1991 (Saros 136) | |
 June 10, 2002 (Saros 137) |
 May 10, 2013 (Saros 138) |
 April 8, 2024 (Saros 139) | |
 March 9, 2035 (Saros 140) |
 February 5, 2046 (Saros 141) |
 January 5, 2057 (Saros 142) | |
 December 6, 2067 (Saros 143) |
 November 4, 2078 (Saros 144) |
 October 4, 2089 (Saros 145) | |
 September 4, 2100 (Saros 146) |
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Notes
References
- Earth visibility chart and eclipse statistics Eclipse Predictions by Fred Espenak, NASA/GSFC
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