| Solar eclipse of February 14, 1934 | |
|---|---|
 Map | |
| Type of eclipse | |
| Nature | Total |
| Gamma | 0.4868 |
| Magnitude | 1.0321 |
| Maximum eclipse | |
| Duration | 173 s (2 min 53 s) |
| Coordinates | 13°12′N 161°42′E / 13.2°N 161.7°E |
| Max. width of band | 123 km (76 mi) |
| Times (UTC) | |
| Greatest eclipse | 0:38:41 |
| References | |
| Saros | 139 (25 of 71) |
| Catalog # (SE5000) | 9360 |
A total solar eclipse occurred on February 14, 1934. 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. Totality was visible from the Dutch East Indies (today's Indonesia), North Borneo (now belonging to Malaysia), and the South Seas Mandate of Japan (the part now belonging to FS Micronesia).
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 1931 to 1935 | |||||
|---|---|---|---|---|---|
| Descending node | Ascending node | ||||
| 114 | September 12, 1931 Partial |
119 | March 7, 1932 Annular | ||
| 124 | August 31, 1932 Total |
129 | February 24, 1933 Annular | ||
| 134 | August 21, 1933 Annular |
139 | February 14, 1934 Total | ||
| 144 | August 10, 1934 Annular |
149 | February 3, 1935 Partial | ||
| 154 | July 30, 1935 Partial | ||||
This eclipse is a member of saros series 139, repeating every 18 years, 11 days, 8 hours, containing 71 events. The series started with partial solar eclipse on May 17, 1501. It contains hybrid eclipses on August 11, 1627, through to December 9, 1825; and total eclipses from December 21, 1843, through to March 26, 2601. The series ends at member 71 as a partial eclipse on July 3, 2763. 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 solar eclipse of June 13, 2132, will be the longest total solar eclipse since July 11, 1991, at 6 minutes, 55.02 seconds.
The longest duration of totality will be produced by member 39 at 7 minutes, 29.22 seconds on July 16, 2186.[2] After that date, the durations of totality will decrease until the series ends. This date is the longest solar eclipse computed between 4000 BC and AD 6000.[3] Saros series eclipses occur during the Moon's ascending node (a term related to our equator and polar-naming conventions).
| Series members 24–45 occur between 1901 and 2300 | ||
|---|---|---|
| 24 | 25 | 26 |
 February 3, 1916 |
February 14, 1934 |
 February 25, 1952 |
| 27 | 28 | 29 |
 March 7, 1970 |
 March 18, 1988 |
 March 29, 2006 |
| 30 | 31 | 32 |
 April 8, 2024 |
 April 20, 2042 |
 April 30, 2060 |
| 33 | 34 | 35 |
 May 11, 2078 |
 May 22, 2096 |
 June 3, 2114 |
| 36 | 37 | 38 |
 June 13, 2132 |
 June 25, 2150 |
 July 5, 2168 |
| 39 | 40 | 41 |
 July 16, 2186 |
 July 27, 2204 |
 August 8, 2222 |
| 42 | 43 | 44 |
 August 18, 2240 |
 August 29, 2258 |
 September 9, 2276 |
| 45 | ||
 September 20, 2294 | ||
.jpg)
