Solar Eclipse Of 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).

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 / 13.2; 161.7
Max. width of band	123 km (76 mi)
Times (UTC)
Greatest eclipse	0:38:41
References
Saros	139 (25 of 71)
Catalog # (SE5000)	9360

Solar eclipses 1931–1935

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.

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

Saros 139

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. 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. 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