Solar eclipse of April 17, 1912 | |
---|---|
Type of eclipse | |
Nature | Hybrid |
Gamma | 0.528 |
Magnitude | 1.0003 |
Maximum eclipse | |
Duration | 2 s (0 min 2 s) |
Coordinates | 38°24′N 11°18′W / 38.4°N 11.3°W |
Max. width of band | 1 km (0.62 mi) |
Times (UTC) | |
Greatest eclipse | 11:34:22 |
References | |
Saros | 137 (30 of 70) |
Catalog # (SE5000) | 9308 |
A total solar eclipse occurred on April 17, 1912. It is a hybrid event, starting and ending as an annular eclipse, with only a small portion of totality. Totality was visible over the sea between Spain and France, with annularity continued northeast across Europe and Asia.
This eclipse occurred two days after the Titanic sunk in the northwestern Atlantic ocean under the darkness of new moon.[1]
The Observatory of Paris had the Globule balloon aloft for the 17 April 1912 hybrid eclipse by Camille Flammarion.[2]
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.[3]
Solar eclipse series sets from 1910 to 1913 | ||||
---|---|---|---|---|
Ascending node | Descending node | |||
117 | May 9, 1910![]() Total |
122 | November 2, 1910![]() Partial | |
127 | April 28, 1911![]() Total |
132 | October 22, 1911![]() Annular | |
137 | April 17, 1912![]() Hybrid |
142 | October 10, 1912![]() Total | |
147 | April 6, 1913![]() Partial |
152 | September 30, 1913![]() Partial |