Solar eclipse of March 6, 1905

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Solar eclipse of March 6, 1905
SE1905Mar06A.png
Map
Type of eclipse
NatureAnnular
Gamma-0.5768
Magnitude0.9269
Maximum eclipse
Duration478 sec (7 m 58 s)
Coordinates39°30′S 117°24′E / 39.5°S 117.4°E / -39.5; 117.4
Max. width of band334 km (208 mi)
Times (UTC)
Greatest eclipse5:12:26
References
Saros138 (25 of 70)
Catalog # (SE5000)9292

An annular solar eclipse occurred on March 6, 1905. 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. Annularity was visible from Heard Island and McDonald Islands (now an Australian external territory), Australia, New Caledonia, and New Hebrides (now Vanuatu).

Related eclipses[edit]

Solar eclipses 1902-1907[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.[1]

Saros 138[edit]

It is a part of Saros cycle 138, repeating every 18 years, 11 days, containing 70 events. The series started with partial solar eclipse on June 6, 1472. It contains annular eclipses from August 31, 1598 through February 18, 2482 with a hybrid eclipse on March 1, 2500. It has total eclipses from March 12, 2518 through April 3, 2554. The series ends at member 70 as a partial eclipse on July 11, 2716. The longest duration of totality will be only 56 seconds on April 3, 2554.


Notes[edit]

  1. ^ 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.

References[edit]