Solar eclipse of March 6, 1905

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Solar eclipse of March 6, 1905
SE1905Mar06A.png
Map
Type of eclipse
Nature Annular
Gamma -0.5768
Magnitude 0.9269
Maximum eclipse
Duration 7m 58s
Coordinates 39.5S 117.4E
Max. width of band 334 km
Times (UTC)
Greatest eclipse 5:12:26
References
Saros 138 (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.

Related eclipses[edit]

Solar eclipses 1902-1907[edit]

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.

Solar eclipse series sets from 1902-1907
Descending node   Ascending node
108 April 8, 1902
SE1902Apr08P.png
Partial
118 March 29, 1903
SE1903Mar29A.png
Annular
123 September 21, 1903
SE1903Sep21T.png
Total
128 March 17, 1904
SE1904Mar17A.png
Annular
133 September 9, 1904
SE1904Sep09T.png
Total
138 March 6, 1905
SE1905Mar06A.png
Annular
143 August 30, 1905
SE1905Aug30T.png
Total
148 February 23, 1906
SE1906Feb23P.png
Partial
153 August 20, 1906
SE1906Aug20P.png
Partial

Notes[edit]

References[edit]