Solar eclipse of April 19, 1958

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Solar eclipse of April 19, 1958
SE1958Apr19A.png
Map
Type of eclipse
Nature Annular
Gamma 0.275
Magnitude 0.9408
Maximum eclipse
Duration 427 sec (7 m 7 s)
Coordinates 26°30′N 123°36′E / 26.5°N 123.6°E / 26.5; 123.6
Max. width of band 228 km (142 mi)
Times (UTC)
Greatest eclipse 3:27:17
References
Saros 128 (55 of 73)
Catalog # (SE5000) 9416

An annular solar eclipse occurred on April 19, 1958. 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 of 1957–1960[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 1957–1960
Descending node   Ascending node
Saros Map Saros Map
118 SE1957Apr30A.png
April 30, 1957
Annular
123 SE1957Oct23T.png
October 23, 1957
Total
128 SE1958Apr19A.png
April 19, 1958
Annular
133 SE1958Oct12T.png
October 12, 1958
Total
138 SE1959Apr08A.png
April 8, 1959
Annular
143 SE1959Oct02T.png
October 2, 1959
Total
148 SE1960Mar27P.png
March 27, 1960
Partial
153 SE1960Sep20P.png
September 20, 1960
Partial

Saros 128[edit]

It is a part of Saros cycle 128, repeating every 18 years, 11 days, containing 73 events. The series started with partial solar eclipse on August 29, 984 AD. It contains total eclipses from May 16, 1417 through June 18, 1471 and hybrid eclipses from June 28, 1489 through July 31, 1543. Then it progresses into annular eclipses from August 11, 1561 through July 25, 2120. The series ends at member 73 as a partial eclipse on November 1, 2282. The longest duration of totality was 1 minutes, 45 seconds on June 7, 1453.[1]

Metonic series[edit]

The metonic series repeats eclipses every 19 years (6939.69 days), lasting about 5 cycles. Eclipses occur in nearly the same calendar date. In addition the octon subseries repeats 1/5 of that or every 3.8 years (1387.94 days).

Notes[edit]

References[edit]