Solar eclipse of November 12, 1928

Solar eclipse of November 12, 1928
	Map
Type of eclipse
Nature	Partial
Gamma	1.0861
Magnitude	0.8078
Maximum eclipse
Coordinates	62.6°N 81.1°E
Times (UTC)
Greatest eclipse	9:48:24
References
Saros	122 (53 of 70)
Catalog # (SE5000)	9348

A partial solar eclipse occurred on November 12, 1928. 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 partial solar eclipse occurs in the polar regions of the Earth when the center of the Moon's shadow misses the Earth.

Related eclipses

Solar eclipses 1928–1931

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]

Solar eclipse series sets from 1928–1931
Ascending node		Descending node
117	May 19, 1928 Total (non-central)	122	November 12, 1928 Partial
127	May 9, 1929 Total	132	November 1, 1929 Annular
137	April 28, 1930 Hybrid	142	October 21, 1930 Total
147	April 18, 1931 Partial	152	October 11, 1931 Partial

Metonic series

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).

22 eclipse events, progressing from north to south between April 8, 1902 and August 31, 1989:
April 7–8	January 24–25	November 12	August 31-September 1	June 19–20
108			114	116
April 8, 1902			August 31, 1913	June 19, 1917
118	120	122	124	126
April 8, 1921	January 24, 1925	November 12, 1928	August 31, 1932	June 19, 1936
128	130	132	134	136
April 7, 1940	January 25, 1944	November 12, 1947	September 1, 1951	June 20, 1955
138	140	142	144	146
April 8, 1959	January 25, 1963	November 12, 1966	August 31, 1970	June 20, 1974
148	150	152	154
April 7, 1978	January 25, 1982	November 12, 1985	August 31, 1989

gollark: ```python>>> import sys>>> from ctypes import *>>> memmove(id(7), id(8), sys.getsizeof(7))140001623574848>>> 78```

gollark: Hold on.

gollark: Oh, I actually proved that 8 was 7 using Python ages ago.

gollark: > (gollark be quiet)But think of how many discoveries might be lost because of not being captured when binned?

gollark: Idea: automatic OCR systems in bins?

References

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.

External links

Earth visibility chart and eclipse statistics Eclipse Predictions by Fred Espenak, NASA/GSFC
- Google interactive map
- Besselian elements

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[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.