Solar eclipse of November 12, 1947

An annular solar eclipse occurred on November 12, 1947. 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 the Pacific Ocean, Peru, Ecuador, Colombia and Brazil.

Solar eclipse of November 12, 1947
Map
Type of eclipse
Nature	Annular
Gamma	0.3743
Magnitude	0.965
Maximum eclipse
Duration	239 sec (3 m 59 s)
Coordinates	3°N 117.4°W
Max. width of band	135 km (84 mi)
Times (UTC)
Greatest eclipse	20:05:37
References
Saros	132 (42 of 71)
Catalog # (SE5000)	9393

Related eclipses

Solar eclipses of 1946–1949

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 1946–1949

Ascending node			Descending node
117	May 30, 1946 Partial		122	November 23, 1946 Partial
127	May 20, 1947 Total		132	November 12, 1947 Annular
137	May 9, 1948 Annular		142	November 1, 1948 Total
147	April 28, 1949 Partial		152	October 21, 1949 Partial

Saros 132

This eclipse is a part of Saros cycle 132, repeating every 18 years, 11 days, containing 71 events. The series started with partial solar eclipse on August 13, 1208. It contains annular eclipses from March 17, 1569 through March 12, 2146, hybrid on March 23, 2164 and April 3, 2183 and total eclipses from April 14, 2200 through June 19, 2308. The series ends at member 71 as a partial eclipse on September 25, 2470. The longest duration of annular was 6 minutes, 56 seconds on May 9, 1641, and totality will be 2 minutes, 14 seconds on June 8, 2290. All eclipses in this series occurs at the Moon’s descending node.

Series members 28–50 occur between 1690 and 2100:
28	29	30
June 11, 1695	June 22, 1713	July 4, 1731
31	32	33
July 14, 1749	July 25, 1767	August 5, 1785
34	35	36
August 17, 1803	August 27, 1821	September 7, 1839
37	38	39
September 18, 1857	September 29, 1875	October 9, 1893
40	41	42
October 22, 1911	November 1, 1929	November 12, 1947
43	44	45
November 23, 1965	December 4, 1983	December 14, 2001
46	47	48
December 26, 2019	January 5, 2038	January 16, 2056
49	50
January 27, 2074	February 7, 2092

Tritos series

This eclipse is a part of a tritos cycle, repeating at alternating nodes every 135 synodic months (≈ 3986.63 days, or 11 years minus 1 month). Their appearance and longitude are irregular due to a lack of synchronization with the anomalistic month (period of perigee), but groupings of 3 tritos cycles (≈ 33 years minus 3 months) come close (≈ 434.044 anomalistic months), so eclipses are similar in these groupings.

Series members between 1801 and 2100
December 21, 1805 (Saros 119)	November 19, 1816 (Saros 120)	October 20, 1827 (Saros 121)
September 18, 1838 (Saros 122)	August 18, 1849 (Saros 123)	July 18, 1860 (Saros 124)
June 18, 1871 (Saros 125)	May 17, 1882 (Saros 126)	April 16, 1893 (Saros 127)
March 17, 1904 (Saros 128)	February 14, 1915 (Saros 129)	January 14, 1926 (Saros 130)
December 13, 1936 (Saros 131)	November 12, 1947 (Saros 132)	October 12, 1958 (Saros 133)
September 11, 1969 (Saros 134)	August 10, 1980 (Saros 135)	July 11, 1991 (Saros 136)
June 10, 2002 (Saros 137)	May 10, 2013 (Saros 138)	April 8, 2024 (Saros 139)
March 9, 2035 (Saros 140)	February 5, 2046 (Saros 141)	January 5, 2057 (Saros 142)
December 6, 2067 (Saros 143)	November 4, 2078 (Saros 144)	October 4, 2089 (Saros 145)
September 4, 2100 (Saros 146)

In the 22nd century:

• Solar Saros 147: Annular Solar Eclipse of 2111 Aug 04
• Solar Saros 148: Total Solar Eclipse of 2122 Jul 04
• Solar Saros 149: Total Solar Eclipse of 2133 Jun 03
• Solar Saros 150: Annular Solar Eclipse of 2144 May 03
• Solar Saros 151: Annular Solar Eclipse of 2155 Apr 02
• Solar Saros 152: Total Solar Eclipse of 2166 Mar 02
• Solar Saros 153: Annular Solar Eclipse of 2177 Jan 29
• Solar Saros 154: Annular Solar Eclipse of 2187 Dec 29
• Solar Saros 155: Total Solar Eclipse of 2198 Nov 28

In the 23rd century:

• Solar Saros 156: Annular Solar Eclipse of 2209 Oct 29
• Solar Saros 157: Annular Solar Eclipse of 2220 Sep 27
• Solar Saros 158: Total Solar Eclipse of 2231 Aug 28
• Solar Saros 159: Partial Solar Eclipse of 2242 Jul 28
• Solar Saros 160: Partial Solar Eclipse of 2253 Jun 26
• Solar Saros 161: Partial Solar Eclipse of 2264 May 26
• Solar Saros 162: Partial Solar Eclipse of 2275 Apr 26
• Solar Saros 163: Partial Solar Eclipse of 2286 Mar 25
• Solar Saros 164: Partial Solar Eclipse of 2297 Feb 22

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

Notes

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

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