Solar eclipse of November 23, 1965
| Solar eclipse of November 23, 1965 | |
|---|---|
| Type of eclipse | |
| Nature | Annular |
| Gamma | 0.3906 |
| Magnitude | 0.9656 |
| Maximum eclipse | |
| Duration | 4m 2s |
| Coordinates | 1.7N 119.8E |
| Max. width of band | 134 km |
| Times (UTC) | |
| Greatest eclipse | 4:14:51 |
| References | |
| Saros | 132 (43 of 71) |
| Catalog # (SE5000) | 9433 |
An annual solar eclipse occurred on November 23, 1965. A solar eclipse occurs when the Moon passes between Earth and the Sun, thereby totally or partially 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, 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 thousands of kilometres wide.
Contents |
Related eclipses [edit]
Solar eclipses of 1964-1967 [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.
Note: Partial solar eclipses on January 14, 1964 and July 9, 1964 belong to the previous lunar year set.
| Ascending node | Descending node | |||
|---|---|---|---|---|
| Saros | Map | Saros | Map | |
| 117 | June 10, 1964 Partial |
122 | December 4, 1964 Partial |
|
| 127 | May 30, 1965 Total |
132 | November 23, 1965 Annular |
|
| 137 | May 20, 1966 Annular |
142 | November 12, 1966 Total |
|
| 147 | May 9, 1967 Partial |
152 | November 2, 1967 Total |
|
Saros 132 [edit]
It 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 4 minutes, 2 seconds on 1965 Nov 23, and totality will be 2 minutes, 14 seconds on May 27, 2272.[1]
Series members 40-50 occur between 1901 and 2100:
| 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 |
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).
This series has 22 eclipse events between September 12, 1931 and July 1, 2011.
| September 11-12 | June 30-July 1 | April 18-19 | February 4-5 | November 22-23 |
|---|---|---|---|---|
| 114 | 116 | 118 | 120 | 122 |
September 12, 1931 |
June 30, 1935 |
April 19, 1939 |
February 4, 1943 |
November 23, 1946 |
| 124 | 126 | 128 | 130 | 132 |
September 12, 1950 |
June 30, 1954 |
April 19, 1958 |
February 5, 1962 |
November 23, 1965 |
| 134 | 136 | 138 | 140 | 142 |
September 11, 1969 |
June 30, 1973 |
April 18, 1977 |
February 4, 1981 |
November 22, 1984 |
| 144 | 146 | 148 | 150 | 152 |
September 11, 1988 |
June 30, 1992 |
April 17, 1996 |
February 5, 2000 |
November 23, 2003 |
| 154 | 156 | |||
September 11, 2007 |
July 1, 2011 |
Notes [edit]
References [edit]
- Earth visibility chart and eclipse statistics Eclipse Predictions by Fred Espenak, NASA/GSFC
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