Solar eclipse of February 5, 1962
| Solar eclipse of February 5, 1962 | |
|---|---|
 Map | |
| Type of eclipse | |
| Nature | Total |
| Gamma | 0.2107 |
| Magnitude | 1.043 |
| Maximum eclipse | |
| Duration | 248 sec (4 m 8 s) |
| Coordinates | 4°12′S 178°06′E / 4.2°S 178.1°E |
| Max. width of band | 147 km (91 mi) |
| Times (UTC) | |
| Greatest eclipse | 0:12:38 |
| References | |
| Saros | 130 (49 of 73) |
| Catalog # (SE5000) | 9424 |
A total solar eclipse occurred on February 5, 1962. 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 total solar eclipse occurs when the Moon's apparent diameter is larger than the Sun's, blocking all direct sunlight, turning day into darkness. Totality occurs in a narrow path across Earth's surface, with the partial solar eclipse visible over a surrounding region thousands of kilometres wide.
Related eclipses
Solar eclipses of 1961-1964
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.
| Ascending node | Descending node | |||||
|---|---|---|---|---|---|---|
| Saros | Map | Saros | Map | |||
| 120 |  February 15, 1961 Total |
125 |  August 11, 1961 Annular | |||
| 130 | February 5, 1962 Total |
135 |  July 31, 1962 Annular | |||
| 140 |  January 25, 1963 Annular |
145 |  July 20, 1963 Total | |||
| 150 |  January 14, 1964 Partial |
155 |  July 9, 1964 Partial | |||
| Partial solar eclipses of June 10, 1964 and December 4, 1964 belong in the next lunar year set. | ||||||
Saros 130
It is a part of Saros cycle 130, repeating every 18 years, 11 days, containing 73 events. The series started with partial solar eclipse on August 20, 1096. It contains total eclipses from April 5, 1475 through July 18, 2232. The series ends at member 73 as a partial eclipse on October 25, 2394. The longest duration of totality was 6 minutes, 41 seconds on July 11, 1619.[1]
|
Series members 43-56 between 1853 and 2100
|
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).
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
References
- Earth visibility chart and eclipse statistics Eclipse Predictions by Fred Espenak, NASA/GSFC
- The Flash Spectrum Observed at the Total Eclipse of February 5, 1962, Publications of the Astronomical Society of Japan, vol. 21, p.141 (1969).
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