| Solar eclipse of January 14, 1926 | |
|---|---|
|
Map
|
|
| Type of eclipse | |
| Nature | Total |
| Gamma | 0.1973 |
| Magnitude | 1.043 |
| Maximum eclipse | |
| Duration | 4m 11s |
| Coordinates | 10.1S 82.3E |
| Max. width of band | 147 km |
| Times (UTC) | |
| Greatest eclipse | 6:36:58 |
| References | |
| Saros | 130 (47 of 73) |
| Catalog # (SE5000) | 9341 |
A total solar eclipse occurred on January 14, 1926. 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. A total solar eclipse occurs when the Moon's apparent diameter is larger than the Sun, blocking all direct sunlight, turning day into darkness. Totality occurs in a narrow path across the surface of the Earth, while a partial solar eclipse will be visible over a region thousands of kilometres wide.
Contents |
This set of solar eclipses repeat approximately every 177 days and 4 hours at alternating nodes of the moon's orbit.
| Ascending node | Descending node | |||
|---|---|---|---|---|
| 115 | July 31, 1924 Partial |
120 | January 24, 1925 Total |
|
| 125 | July 20, 1925 Annular |
130 | January 14, 1926 Total |
|
| 135 | July 9, 1926 Annular |
140 | January 3, 1927 Annular |
|
| 145 | June 29, 1927 Total |
150 | December 24, 1927 Partial |
|
| 155 | June 17, 1928 Partial |
|||
It is a part of Saros cycle 130, repeating every 18 years, 11 days, containing 71 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 71 as a partial eclipse on October 25, 2394. The longest duration of totality was 6 minutes, 37 seconds on June 30, 1601.[1]
Series members 46-56 occur between 1901 and 2100:
| 46 | 47 | 48 |
|---|---|---|
January 3, 1908 |
January 14, 1926 |
January 25, 1944 |
| 49 | 50 | 51 |
February 5, 1962 |
February 16, 1980 |
February 26, 1998 |
| 52 | 53 | 54 |
March 9, 2016 |
March 20, 2034 |
March 30, 2052 |
| 55 | 56 | |
April 11, 2070 |
April 21, 2088 |
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 synchonization 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 1901 and 2100 are:
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) |
