Solar eclipse of September 11, 1969
| Solar eclipse of September 11, 1969 | |
|---|---|
 Map | |
| Type of eclipse | |
| Nature | Annular |
| Gamma | 0.2201 |
| Magnitude | 0.969 |
| Maximum eclipse | |
| Duration | 191 sec (3 m 11 s) |
| Coordinates | 15°36′N 114°06′W / 15.6°N 114.1°W |
| Max. width of band | 114 km (71 mi) |
| Times (UTC) | |
| Greatest eclipse | 19:58:59 |
| References | |
| Saros | 134 (41 of 71) |
| Catalog # (SE5000) | 9441 |
An annular solar eclipse occurred on September 11, 1969. 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.
Related eclipses
Solar eclipses of 1968-1971
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 | |||
| 119 |  March 28, 1968 Partial |
124 |  September 22, 1968 Total | |||
| 129 |  March 18, 1969 Annular |
134 | September 11, 1969 Annular | |||
| 139 |  March 7, 1970 Total |
144 |  August 31, 1970 Annular | |||
| 149 |  February 25, 1971 Partial |
154 |  August 20, 1971 Partial | |||
| A partial solar eclipse of July 22, 1971 occurs in the next lunar year set. | ||||||
Saros 134
It is a part of Saros cycle 134, repeating every 18 years, 11 days, containing 71 events. The series started with partial solar eclipse on June 22, 1248. It contains total eclipses from October 9, 1428 through December 24, 1554 and hybrid eclipses from January 3, 1573 through June 27, 1843, and annular eclipses from July 8, 1861 through May 21, 2384. The series ends at member 71 as a partial eclipse on August 6, 2510. The longest duration of totality was 1 minutes, 30 seconds on October 9, 1428.[1]
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.
 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) |
Notess
References
- Earth visibility chart and eclipse statistics Eclipse Predictions by Fred Espenak, NASA/GSFC
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