Solar eclipse of November 1, 1929
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| Solar eclipse of November 1, 1929 | |
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| Type of eclipse | |
| Nature | Annular |
| Gamma | 0.3514 |
| Magnitude | 0.9649 |
| Maximum eclipse | |
| Duration | 234 sec (3 m 54 s) |
| Coordinates | Lua error in package.lua at line 80: module 'strict' not found. |
| Max. width of band | 134 km (83 mi) |
| Times (UTC) | |
| Greatest eclipse | 12:05:10 |
| References | |
| Saros | 132 (41 of 71) |
| Catalog # (SE5000) | 9350 |
An annual solar eclipse occurred on November 1, 1929. 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 1928-1931
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 | |||
|---|---|---|---|---|
| 117 | May 19, 1928 Total |
122 | November 12, 1928 150px Partial |
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| 127 | May 9, 1929 150px Total |
132 | November 1, 1929 150px Annular |
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| 137 | April 28, 1930 150px Hybrid |
142 | October 21, 1930 Total |
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| 147 | April 18, 1931 150px Partial |
152 | October 11, 1931 150px Partial |
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Saros 132
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 6 minutes, 56 seconds on May 9, 1641, and totality will be 2 minutes, 14 seconds on June 8, 2290.[1]
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Series members 40-50 occur between 1901 and 2100:
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Notes
References
- Earth visibility chart and eclipse statistics Eclipse Predictions by Fred Espenak, NASA/GSFC
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