Solar eclipse of December 6, 2067
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| Solar eclipse of December 6, 2067 | |
|---|---|
Map
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| Type of eclipse | |
| Nature | Hybrid |
| Gamma | 0.2845 |
| Magnitude | 1.0011 |
| Maximum eclipse | |
| Duration | 8 sec (0 m 8 s) |
| Coordinates | Lua error in package.lua at line 80: module 'strict' not found. |
| Max. width of band | 4 km (2.5 mi) |
| Times (UTC) | |
| Greatest eclipse | 14:03:43 |
| References | |
| Saros | 143 (26 of 72) |
| Catalog # (SE5000) | 9659 |
A total solar eclipse will occur on December 6, 2067. It is a hybrid event, beginning and ending as an annular eclipse. 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.
Contents
Related eclipses
Solar eclipses 2065-2069
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.
| 118 | July 3, 2065 Partial |
123 | December 27, 2065 Partial |
| 128 | June 22, 2066 Annular |
133 | December 17, 2066 Total |
| 138 | June 11, 2067 Annular |
143 | December 6, 2067 Hybrid |
| 148 | May 31, 2068 Total |
153 | November 24, 2068 Partial |
| 158 | May 20, 2069 Partial |
Saros 143
It is a part of Saros cycle 143, repeating every 18 years, 11 days, containing 72 events. The series started with partial solar eclipse on March 7, 1617 and total event from June 24, 1797 through October 24, 1995. It has hybrid eclipses from November 3, 2013 through December 6, 2067, and annular eclipses from December 16, 2085 through September 16, 2536. The series ends at member 72 as a partial eclipse on April 23, 2873. The longest duration of totality was 3 minutes, 50 seconds on August 19, 1887.[1]
Series members 17-28 occur between 1901 and 2100:
| 17 | 18 | 19 |
|---|---|---|
 August 30, 1905 |
 September 10, 1923 |
 September 21, 1941 |
| 20 | 21 | 22 |
 October 2, 1959 |
 October 12, 1977 |
 October 24, 1995 |
| 23 | 24 | 25 |
 November 3, 2013 |
 November 14, 2031 |
 November 25, 2049 |
| 26 | 27 | 28 |
December 6, 2067 |
 December 16, 2085 |
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.
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) |
Notes
References
- Earth visibility chart and eclipse statistics Eclipse Predictions by Fred Espenak, NASA/GSFC
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