Solar eclipse of December 6, 2067

Summary

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.

Solar eclipse of December 6, 2067
Map
Type of eclipse
NatureHybrid
Gamma0.2845
Magnitude1.0011
Maximum eclipse
Duration8 s (0 min 8 s)
Coordinates6°00′S 32°24′W / 6°S 32.4°W / -6; -32.4
Max. width of band4 km (2.5 mi)
Times (UTC)
Greatest eclipse14:03:43
References
Saros143 (26 of 72)
Catalog # (SE5000)9659

Related eclipses edit

Solar eclipses 2065–2069 edit

This eclipse is a member of a semester series. An eclipse 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.[1]

Solar eclipse series sets from 2065 to 2069
Descending node   Ascending node
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 edit

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. All eclipses in this series occurs at the Moon’s ascending node.

Series members 17–28 occur between 1741 and 2100
8 9 10
 
May 23, 1743
 
June 3, 1761
 
June 14, 1779
11 12 13
 
June 24, 1797
 
July 6, 1815
 
July 17, 1833
14 15 16
 
July 28, 1851
 
August 7, 1869
 
August 19, 1887
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 edit

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 1801 and 2100
 
December 21, 1805
(Saros 119)
 
November 19, 1816
(Saros 120)
 
October 20, 1827
(Saros 121)
 
September 18, 1838
(Saros 122)
 
August 18, 1849
(Saros 123)
 
July 18, 1860
(Saros 124)
 
June 18, 1871
(Saros 125)
 
May 17, 1882
(Saros 126)
 
April 16, 1893
(Saros 127)
 
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)

In the 22nd century:

  • Solar saros 147: annular solar eclipse of August 4, 2111
  • Solar saros 148: total solar eclipse of July 4, 2122
  • Solar saros 149: total solar eclipse of June 3, 2133
  • Solar saros 150: annular solar eclipse of May 3, 2144
  • Solar saros 151: annular solar eclipse of April 2, 2155
  • Solar saros 152: total solar eclipse of March 2, 2166
  • Solar saros 153: annular solar eclipse of January 29, 2177
  • Solar saros 154: annular solar eclipse of December 29, 2187
  • Solar saros 155: total solar eclipse of November 28, 2198

In the 23rd century:

  • Solar saros 156: annular solar eclipse of October 29, 2209
  • Solar saros 157: annular solar eclipse of September 27, 2220
  • Solar saros 158: total solar eclipse of August 28, 2231
  • Solar saros 159: partial solar eclipse of July 28, 2242
  • Solar saros 160: partial solar eclipse of June 26, 2253
  • Solar saros 161: partial solar eclipse of May 26, 2264
  • Solar saros 162: partial solar eclipse of April 26, 2275
  • Solar saros 163: partial solar eclipse of March 25, 2286
  • Solar saros 164: partial solar eclipse of February 22, 2297

Metonic series edit

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). All eclipses in this table occur at the Moon's ascending node.

Notes edit

  1. ^ van Gent, R.H. "Solar- and Lunar-Eclipse Predictions from Antiquity to the Present". A Catalogue of Eclipse Cycles. Utrecht University. Retrieved 6 October 2018.

References edit

  • Earth visibility chart and eclipse statistics Eclipse Predictions by Fred Espenak, NASA/GSFC
    • Google interactive map
    • Besselian elements