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Solar eclipse of December 26, 2019

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Solar eclipse of December 26, 2019
Annularity as seen from Jaffna, Sri Lanka
Map
Type of eclipse
NatureAnnular
Gamma0.4135
Magnitude0.9701
Maximum eclipse
Duration220 s (3 min 40 s)
Coordinates1°00′N 102°18′E / 1°N 102.3°E / 1; 102.3
Max. width of band118 km (73 mi)
Times (UTC)
Greatest eclipse5:18:53
References
Saros132 (46 of 71)
Catalog # (SE5000)9552

An annular solar eclipse will occur on December 26, 2019. 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. The annularity will be visible in Saudi Arabia, Qatar, United Arab Emirates, Oman, India, Sri Lanka, Malaysia, Indonesia, Singapore, Northern Mariana Islands, and Guam. Population centers in the path of the annularity include Kozhikode, Coimbatore, Jaffna, Trincomalee, Sibolga, Batam, Singapore, Singkawang and Guam. Cities such as Doha, Madurai, Pekanbaru, Dumai and Kuching will narrowly miss the annular path.

Images


Animated path

Astronomers Without Borders collected eclipse glasses for redistribution to Latin America and Asia for their 2019 eclipses from the Solar eclipse of August 21, 2017.[1]

Tzolkinex

Half-Saros cycle

Tritos

Solar Saros 132

Inex

Triad

  • Followed: Solar eclipse of October 26, 2106

Solar eclipses 2018-2021

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.[2]

The partial solar eclipses on February 15, 2018 and August 11, 2018 occur in the previous lunar year eclipse set.

Solar eclipse series sets from 2018 to 2021
Ascending node   Descending node
Saros Map Gamma Saros Map Gamma
117

Partial in Melbourne, Australia
July 13, 2018

Partial
−1.35423 122

Partial in Nakhodka, Russia
January 6, 2019

Partial
1.14174
127

Totality in La Serena, Chile
July 2, 2019

Total
−0.64656 132

Annularity in Jaffna, Sri Lanka
December 26, 2019

Annular
0.41351
137

Annularity in Beigang, Yunlin, Taiwan
June 21, 2020

Annular
0.12090 142

Totality in Gorbea, Chile
December 14, 2020

Total
−0.29394
147

Partial in Halifax, Canada
June 10, 2021

Annular
0.91516 152

From HMS Protector off South Georgia
December 4, 2021

Total
−0.95261

Saros 132

This eclipse is a part of Saros series 132, repeating every 18 years, 11 days, and containing 71 events. The series started with a partial solar eclipse on August 13, 1208. It contains annular eclipses from March 17, 1569 through March 12, 2146; hybrid eclipses on March 23, 2164 and April 3, 2182; 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. Its eclipses are tabulated in three columns; every third eclipse in the same column is one exeligmos apart, so they all cast shadows over approximately the same parts of the Earth.

The longest duration of annularity was produced by member 25 at 6 minutes, 56 seconds on May 9, 1641, and the longest duration of totality will be produced by member 61 at 2 minutes, 14 seconds on June 8, 2290. All eclipses in this series occur at the Moon’s descending node of orbit.[3]

Series members 34–56 occur between 1801 and 2200:
34 35 36

August 17, 1803

August 27, 1821

September 7, 1839
37 38 39

September 18, 1857

September 29, 1875

October 9, 1893
40 41 42

October 22, 1911

November 1, 1929

November 12, 1947
43 44 45

November 23, 1965

December 4, 1983

December 14, 2001
46 47 48

December 26, 2019

January 5, 2038

January 16, 2056
49 50 51

January 27, 2074

February 7, 2092

February 18, 2110
52 53 54

March 1, 2128

March 12, 2146

March 23, 2164
55 56

April 3, 2182

April 14, 2200

Metonic series

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 descending node.

21 eclipse events between May 21, 1993 and May 20, 2069
May 20–21 March 9 December 25–26 October 13–14 August 1–2
118 120 122 124 126

May 21, 1993

March 9, 1997

December 25, 2000

October 14, 2004

August 1, 2008
128 130 132 134 136

May 20, 2012

March 9, 2016

December 26, 2019

October 14, 2023

August 2, 2027
138 140 142 144 146

May 21, 2031

March 9, 2035

December 26, 2038

October 14, 2042

August 2, 2046
148 150 152 154 156

May 20, 2050

March 9, 2054

December 26, 2057

October 13, 2061

August 2, 2065
158

May 20, 2069

Notes

  1. ^ Cooper, Gael (2017-08-22). "Wait! Dig those eclipse glasses out of the garbage Here comes the sun. Astronomers Without Borders will be collecting the protective eyewear for use in future eclipses worldwide". Retrieved 2017-08-27.
  2. ^ 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.
  3. ^ "NASA - Catalog of Solar Eclipses of Saros 132". eclipse.gsfc.nasa.gov.

References