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Solar eclipse of December 5, 2048

From Wikipedia, the free encyclopedia

Solar eclipse of December 5, 2048
Map
Type of eclipse
NatureTotal
Gamma−0.3973
Magnitude1.044
Maximum eclipse
Duration208 s (3 min 28 s)
Coordinates46°06′S 56°24′W / 46.1°S 56.4°W / -46.1; -56.4
Max. width of band160 km (99 mi)
Times (UTC)
Greatest eclipse15:35:27
References
Saros133 (47 of 72)
Catalog # (SE5000)9616

A total solar eclipse will occur on Saturday, December 5, 2048. 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. A total solar eclipse occurs when the Moon's apparent diameter is larger than the Sun's, blocking all direct sunlight and turning day into darkness. Totality occurs in a narrow path across Earth's surface, with the partial solar eclipse visible over a surrounding region spanning thousands of kilometres.

Animated Path

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Transcription

Related eclipses

Solar eclipses of 2047–2050

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]

Note: Partial lunar eclipses on January 26, 2047 and July 22, 2047 occur on the previous lunar year eclipse set.

Solar eclipse sets from 2047 to 2050
Descending node   Ascending node
118 June 23, 2047

Partial
123 December 16, 2047

Partial
128 June 11, 2048

Annular
133 December 5, 2048

Total
138 May 31, 2049

Annular
143 November 25, 2049

Hybrid
148 May 20, 2050

Hybrid
153 November 14, 2050

Partial

Tritos

Tzolkinex

Saros 133

Solar Saros 133, repeating every 18 years, 11 days, contains 72 events. The series started with a partial solar eclipse on July 13, 1219. It contains annular eclipses from November 20, 1435, through January 13, 1526, with a hybrid eclipse on January 24, 1544. It has total eclipses from February 3, 1562, through June 21, 2373. The series ends at member 72 as a partial eclipse on September 5, 2499. The longest duration of totality was 6 minutes, 49.97 seconds on August 7, 1850.[2] The total eclipses of this saros series are getting shorter and farther south with each iteration. All eclipses in this series occurs at the Moon’s ascending node.

Series members 30–56 occur between 1742 and 2211
30 31 32
June 3, 1742 June 13, 1760

June 24, 1778
33 34 35
July 4, 1796 July 17, 1814 July 27, 1832
36 37 38
August 7, 1850

August 18, 1868

August 29, 1886
39 40 41

September 9, 1904

September 21, 1922

October 1, 1940
42 43 44

October 12, 1958

October 23, 1976

November 3, 1994
45 46 47

November 13, 2012

November 25, 2030

December 5, 2048
48 49 50

December 17, 2066

December 27, 2084

January 8, 2103
51 52 53

January 19, 2121

January 30, 2139

February 9, 2157
54 55 56

February 21, 2175

March 3, 2193

March 15, 2211

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 ascending node.

References

  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.
  2. ^ http://eclipse.gsfc.nasa.gov/SEsaros/SEsaros133.html

External links

This page was last edited on 21 May 2024, at 15:41
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