Solar eclipse of November 19, 1816

Solar eclipse of November 19, 1816
Map
Type of eclipse
NatureTotal
Gamma0.8408
Magnitude1.0233
Maximum eclipse
Duration120 s (2 min 0 s)
Coordinates35°00′N 41°30′E / 35°N 41.5°E / 35; 41.5
Max. width of band144 km (89 mi)
Times (UTC)
Greatest eclipse10:17:23
References
Saros120 (50 of 71)
Catalog # (SE5000)9081

A total solar eclipse occurred at the Moon's descending node of orbit on Tuesday, November 19, 1816, with a magnitude of 1.0233. 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, turning day into darkness. Totality occurs in a narrow path across Earth's surface, with the partial solar eclipse visible over a surrounding region thousands of kilometres wide. Occurring about 1.7 days before perigee (on November 17, 1816, at 17:10 UTC), the Moon's apparent diameter was larger.[1]

The path of totality was visible from parts of modern-day Norway, Sweden, Poland, western Ukraine, Romania, Turkey, Syria, Iraq, Iran, Afghanistan, Pakistan, northern India, and western China. A partial solar eclipse was also visible for parts of Europe, North Africa, Northeast Africa, the Middle East, Central Asia, and South Asia.

Observations

From Germany, this total eclipse could not be seen with clouded sky except by few observers at Pomerania only.[2]

Capel Lofft observed this eclipse from Ipswich.[3]

Eclipse details

Shown below are two tables displaying details about this particular solar eclipse. The first table outlines times at which the moon's penumbra or umbra attains the specific parameter, and the second table describes various other parameters pertaining to this eclipse.[4]

November 19, 1816 Solar Eclipse Times
Event Time (UTC)
First Penumbral External Contact 1816 November 19 at 08:01:46.3 UTC
First Umbral External Contact 1816 November 19 at 09:20:18.4 UTC
First Central Line 1816 November 19 at 09:21:02.3 UTC
First Umbral Internal Contact 1816 November 19 at 09:21:46.7 UTC
Equatorial Conjunction 1816 November 19 at 09:47:11.3 UTC
Ecliptic Conjunction 1816 November 19 at 10:08:45.7 UTC
Greatest Eclipse 1816 November 19 at 10:17:22.4 UTC
Greatest Duration 1816 November 19 at 10:17:35.6 UTC
Last Umbral Internal Contact 1816 November 19 at 11:13:19.6 UTC
Last Central Line 1816 November 19 at 11:14:01.9 UTC
Last Umbral External Contact 1816 November 19 at 11:14:43.9 UTC
Last Penumbral External Contact 1816 November 19 at 12:33:14.9 UTC
November 19, 1816 Solar Eclipse Parameters
Parameter Value
Eclipse Magnitude 1.02326
Eclipse Obscuration 1.04707
Gamma 0.84075
Sun Right Ascension 15h38m54.9s
Sun Declination -19°30'48.2"
Sun Semi-Diameter 16'11.7"
Sun Equatorial Horizontal Parallax 08.9"
Moon Right Ascension 15h40m03.9s
Moon Declination -18°42'56.6"
Moon Semi-Diameter 16'25.6"
Moon Equatorial Horizontal Parallax 1°00'17.2"
ΔT 12.2 s

Eclipse season

See also: Eclipse cycle

This eclipse is part of an eclipse season, a period, roughly every six months, when eclipses occur. Only two (or occasionally three) eclipse seasons occur each year, and each season lasts about 35 days and repeats just short of six months (173 days) later; thus two full eclipse seasons always occur each year. Either two or three eclipses happen each eclipse season. In the sequence below, each eclipse is separated by a fortnight.

Eclipse season of November–December 1816
November 19
Descending node (new moon)
 December 4
Ascending node (full moon)
Total solar eclipse
Solar Saros 120		 Partial lunar eclipse
Lunar Saros 132

Eclipses in 1816

Metonic

Tzolkinex

Half-Saros

Tritos

Solar Saros 120

Inex

Triad

Solar eclipses of 1816–1819

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.[5]

The partial solar eclipses on March 25, 1819 and September 19, 1819 occur in the next lunar year eclipse set.

Solar eclipse series sets from 1816 to 1819
Ascending node   Descending node
Saros Map Gamma Saros Map Gamma
115 May 27, 1816

Annular 		−0.9492 120 November 19, 1816

Total 		0.8408
125 May 16, 1817

Annular 		−0.2049 130 November 9, 1817

Total 		0.1487
135 May 5, 1818

Annular 		0.5440 140 October 29, 1818

Total 		−0.5524
145 April 24, 1819

Partial 		1.2579 150 October 19, 1819

Partial 		−1.3226

Saros 120

This eclipse is a part of Saros series 120, repeating every 18 years, 11 days, and containing 71 events. The series started with a partial solar eclipse on May 27, 933 AD. It contains annular eclipses from August 11, 1059 through April 26, 1492; hybrid eclipses from May 8, 1510 through June 8, 1564; and total eclipses from June 20, 1582 through March 30, 2033. The series ends at member 71 as a partial eclipse on July 7, 2195. 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 11 at 6 minutes, 24 seconds on September 11, 1113, and the longest duration of totality was produced by member 60 at 2 minutes, 50 seconds on March 9, 1997. All eclipses in this series occur at the Moon’s descending node of orbit.[6]

Series members 50–71 occur between 1801 and 2195:
50 51 52

November 19, 1816
November 30, 1834
December 11, 1852
53 54 55

December 22, 1870
January 1, 1889
January 14, 1907
56 57 58

January 24, 1925
February 4, 1943
February 15, 1961
59 60 61

February 26, 1979
March 9, 1997
March 20, 2015
62 63 64

March 30, 2033
April 11, 2051
April 21, 2069
65 66 67

May 2, 2087
May 14, 2105
May 25, 2123
68 69 70

June 4, 2141
June 16, 2159
June 26, 2177
71

July 7, 2195

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.

22 eclipse events between September 8, 1801 and September 7, 1877
September 7–8 June 26–27 April 14–15 January 31–February 1 November 19–20
112 114 116 118 120

September 8, 1801
June 26, 1805
April 14, 1809
February 1, 1813
November 19, 1816
122 124 126 128 130

September 7, 1820
June 26, 1824
April 14, 1828
February 1, 1832
November 20, 1835
132 134 136 138 140

September 7, 1839
June 27, 1843
April 15, 1847
February 1, 1851
November 20, 1854
142 144 146 148 150

September 7, 1858
June 27, 1862
April 15, 1866
January 31, 1870
November 20, 1873
152

September 7, 1877

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 1801 and 2200

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)
August 4, 2111
(Saros 147)
July 4, 2122
(Saros 148)

June 3, 2133
(Saros 149)
May 3, 2144
(Saros 150)
April 2, 2155
(Saros 151)
March 2, 2166
(Saros 152)
January 29, 2177
(Saros 153)

December 29, 2187
(Saros 154)
November 28, 2198
(Saros 155)

Inex series

This eclipse is a part of the long period inex cycle, repeating at alternating nodes, every 358 synodic months (≈ 10,571.95 days, or 29 years minus 20 days). Their appearance and longitude are irregular due to a lack of synchronization with the anomalistic month (period of perigee). However, groupings of 3 inex cycles (≈ 87 years minus 2 months) comes close (≈ 1,151.02 anomalistic months), so eclipses are similar in these groupings.

Series members between 1801 and 2200

November 19, 1816
(Saros 120)
October 30, 1845
(Saros 121)
October 10, 1874
(Saros 122)

September 21, 1903
(Saros 123)
August 31, 1932
(Saros 124)
August 11, 1961
(Saros 125)

July 22, 1990
(Saros 126)
July 2, 2019
(Saros 127)
June 11, 2048
(Saros 128)

May 22, 2077
(Saros 129)
May 3, 2106
(Saros 130)
April 13, 2135
(Saros 131)

March 23, 2164
(Saros 132)
March 3, 2193
(Saros 133)

Notes

  1. ^ "Moon Distances for London, United Kingdom, England". timeanddate. Retrieved 22 September 2024.
  2. ^ ON THE ECLIPSES AND OCCULTATIONS SEEN IN GERMANY IN THE PAST
  3. ^ Blake, William (1796). "The Monthly magazine. v.42 (1816). - Full View | HathiTrust Digital Library | HathiTrust Digital Library". Monthly Magazine and Critical Register of Books. Retrieved 2017-07-04.
  4. ^ "Total Solar Eclipse of 1816 Nov 19". EclipseWise.com. Retrieved 22 September 2024.
  5. ^ 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.
  6. ^ "NASA - Catalog of Solar Eclipses of Saros 120". eclipse.gsfc.nasa.gov.

References

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