Solar eclipse of April 20, 2061

Last updated
Solar eclipse of April 20, 2061
SE2061Apr20T.png
Map
Type of eclipse
NatureTotal
Gamma 0.9578
Magnitude 1.0475
Maximum eclipse
Duration157 s (2 min 37 s)
Coordinates 64°30′N59°12′E / 64.5°N 59.2°E / 64.5; 59.2
Max. width of band559 km (347 mi)
Times (UTC)
Greatest eclipse2:56:49
References
Saros 149 (23 of 71)
Catalog # (SE5000) 9644

A total solar eclipse will occur at the Moon's ascending node of orbit on Wednesday, April 20, 2061, [1] with a magnitude of 1.0475. 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 1.1 days before perigee (on April 21, 2061, at 4:00 UTC), the Moon's apparent diameter will be larger. [2]

Contents

Visibility

The eclipse will begin over Southern Russia and eastern Ukraine at sunrise and the moon shadow will move rapidly in a northeastern direction over west Kazakhstan (West Kazakhstan Region). The shadow will cover the Urals and races over the Arctic Ocean in a north-westerly direction and reaches the Svalbard archipelago. At sunset the eclipse will end just before the coast of Greenland.

The greatest eclipse will be in Russia on the east of Komi Republic (in Europe), ~120 km to south-east of Pechora.

A partial solar eclipse will also be visible for parts of Eastern Europe, Asia, Alaska, and northwestern Canada.

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. [3]

April 20, 2061 Solar Eclipse Times
EventTime (UTC)
First Penumbral External Contact2061 April 20 at 00:52:32.9 UTC
First Umbral External Contact2061 April 20 at 02:23:47.2 UTC
First Central Line2061 April 20 at 02:27:39.9 UTC
First Umbral Internal Contact2061 April 20 at 02:32:06.2 UTC
Greatest Eclipse2061 April 20 at 02:56:49.1 UTC
Ecliptic Conjunction2061 April 20 at 03:06:25.5 UTC
Equatorial Conjunction2061 April 20 at 03:45:10.8 UTC
Greatest Duration2061 April 20 at 09:41:30.5 UTC
Last Umbral Internal Contact2061 April 20 at 03:21:00.1 UTC
Last Central Line2061 April 20 at 03:25:27.9 UTC
Last Umbral External Contact2061 April 20 at 03:29:22.2 UTC
Last Penumbral External Contact2061 April 20 at 05:00:43.2 UTC
April 20, 2061 Solar Eclipse Parameters
ParameterValue
Eclipse Magnitude1.04755
Eclipse Obscuration1.09736
Gamma0.95776
Sun Right Ascension01h53m47.8s
Sun Declination+11°39'59.8"
Sun Semi-Diameter15'55.3"
Sun Equatorial Horizontal Parallax08.8"
Moon Right Ascension01h52m03.2s
Moon Declination+12°32'19.1"
Moon Semi-Diameter16'36.4"
Moon Equatorial Horizontal Parallax1°00'56.9"
ΔT91.3 s

Eclipse season

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 April 2061
April 4
Descending node (full moon)
 April 20
Ascending node (new moon)
SE2061Apr20T.png
Total lunar eclipse
Lunar Saros 123		 Total solar eclipse
Solar Saros 149

Eclipses in 2061

Metonic

Tzolkinex

Half-Saros

Tritos

Solar Saros 149

Inex

Triad

Solar eclipses of 2058–2061

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. [4]

The partial solar eclipse on June 21, 2058 occurs in the previous lunar year eclipse set.

Solar eclipse series sets from 2058 to 2061
Ascending node Descending node
SarosMapGammaSarosMapGamma
119 May 22, 2058
SE2058May22P.png
Partial		−1.3194124 November 16, 2058
SE2058Nov16P.png
Partial		1.1224
129 May 11, 2059
SE2059May11T.png
Total		−0.508134 November 5, 2059
SE2059Nov05A.png
Annular		0.4454
139 April 30, 2060
SE2060Apr30T.png
Total		0.2422144 October 24, 2060
SE2060Oct24A.png
Annular		−0.2625
149 April 20, 2061
SE2061Apr20T.png
Total		0.9578154 October 13, 2061
SE2061Oct13A.png
Annular		−0.9639

Saros 149

This eclipse is a part of Saros series 149, repeating every 18 years, 11 days, and containing 71 events. The series started with a partial solar eclipse on August 21, 1664. It contains total eclipses from April 9, 2043 through October 2, 2331; hybrid eclipses from October 13, 2349 through November 3, 2385; and annular eclipses from November 15, 2403 through July 13, 2800. The series ends at member 71 as a partial eclipse on September 28, 2926. 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 totality will be produced by member 31 at 4 minutes, 10 seconds on July 17, 2205, and the longest duration of annularity will be produced by member 62 at 5 minutes, 6 seconds on June 21, 2764. All eclipses in this series occur at the Moon’s ascending node of orbit. [5]

Series members 9–30 occur between 1801 and 2200:
91011
SE1808Nov18P.gif
November 18, 1808		 SE1826Nov29P.gif
November 29, 1826		 SE1844Dec09P.gif
December 9, 1844
121314
SE1862Dec21P.gif
December 21, 1862		 SE1880Dec31P.gif
December 31, 1880		 SE1899Jan11P.gif
January 11, 1899
151617
SE1917Jan23P.png
January 23, 1917 		SE1935Feb03P.png
February 3, 1935 		SE1953Feb14P.png
February 14, 1953
181920
SE1971Feb25P.png
February 25, 1971 		SE1989Mar07P.png
March 7, 1989 		SE2007Mar19P.png
March 19, 2007
212223
SE2025Mar29P.png
March 29, 2025 		SE2043Apr09T.png
April 9, 2043 		SE2061Apr20T.png
April 20, 2061
242526
SE2079May01T.png
May 1, 2079 		SE2097May11T.png
May 11, 2097 		SE2115May24T.png
May 24, 2115
272829
SE2133Jun03T.png
June 3, 2133		 Saros149 28van71 SE2151Jun14T.jpg
June 14, 2151		 SE2169Jun25T.png
June 25, 2169
30
Saros149 30van71 SE2187Jul06T.jpg
July 6, 2187

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.

21 eclipse events between July 1, 2000 and July 1, 2076
July 1–2April 19–20February 5–7November 24–25September 12–13
117119121123125
SE2000Jul01P.png
July 1, 2000 		SE2004Apr19P.png
April 19, 2004 		SE2008Feb07A.png
February 7, 2008 		SE2011Nov25P.png
November 25, 2011 		SE2015Sep13P.png
September 13, 2015
127129131133135
SE2019Jul02T.png
July 2, 2019 		SE2023Apr20H.png
April 20, 2023 		SE2027Feb06A.png
February 6, 2027 		SE2030Nov25T.png
November 25, 2030 		SE2034Sep12A.png
September 12, 2034
137139141143145
SE2038Jul02A.png
July 2, 2038 		SE2042Apr20T.png
April 20, 2042 		SE2046Feb05A.png
February 5, 2046 		SE2049Nov25H.png
November 25, 2049 		SE2053Sep12T.png
September 12, 2053
147149151153155
SE2057Jul01A.png
July 1, 2057 		SE2061Apr20T.png
April 20, 2061 		SE2065Feb05P.png
February 5, 2065 		SE2068Nov24P.png
November 24, 2068 		SE2072Sep12T.png
September 12, 2072
157
SE2076Jul01P.png
July 1, 2076

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
SE1810Apr04A.gif
April 4, 1810
(Saros 126)		 SE1821Mar04T.gif
March 4, 1821
(Saros 127)		 SE1832Feb01A.gif
February 1, 1832
(Saros 128)		 SE1842Dec31A.gif
December 31, 1842
(Saros 129)		 SE1853Nov30T.png
November 30, 1853
(Saros 130)
SE1864Oct30A.gif
October 30, 1864
(Saros 131)		 SE1875Sep29A.gif
September 29, 1875
(Saros 132)		 SE1886Aug29T.png
August 29, 1886
(Saros 133)		 SE1897Jul29A.gif
July 29, 1897
(Saros 134)		 SE1908Jun28A.png
June 28, 1908
(Saros 135)
SE1919May29T.png
May 29, 1919
(Saros 136)		 SE1930Apr28H.png
April 28, 1930
(Saros 137)		 SE1941Mar27A.png
March 27, 1941
(Saros 138)		 SE1952Feb25T.png
February 25, 1952
(Saros 139)		 SE1963Jan25A.png
January 25, 1963
(Saros 140)
SE1973Dec24A.png
December 24, 1973
(Saros 141)		 SE1984Nov22T.png
November 22, 1984
(Saros 142)		 SE1995Oct24T.png
October 24, 1995
(Saros 143)		 SE2006Sep22A.png
September 22, 2006
(Saros 144)		 SE2017Aug21T.png
August 21, 2017
(Saros 145)
SE2028Jul22T.png
July 22, 2028
(Saros 146)		 SE2039Jun21A.png
June 21, 2039
(Saros 147)		 SE2050May20H.png
May 20, 2050
(Saros 148)		 SE2061Apr20T.png
April 20, 2061
(Saros 149)		 SE2072Mar19P.png
March 19, 2072
(Saros 150)
SE2083Feb16P.png
February 16, 2083
(Saros 151)		 SE2094Jan16T.png
January 16, 2094
(Saros 152)		 Saros153 14van70 SE2104Dec17A.jpg
December 17, 2104
(Saros 153)		 SE2115Nov16A.png
November 16, 2115
(Saros 154)		 SE2126Oct16T.png
October 16, 2126
(Saros 155)
Saros156 08van69 SE2137Sep15P.jpg
September 15, 2137
(Saros 156)		 Saros157 06van70 SE2148Aug14P.jpg
August 14, 2148
(Saros 157)		 Saros158 06van70 SE2159Jul15P.jpg
July 15, 2159
(Saros 158)		 Saros159 03van70 SE2170Jun14P.jpg
June 14, 2170
(Saros 159)		 Saros160 01van71 SE2181May13P.jpg
May 13, 2181
(Saros 160)
Saros161 02van72 SE2192Apr12P.jpg
April 12, 2192
(Saros 161)

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
SE1829Sep28A.gif
September 28, 1829
(Saros 141)		 SE1858Sep07T.png
September 7, 1858
(Saros 142)		 SE1887Aug19T.png
August 19, 1887
(Saros 143)
SE1916Jul30A.png
July 30, 1916
(Saros 144)		 SE1945Jul09T.png
July 9, 1945
(Saros 145)		 SE1974Jun20T.png
June 20, 1974
(Saros 146)
SE2003May31A.png
May 31, 2003
(Saros 147)		 SE2032May09A.png
May 9, 2032
(Saros 148)		 SE2061Apr20T.png
April 20, 2061
(Saros 149)
SE2090Mar31P.png
March 31, 2090
(Saros 150)		 Saros151 20van72 SE2119Mar11A.jpg
March 11, 2119
(Saros 151)		 Saros152 20van70 SE2148Feb19T.jpg
February 19, 2148
(Saros 152)
Saros153 18van70 SE2177Jan29A.jpg
January 29, 2177
(Saros 153)

Related Research Articles

<span class="mw-page-title-main">Solar eclipse of May 9, 2032</span> Future annular solar eclipse

An annular solar eclipse will occur at the Moon's descending node of orbit on Sunday, May 9, 2032, with a magnitude of 0.9957. 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 Moon's apparent diameter will be near the average diameter because it will occur 5.7 days after perigee and 7.4 days before apogee.

<span class="mw-page-title-main">Solar eclipse of November 3, 2032</span> Future solar eclipse

A partial solar eclipse will occur at the Moon's ascending node of orbit on Wednesday, November 3, 2032, with a magnitude of 0.8554. 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 partial solar eclipse occurs in the polar regions of the Earth when the center of the Moon's shadow misses the Earth.

<span class="mw-page-title-main">Solar eclipse of August 31, 1989</span> 20th-century partial solar eclipse

A partial solar eclipse occurred at the Moon's descending node of orbit on Thursday, August 31, 1989, with a magnitude of 0.6344. 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 partial solar eclipse occurs in the polar regions of the Earth when the center of the Moon's shadow misses the Earth.

<span class="mw-page-title-main">Solar eclipse of August 9, 1953</span> 20th-century partial solar eclipse

A partial solar eclipse occurred at the Moon's descending node of orbit on Sunday, August 9, 1953, with a magnitude of 0.3729. 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 partial solar eclipse occurs in the polar regions of the Earth when the center of the Moon's shadow misses the Earth.

<span class="mw-page-title-main">Solar eclipse of October 3, 2043</span> Future annular solar eclipse

An annular solar eclipse will occur at the Moon's descending node of orbit on Saturday, October 3, 2043, with a magnitude of 0.9497. 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. Occurring about 4.8 days before apogee, the Moon's apparent diameter will be smaller.

<span class="mw-page-title-main">Solar eclipse of November 14, 2050</span> Future partial solar eclipse

A partial solar eclipse will occur at the Moon's ascending node of orbit on Monday, November 14, 2050, with a magnitude of 0.8874. 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 partial solar eclipse occurs in the polar regions of the Earth when the center of the Moon's shadow misses the Earth.

<span class="mw-page-title-main">Solar eclipse of October 4, 2070</span> Future annular solar eclipse

An annular solar eclipse will occur at the Moon's ascending node of orbit on Saturday, October 4, 2070, with a magnitude of 0.9731. 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.

<span class="mw-page-title-main">Solar eclipse of September 22, 2052</span> Future annular solar eclipse

An annular solar eclipse will occur at the Moon's ascending node of orbit between Sunday, September 22 and Monday, September 23, 2052, with a magnitude of 0.9734. 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. Occurring about 5.9 days before apogee, the Moon's apparent diameter will be smaller.

<span class="mw-page-title-main">Solar eclipse of March 9, 2054</span> Future partial solar eclipse

A partial solar eclipse will occur at the Moon's descending node of orbit on Monday, March 9, 2054, with a magnitude of 0.6678. 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 partial solar eclipse occurs in the polar regions of the Earth when the center of the Moon's shadow misses the Earth.

<span class="mw-page-title-main">Solar eclipse of October 13, 2061</span> Future annular solar eclipse

An annular solar eclipse will occur at the Moon's descending node of orbit on Thursday, October 13, 2061, with a magnitude of 0.9469. 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. Occurring about 1.1 days before apogee, the Moon's apparent diameter will be smaller.

<span class="mw-page-title-main">Solar eclipse of August 2, 2065</span> Future partial solar eclipse

A partial solar eclipse will occur at the Moon's descending node of orbit on Sunday, August 2, 2065, with a magnitude of 0.4903. 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 partial solar eclipse occurs in the polar regions of the Earth when the center of the Moon's shadow misses the Earth.

<span class="mw-page-title-main">Solar eclipse of February 5, 2065</span> Future partial solar eclipse

A partial solar eclipse will occur at the Moon's ascending node of orbit on Thursday, February 5, 2065, with a magnitude of 0.9123. 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 partial solar eclipse occurs in the polar regions of the Earth when the center of the Moon's shadow misses the Earth.

<span class="mw-page-title-main">Solar eclipse of November 24, 2068</span> Future partial solar eclipse

A partial solar eclipse will occur at the Moon's ascending node of orbit on Saturday, November 24, 2068, with a magnitude of 0.9109. 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 partial solar eclipse occurs in the polar regions of the Earth when the center of the Moon's shadow misses the Earth.

<span class="mw-page-title-main">Solar eclipse of May 31, 2068</span> Total eclipse

A total solar eclipse will occur at the Moon's descending node of orbit on Thursday, May 31, 2068, with a magnitude of 1.011. 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.

<span class="mw-page-title-main">Solar eclipse of April 11, 2070</span> Total eclipse

A total solar eclipse will occur at the Moon's descending node of orbit between Thursday, April 10 and Friday, April 11, 2070, with a magnitude of 1.0472. 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.

<span class="mw-page-title-main">Solar eclipse of March 19, 2072</span> Future partial solar eclipse

A partial solar eclipse will occur at the Moon's descending node of orbit on Saturday, March 19, 2072, with a magnitude of 0.7199. 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 partial solar eclipse occurs in the polar regions of the Earth when the center of the Moon's shadow misses the Earth.

<span class="mw-page-title-main">Solar eclipse of September 12, 2072</span> Total eclipse

A total solar eclipse will occur at the Moon's ascending node of orbit on Monday, September 12, 2072, with a magnitude of 1.0558. 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.

<span class="mw-page-title-main">Solar eclipse of October 24, 2079</span> Future annular solar eclipse

An annular solar eclipse will occur at the Moon's descending node of orbit on Tuesday, October 24, 2079, with a magnitude of 0.9484. 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.

<span class="mw-page-title-main">Solar eclipse of November 4, 2097</span> Future annular solar eclipse

An annular solar eclipse will occur at the Moon's descending node of orbit on Monday, November 4, 2097, with a magnitude of 0.9494. 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.

<span class="mw-page-title-main">Solar eclipse of March 31, 2090</span> Future partial solar eclipse

A partial solar eclipse will occur at the Moon's descending node of orbit on Friday, March 31, 2090, with a magnitude of 0.7843. 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 partial solar eclipse occurs in the polar regions of the Earth when the center of the Moon's shadow misses the Earth.

References

  1. ↑ "April 20, 2061 Total Solar Eclipse". timeanddate. Retrieved 17 August 2024.
  2. ↑ "Moon Distances for London, United Kingdom, England". timeanddate. Retrieved 17 August 2024.
  3. ↑ "Total Solar Eclipse of 2061 Apr 20". EclipseWise.com. Retrieved 17 August 2024.
  4. ↑ 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.
  5. ↑ "NASA - Catalog of Solar Eclipses of Saros 149". eclipse.gsfc.nasa.gov.
This page is based on this Wikipedia article
Text is available under the CC BY-SA 4.0 license; additional terms may apply.
Images, videos and audio are available under their respective licenses.