Solar eclipse of March 20, 2053

Last updated
Solar eclipse of March 20, 2053
SE2053Mar20A.png
Map
Type of eclipse
NatureAnnular
Gamma −0.4089
Magnitude 0.9919
Maximum eclipse
Duration50 s (0 min 50 s)
Coordinates 23°S83°E / 23°S 83°E / -23; 83
Max. width of band31 km (19 mi)
Times (UTC)
Greatest eclipse7:08:19
References
Saros 140 (31 of 71)
Catalog # (SE5000) 9625

An annular solar eclipse will occur at the Moon's descending node of orbit on Thursday, March 20, 2053, [1] with a magnitude of 0.9919. 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 5.6 days before perigee (on March 25, 2053, at 21:15 UTC), the Moon's apparent diameter will be larger. [2]

Contents

The path of annularity will be visible from parts of southern Indonesia. A partial solar eclipse will also be visible for parts of Southern Africa, Southeast Asia, Australia, and Antarctica.

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]

March 20, 2053 Solar Eclipse Times
EventTime (UTC)
First Penumbral External Contact2053 March 20 at 04:23:06.2 UTC
First Umbral External Contact2053 March 20 at 05:26:59.8 UTC
First Central Line2053 March 20 at 05:27:48.3 UTC
Greatest Duration2053 March 20 at 05:27:48.3 UTC
First Umbral Internal Contact2053 March 20 at 05:28:36.8 UTC
First Penumbral Internal Contact2053 March 20 at 06:49:15.3 UTC
Equatorial Conjunction2053 March 20 at 06:53:52.2 UTC
Greatest Eclipse2053 March 20 at 07:08:19.4 UTC
Ecliptic Conjunction2053 March 20 at 07:12:48.2 UTC
Last Penumbral Internal Contact2053 March 20 at 07:27:48.7 UTC
Last Umbral Internal Contact2053 March 20 at 08:48:15.0 UTC
Last Central Line2053 March 20 at 08:49:00.5 UTC
Last Umbral External Contact2053 March 20 at 08:49:45.8 UTC
Last Penumbral External Contact2053 March 20 at 09:53:32.9 UTC
March 20, 2053 Solar Eclipse Parameters
ParameterValue
Eclipse Magnitude0.99189
Eclipse Obscuration0.98385
Gamma−0.40894
Sun Right Ascension00h00m30.3s
Sun Declination+00°03'17.2"
Sun Semi-Diameter16'03.6"
Sun Equatorial Horizontal Parallax08.8"
Moon Right Ascension00h00m59.0s
Moon Declination-00°19'05.6"
Moon Semi-Diameter15'41.9"
Moon Equatorial Horizontal Parallax0°57'37.0"
ΔT86.0 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 March 2053
March 4
Ascending node (full moon)
March 20
Descending node (new moon)
Lunar eclipse chart close-2053Mar04.png SE2053Mar20A.png
Penumbral lunar eclipse
Lunar Saros 114
Annular solar eclipse
Solar Saros 140

Eclipses in 2053

Metonic

Tzolkinex

Half-Saros

Tritos

Solar Saros 140

Inex

Triad

Solar eclipses of 2051–2054

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 August 3, 2054 occurs in the next lunar year eclipse set.

Solar eclipse series sets from 2051 to 2054
Descending node Ascending node
SarosMapGammaSarosMapGamma
120 April 11, 2051
SE2051Apr11P.png
Partial
1.0169125 October 4, 2051
SE2051Oct04P.png
Partial
−1.2094
130 March 30, 2052
SE2052Mar30T.png
Total
0.3238135 September 22, 2052
SE2052Sep22A.png
Annular
−0.448
140 March 20, 2053
SE2053Mar20A.png
Annular
−0.4089145 September 12, 2053
SE2053Sep12T.png
Total
0.314
150 March 9, 2054
SE2054Mar09P.png
Partial
−1.1711155 September 2, 2054
SE2054Sep02P.png
Partial
1.0215

Saros 140

This eclipse is a part of Saros series 140, repeating every 18 years, 11 days, and containing 71 events. The series started with a partial solar eclipse on April 16, 1512. It contains total eclipses from July 21, 1656 through November 9, 1836; hybrid eclipses from November 20, 1854 through December 23, 1908; and annular eclipses from January 3, 1927 through December 7, 2485. The series ends at member 71 as a partial eclipse on June 1, 2774. 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 was produced by member 11 at 4 minutes, 10 seconds on August 12, 1692, and the longest duration of annularity will be produced by member 53 at 7 minutes, 35 seconds on November 15, 2449. All eclipses in this series occur at the Moon’s descending node of orbit. [5]

Series members 18–39 occur between 1801 and 2200:
181920
SE1818Oct29T.png
October 29, 1818
SE1836Nov09T.png
November 9, 1836
SE1854Nov20H.png
November 20, 1854
212223
SE1872Nov30H.png
November 30, 1872
SE1890Dec12H.png
December 12, 1890
SE1908Dec23H.png
December 23, 1908
242526
SE1927Jan03A.png
January 3, 1927
SE1945Jan14A.png
January 14, 1945
SE1963Jan25A.png
January 25, 1963
272829
SE1981Feb04A.png
February 4, 1981
SE1999Feb16A.png
February 16, 1999
SE2017Feb26A.png
February 26, 2017
303132
SE2035Mar09A.png
March 9, 2035
SE2053Mar20A.png
March 20, 2053
SE2071Mar31A.png
March 31, 2071
333435
SE2089Apr10A.png
April 10, 2089
SE2107Apr23A.png
April 23, 2107
SE2125May03A.png
May 3, 2125
363738
SE2143May14A.png
May 14, 2143
SE2161May25A.png
May 25, 2161
SE2179Jun05A.png
June 5, 2179
39
SE2197Jun15A.png
June 15, 2197

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 June 1, 2011 and October 24, 2098
May 31–June 1March 19–20January 5–6October 24–25August 12–13
118120122124126
SE2011Jun01P.png
June 1, 2011
SE2015Mar20T.png
March 20, 2015
SE2019Jan06P.png
January 6, 2019
SE2022Oct25P.png
October 25, 2022
SE2026Aug12T.png
August 12, 2026
128130132134136
SE2030Jun01A.png
June 1, 2030
SE2034Mar20T.png
March 20, 2034
SE2038Jan05A.png
January 5, 2038
SE2041Oct25A.png
October 25, 2041
SE2045Aug12T.png
August 12, 2045
138140142144146
SE2049May31A.png
May 31, 2049
SE2053Mar20A.png
March 20, 2053
SE2057Jan05T.png
January 5, 2057
SE2060Oct24A.png
October 24, 2060
SE2064Aug12T.png
August 12, 2064
148150152154156
SE2068May31T.png
May 31, 2068
SE2072Mar19P.png
March 19, 2072
SE2076Jan06T.png
January 6, 2076
SE2079Oct24A.png
October 24, 2079
SE2083Aug13P.png
August 13, 2083
158160162164
SE2087Jun01P.png
June 1, 2087
SE2098Oct24P.png
October 24, 2098

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
SE1802Mar04T.png
March 4, 1802
(Saros 117)
SE1813Feb01A.gif
February 1, 1813
(Saros 118)
SE1824Jan01A.gif
January 1, 1824
(Saros 119)
SE1834Nov30T.gif
November 30, 1834
(Saros 120)
SE1845Oct30H.png
October 30, 1845
(Saros 121)
SE1856Sep29A.gif
September 29, 1856
(Saros 122)
SE1867Aug29T.png
August 29, 1867
(Saros 123)
SE1878Jul29T.png
July 29, 1878
(Saros 124)
SE1889Jun28A.png
June 28, 1889
(Saros 125)
SE1900May28T.png
May 28, 1900
(Saros 126)
SE1911Apr28T.png
April 28, 1911
(Saros 127)
SE1922Mar28A.png
March 28, 1922
(Saros 128)
SE1933Feb24A.png
February 24, 1933
(Saros 129)
SE1944Jan25T.png
January 25, 1944
(Saros 130)
SE1954Dec25A.png
December 25, 1954
(Saros 131)
SE1965Nov23A.png
November 23, 1965
(Saros 132)
SE1976Oct23T.png
October 23, 1976
(Saros 133)
SE1987Sep23A.png
September 23, 1987
(Saros 134)
SE1998Aug22A.png
August 22, 1998
(Saros 135)
SE2009Jul22T.png
July 22, 2009
(Saros 136)
SE2020Jun21A.png
June 21, 2020
(Saros 137)
SE2031May21A.png
May 21, 2031
(Saros 138)
SE2042Apr20T.png
April 20, 2042
(Saros 139)
SE2053Mar20A.png
March 20, 2053
(Saros 140)
SE2064Feb17A.png
February 17, 2064
(Saros 141)
SE2075Jan16T.png
January 16, 2075
(Saros 142)
SE2085Dec16A.png
December 16, 2085
(Saros 143)
SE2096Nov15A.png
November 15, 2096
(Saros 144)
SE2107Oct16T.png
October 16, 2107
(Saros 145)
SE2118Sep15T.png
September 15, 2118
(Saros 146)
SE2129Aug15A.png
August 15, 2129
(Saros 147)
Saros148 28van75 SE2140Jul14T.jpg
July 14, 2140
(Saros 148)
Saros149 28van71 SE2151Jun14T.jpg
June 14, 2151
(Saros 149)
Saros150 25van71 SE2162May14A.jpg
May 14, 2162
(Saros 150)
Saros151 23van72 SE2173Apr12A.jpg
April 12, 2173
(Saros 151)
Saros152 22van70 SE2184Mar12T.jpg
March 12, 2184
(Saros 152)
Saros153 19van70 SE2195Feb10A.jpg
February 10, 2195
(Saros 153)

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
SE1821Aug27A.gif
August 27, 1821
(Saros 132)
SE1850Aug07T.gif
August 7, 1850
(Saros 133)
SE1879Jul19A.png
July 19, 1879
(Saros 134)
SE1908Jun28A.png
June 28, 1908
(Saros 135)
SE1937Jun08T.png
June 8, 1937
(Saros 136)
SE1966May20A.png
May 20, 1966
(Saros 137)
SE1995Apr29A.png
April 29, 1995
(Saros 138)
SE2024Apr08T.png
April 8, 2024
(Saros 139)
SE2053Mar20A.png
March 20, 2053
(Saros 140)
SE2082Feb27A.png
February 27, 2082
(Saros 141)
SE2111Feb08T.png
February 8, 2111
(Saros 142)
SE2140Jan20A.png
January 20, 2140
(Saros 143)
SE2168Dec29A.png
December 29, 2168
(Saros 144)
SE2197Dec09T.png
December 9, 2197
(Saros 145)

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References

  1. "March 20, 2053 Annular Solar Eclipse". timeanddate. Retrieved 15 August 2024.
  2. "Moon Distances for London, United Kingdom, England". timeanddate. Retrieved 15 August 2024.
  3. "Annular Solar Eclipse of 2053 Mar 20". EclipseWise.com. Retrieved 15 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 140". eclipse.gsfc.nasa.gov.