Solar eclipse of June 21, 2058

Last updated
Solar eclipse of June 21, 2058
SE2058Jun21P.png
Map
Type of eclipse
NaturePartial
Gamma 1.4869
Magnitude 0.126
Maximum eclipse
Coordinates 65°54′N9°54′E / 65.9°N 9.9°E / 65.9; 9.9
Times (UTC)
Greatest eclipse0:19:35
References
Saros 157 (1 of 70)
Catalog # (SE5000) 9637

A partial solar eclipse will occur at the Moon's ascending node of orbit between Thursday, June 20 and Friday, June 21, 2058, [1] with a magnitude of 0.126. 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.

Contents

The partial solar eclipse will be visible for parts of western Russia, Scandinavia, and Greenland. This event will mark the beginning of Saros series 157.

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. [2]

June 21, 2058 Solar Eclipse Times
EventTime (UTC)
First Penumbral External Contact2058 June 20 at 23:24:06.1 UTC
Greatest Eclipse2058 June 21 at 00:19:34.6 UTC
Ecliptic Conjunction2058 June 21 at 00:36:33.9 UTC
Equatorial Conjunction2058 June 21 at 00:36:38.7 UTC
Last Penumbral External Contact2058 June 21 at 01:14:58.7 UTC
June 21, 2058 Solar Eclipse Parameters
ParameterValue
Eclipse Magnitude0.12608
Eclipse Obscuration0.05190
Gamma1.48693
Sun Right Ascension05h59m41.6s
Sun Declination+23°25'56.0"
Sun Semi-Diameter15'44.3"
Sun Equatorial Horizontal Parallax08.7"
Moon Right Ascension05h59m06.9s
Moon Declination+24°46'21.8"
Moon Semi-Diameter14'50.9"
Moon Equatorial Horizontal Parallax0°54'29.6"
ΔT89.4 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. The first and last eclipse in this sequence is separated by one synodic month.

Eclipse season of May–June 2058
May 22
Ascending node (new moon)
June 6
Descending node (full moon)
June 21
Ascending node (new moon)
SE2058May22P.png Lunar eclipse chart close-2058Jun06.png SE2058Jun21P.png
Partial solar eclipse
Solar Saros 119
Total lunar eclipse
Lunar Saros 131
Partial solar eclipse
Solar Saros 157

Eclipses in 2058

Metonic

Tzolkinex

Half-Saros

Tritos

Solar Saros 157

Inex

Triad

Solar eclipses of 2054–2058

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. [3]

The partial solar eclipses on March 9, 2054 and September 2, 2054 occur in the previous lunar year eclipse set, and the partial solar eclipses on May 22, 2058 and November 16, 2058 occur in the next lunar year eclipse set.

Solar eclipse series sets from 2054 to 2058
Ascending node Descending node
SarosMapGammaSarosMapGamma
117 August 3, 2054
SE2054Aug03P.png
Partial
−1.4941122 January 27, 2055
SE2055Jan27P.png
Partial
1.155
127 July 24, 2055
SE2055Jul24T.png
Total
−0.8012132 January 16, 2056
SE2056Jan16A.png
Annular
0.4199
137 July 12, 2056
SE2056Jul12A.png
Annular
−0.0426142 January 5, 2057
SE2057Jan05T.png
Total
−0.2837
147 July 1, 2057
SE2057Jul01A.png
Annular
0.7455152 December 26, 2057
SE2057Dec26T.png
Total
−0.9405
157 June 21, 2058
SE2058Jun21P.png
Partial
1.4869

Saros 157

This eclipse is a part of Saros series 157, repeating every 18 years, 11 days, and containing 70 events. The series will start with a partial solar eclipse on June 21, 2058. It contains annular eclipses from August 25, 2166 through March 10, 2491; hybrid eclipses from March 22, 2509 through April 12, 2545; and total eclipses from April 24, 2563 through April 21, 3158. The series ends at member 70 as a partial eclipse on July 17, 3302. 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 will be produced by member 15 at 4 minutes, 16 seconds on November 22, 2310, and the longest duration of totality will be produced by member 38 at 5 minutes, 57 seconds on July 31, 2725. All eclipses in this series occur at the Moon’s ascending node of orbit. [4]

Series members 1–8 occur between 2058 and 2200:
123
SE2058Jun21P.png
June 21, 2058
SE2076Jul01P.png
July 1, 2076
SE2094Jul12P.png
July 12, 2094
456
Saros157 04van70 SE2112Jul23P.jpg
July 23, 2112
Saros157 05van70 SE2130Aug04P.jpg
August 4, 2130
Saros157 06van70 SE2148Aug14P.jpg
August 14, 2148
78
Saros157 07van70 SE2166Aug25A.jpg
August 25, 2166
Saros157 08van70 SE2184Sep04A.jpg
September 4, 2184

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 June 21, 1982 and June 21, 2058
June 21April 8–9January 26November 13–14September 1–2
117119121123125
SE1982Jun21P.png
June 21, 1982
SE1986Apr09P.png
April 9, 1986
SE1990Jan26A.png
January 26, 1990
SE1993Nov13P.png
November 13, 1993
SE1997Sep02P.png
September 2, 1997
127129131133135
SE2001Jun21T.png
June 21, 2001
SE2005Apr08H.png
April 8, 2005
SE2009Jan26A.png
January 26, 2009
SE2012Nov13T.png
November 13, 2012
SE2016Sep01A.png
September 1, 2016
137139141143145
SE2020Jun21A.png
June 21, 2020
SE2024Apr08T.png
April 8, 2024
SE2028Jan26A.png
January 26, 2028
SE2031Nov14H.png
November 14, 2031
SE2035Sep02T.png
September 2, 2035
147149151153155
SE2039Jun21A.png
June 21, 2039
SE2043Apr09T.png
April 9, 2043
SE2047Jan26P.png
January 26, 2047
SE2050Nov14P.png
November 14, 2050
SE2054Sep02P.png
September 2, 2054
157
SE2058Jun21P.png
June 21, 2058

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.

The partial solar eclipses on November 16, 2134 (part of Saros 164) and October 16, 2145 (part of Saros 165) are also a part of this series but are not included in the table below.

Series members between 1801 and 2069
SE1807Jun06H.png
June 6, 1807
(Saros 134)
SE1818May05A.gif
May 5, 1818
(Saros 135)
SE1829Apr03T.gif
April 3, 1829
(Saros 136)
SE1840Mar04A.png
March 4, 1840
(Saros 137)
SE1851Feb01A.gif
February 1, 1851
(Saros 138)
SE1861Dec31T.gif
December 31, 1861
(Saros 139)
SE1872Nov30H.gif
November 30, 1872
(Saros 140)
SE1883Oct30A.gif
October 30, 1883
(Saros 141)
SE1894Sep29T.gif
September 29, 1894
(Saros 142)
SE1905Aug30T.png
August 30, 1905
(Saros 143)
SE1916Jul30A.png
July 30, 1916
(Saros 144)
SE1927Jun29T.png
June 29, 1927
(Saros 145)
SE1938May29T.png
May 29, 1938
(Saros 146)
SE1949Apr28P.png
April 28, 1949
(Saros 147)
SE1960Mar27P.png
March 27, 1960
(Saros 148)
SE1971Feb25P.png
February 25, 1971
(Saros 149)
SE1982Jan25P.png
January 25, 1982
(Saros 150)
SE1992Dec24P.png
December 24, 1992
(Saros 151)
SE2003Nov23T.png
November 23, 2003
(Saros 152)
SE2014Oct23P.png
October 23, 2014
(Saros 153)
SE2025Sep21P.png
September 21, 2025
(Saros 154)
SE2036Aug21P.png
August 21, 2036
(Saros 155)
SE2047Jul22P.png
July 22, 2047
(Saros 156)
SE2058Jun21P.png
June 21, 2058
(Saros 157)
SE2069May20P.png
May 20, 2069
(Saros 158)

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
SE1826Nov29P.gif
November 29, 1826
(Saros 149)
SE1855Nov09P.png
November 9, 1855
(Saros 150)
SE1884Oct19P.gif
October 19, 1884
(Saros 151)
SE1913Sep30P.png
September 30, 1913
(Saros 152)
SE1942Sep10P.png
September 10, 1942
(Saros 153)
SE1971Aug20P.png
August 20, 1971
(Saros 154)
SE2000Jul31P.png
July 31, 2000
(Saros 155)
SE2029Jul11P.png
July 11, 2029
(Saros 156)
SE2058Jun21P.png
June 21, 2058
(Saros 157)
SE2087Jun01P.png
June 1, 2087
(Saros 158)
Saros161 01van72 SE2174Apr01P.jpg
April 1, 2174
(Saros 161)

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References

  1. "June 20–21, 2058 Partial Solar Eclipse". timeanddate. Retrieved 17 August 2024.
  2. "Partial Solar Eclipse of 2058 Jun 21". EclipseWise.com. Retrieved 17 August 2024.
  3. 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.
  4. "NASA - Catalog of Solar Eclipses of Saros 157". eclipse.gsfc.nasa.gov.