Solar eclipse of June 1, 2030

Last updated
Solar eclipse of June 1, 2030
SE2030Jun01A.png
Map
Type of eclipse
NatureAnnular
Gamma 0.5626
Magnitude 0.9443
Maximum eclipse
Duration321 s (5 min 21 s)
Coordinates 56°30′N80°06′E / 56.5°N 80.1°E / 56.5; 80.1
Max. width of band250 km (160 mi)
Times (UTC)
Greatest eclipse6:29:13
References
Saros 128 (59 of 73)
Catalog # (SE5000) 9575

An annular solar eclipse will occur at the Moon's descending node of orbit on Saturday, June 1, 2030, [1] with a magnitude of 0.9443. 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 23 hours after apogee (on May 31, 2030, at 7:15 UTC), the Moon's apparent diameter will be smaller. [2]

Contents

The annular eclipse will start in northern Africa and will cross the Eurasian continent, including Algeria, Tunisia, Libya, Malta, Greece, northwestern Turkey, southeastern Bulgaria, southeastern Ukraine, Russia, northern Kazakhstan, northeastern China and northern Japan. It will also pass through a number of large cities such as Tripoli, Athens, Istanbul, Krasnodar, Rostov-on-Don, Volgograd, Omsk, Krasnoyarsk and Sapporo. The greatest eclipse will be near the border of Tomsk and Novosibirsk oblasts, ~200 km west of Tomsk. A partial eclipse will be visible for much of North Africa, Europe, Asia, Alaska, and northern Canada.

Solar eclipse of June 1, 2030
Interactive map of the path of the Umbral Shadow

Images

SE2030Jun01A.gif
Animated path

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]

June 1, 2030 Solar Eclipse Times
EventTime (UTC)
First Penumbral External Contact2030 June 01 at 03:35:53.3 UTC
First Umbral External Contact2030 June 01 at 04:48:25.8 UTC
First Central Line2030 June 01 at 04:51:16.8 UTC
First Umbral Internal Contact2030 June 01 at 04:54:09.4 UTC
Ecliptic Conjunction2030 June 01 at 06:22:30.7 UTC
Greatest Eclipse2030 June 01 at 06:29:12.9 UTC
Greatest Duration2030 June 01 at 06:29:55.1 UTC
Equatorial Conjunction2030 June 01 at 06:31:58.0 UTC
Last Umbral Internal Contact2030 June 01 at 08:04:14.9 UTC
Last Central Line2030 June 01 at 08:07:06.9 UTC
Last Umbral External Contact2030 June 01 at 08:09:57.3 UTC
Last Penumbral External Contact2030 June 01 at 09:22:29.8 UTC
June 1, 2030 Solar Eclipse Parameters
ParameterValue
Eclipse Magnitude0.94426
Eclipse Obscuration0.89163
Gamma0.56265
Sun Right Ascension04h37m01.2s
Sun Declination+22°03'55.3"
Sun Semi-Diameter15'46.4"
Sun Equatorial Horizontal Parallax08.7"
Moon Right Ascension04h36m55.8s
Moon Declination+22°34'11.5"
Moon Semi-Diameter14'42.7"
Moon Equatorial Horizontal Parallax0°53'59.6"
ΔT74.0 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 June 2030
June 1
Descending node (new moon)
June 15
Ascending node (full moon)
SE2030Jun01A.png Lunar eclipse chart close-2030Jun15.png
Annular solar eclipse
Solar Saros 128
Partial lunar eclipse
Lunar Saros 140

Eclipses in 2030

Metonic

Tzolkinex

Half-Saros

Tritos

Solar Saros 128

Inex

Triad

Solar eclipses of 2029–2032

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 eclipses on January 14, 2029 and July 11, 2029 occur in the previous lunar year eclipse set.

Solar eclipse series sets from 2029 to 2032
Descending node Ascending node
SarosMapGammaSarosMapGamma
118 June 12, 2029
SE2029Jun12P.png
Partial
1.29431123 December 5, 2029
SE2029Dec05P.png
Partial
−1.06090
128 June 1, 2030
SE2030Jun01A.png
Annular
0.56265133 November 25, 2030
SE2030Nov25T.png
Total
−0.38669
138 May 21, 2031
SE2031May21A.png
Annular
−0.19699143 November 14, 2031
SE2031Nov14H.png
Hybrid
0.30776
148 May 9, 2032
SE2032May09A.png
Annular
−0.93748153 November 3, 2032
SE2032Nov03P.png
Partial
1.06431

Saros 128

This eclipse is a part of Saros series 128, repeating every 18 years, 11 days, and containing 73 events. The series started with a partial solar eclipse on August 29, 984 AD. It contains total eclipses from May 16, 1417 through June 18, 1471; hybrid eclipses from June 28, 1489 through July 31, 1543; and annular eclipses from August 11, 1561 through July 25, 2120. The series ends at member 73 as a partial eclipse on November 1, 2282. 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 27 at 1 minutes, 45 seconds on June 7, 1453, and the longest duration of annularity was produced by member 48 at 8 minutes, 35 seconds on February 1, 1832. All eclipses in this series occur at the Moon’s descending node of orbit. [5]

Series members 47–68 occur between 1801 and 2200:
474849
SE1814Jan21A.gif
January 21, 1814
SE1832Feb01A.gif
February 1, 1832
SE1850Feb12A.gif
February 12, 1850
505152
SE1868Feb23A.gif
February 23, 1868
SE1886Mar05A.gif
March 5, 1886
SE1904Mar17A.png
March 17, 1904
535455
SE1922Mar28A.png
March 28, 1922
SE1940Apr07A.png
April 7, 1940
SE1958Apr19A.png
April 19, 1958
565758
SE1976Apr29A.png
April 29, 1976
SE1994May10A.png
May 10, 1994
SE2012May20A.png
May 20, 2012
596061
SE2030Jun01A.png
June 1, 2030
SE2048Jun11A.png
June 11, 2048
SE2066Jun22A.png
June 22, 2066
626364
SE2084Jul03A.png
July 3, 2084
SE2102Jul15A.png
July 15, 2102
SE2120Jul25A.png
July 25, 2120
656667
Saros128 65van73 SE2138Aug05P.jpg
August 5, 2138
Saros128 66van73 SE2156Aug16P.jpg
August 16, 2156
Saros128 67van73 SE2174Aug27P.jpg
August 27, 2174
68
Saros128 68van73 SE2192Sep06P.jpg
September 6, 2192

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
SE1801Mar14P.png
March 14, 1801
(Saros 107)
SE1812Feb12P.gif
February 12, 1812
(Saros 108)
SE1823Jan12P.gif
January 12, 1823
(Saros 109)
SE1844Nov10P.gif
November 10, 1844
(Saros 111)
SE1877Aug09P.gif
August 9, 1877
(Saros 114)
SE1888Jul09P.gif
July 9, 1888
(Saros 115)
SE1899Jun08P.gif
June 8, 1899
(Saros 116)
SE1910May09T.png
May 9, 1910
(Saros 117)
SE1921Apr08A.png
April 8, 1921
(Saros 118)
SE1932Mar07A.png
March 7, 1932
(Saros 119)
SE1943Feb04T.png
February 4, 1943
(Saros 120)
SE1954Jan05A.png
January 5, 1954
(Saros 121)
SE1964Dec04P.png
December 4, 1964
(Saros 122)
SE1975Nov03P.png
November 3, 1975
(Saros 123)
SE1986Oct03H.png
October 3, 1986
(Saros 124)
SE1997Sep02P.png
September 2, 1997
(Saros 125)
SE2008Aug01T.png
August 1, 2008
(Saros 126)
SE2019Jul02T.png
July 2, 2019
(Saros 127)
SE2030Jun01A.png
June 1, 2030
(Saros 128)
SE2041Apr30T.png
April 30, 2041
(Saros 129)
SE2052Mar30T.png
March 30, 2052
(Saros 130)
SE2063Feb28A.png
February 28, 2063
(Saros 131)
SE2074Jan27A.png
January 27, 2074
(Saros 132)
SE2084Dec27T.png
December 27, 2084
(Saros 133)
SE2095Nov27A.png
November 27, 2095
(Saros 134)
SE2106Oct26A.png
October 26, 2106
(Saros 135)
SE2117Sep26T.png
September 26, 2117
(Saros 136)
SE2128Aug25A.png
August 25, 2128
(Saros 137)
SE2139Jul25A.png
July 25, 2139
(Saros 138)
SE2150Jun25T.png
June 25, 2150
(Saros 139)
SE2161May25A.png
May 25, 2161
(Saros 140)
SE2172Apr23A.png
April 23, 2172
(Saros 141)
SE2183Mar23T.png
March 23, 2183
(Saros 142)
SE2194Feb21A.png
February 21, 2194
(Saros 143)

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
SE1827Oct20H.gif
October 20, 1827
(Saros 121)
SE1856Sep29A.gif
September 29, 1856
(Saros 122)
SE1885Sep08T.png
September 8, 1885
(Saros 123)
SE1914Aug21T.png
August 21, 1914
(Saros 124)
SE1943Aug01A.png
August 1, 1943
(Saros 125)
SE1972Jul10T.png
July 10, 1972
(Saros 126)
SE2001Jun21T.png
June 21, 2001
(Saros 127)
SE2030Jun01A.png
June 1, 2030
(Saros 128)
SE2059May11T.png
May 11, 2059
(Saros 129)
SE2088Apr21T.png
April 21, 2088
(Saros 130)
SE2117Apr02A.png
April 2, 2117
(Saros 131)
SE2146Mar12A.png
March 12, 2146
(Saros 132)
SE2175Feb21T.png
February 21, 2175
(Saros 133)

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<span class="mw-page-title-main">Solar eclipse of August 1, 1943</span> 20th-century annular solar eclipse

An annular solar eclipse occurred at the Moon's ascending node of orbit on Sunday, August 1, 1943, with a magnitude of 0.9409. 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 25 minutes before apogee, the Moon's apparent diameter was near its minimum. Apogee did occur as the eclipse was just before its greatest eclipse.

<span class="mw-page-title-main">Solar eclipse of December 24, 1927</span> 20th-century partial solar eclipse

A partial solar eclipse occurred at the Moon's descending node of orbit on Saturday, December 24, 1927, with a magnitude of 0.549. 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. "June 1, 2030 Annular Solar Eclipse". timeanddate. Retrieved 13 August 2024.
  2. "Moon Distances for London, United Kingdom, England". timeanddate. Retrieved 13 August 2024.
  3. "Annular Solar Eclipse of 2030 Jun 01". EclipseWise.com. Retrieved 13 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 128". eclipse.gsfc.nasa.gov.