Solar eclipse of June 1, 2030

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Solar eclipse of June 1, 2030
SE2030Jun01A.png
Map
Type of eclipse
Nature Annular
Gamma 0.5626
Magnitude 0.9443
Maximum eclipse
Duration 5m 21s
Coordinates 56.5N 80.1E
Max. width of band 250 km
Times (UTC)
Greatest eclipse 6:29:13
References
Saros 128 (59 of 73)
Catalog # (SE5000) 9575

An annular solar eclipse will occur on June 1, 2030. 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.

Images[edit]

SE2030Jun01A.gif
Animated path

Related eclipses[edit]

Solar eclipses 2029-2032[edit]

Each member 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.

Note: Partial solar eclipses on January 14, 2029 and July 11, 2029 occur on the previous lunar year eclipse set.

Solar eclipse series sets from 2029-2032
Descending node   Ascending node
118 June 12, 2029
SE2029Jun12P.png
Partial
123 December 5, 2029
SE2029Dec05P.png
Partial
128 June 1, 2030
SE2030Jun01A.png
Annular
133 November 25, 2030
SE2030Nov25T.png
Total
138 May 21, 2031
SE2031May21A.png
Annular
143 November 14, 2031
SE2031Nov14H.png
Hybrid
148 May 9, 2032
SE2032May09A.png
Annular
153 November 3, 2032
SE2032Nov03P.png
Partial

Saros 128[edit]

It is a part of Saros cycle 128, repeating every 18 years, 11 days, containing 73 events. The series started with partial solar eclipse on August 29, 984 AD. It contains total eclipses from May 16, 1417 through June 18, 1471 and hybrid eclipses from June 28, 1489 through July 31, 1543. Then it progresses into annular eclipses from August 11, 1561 through July 25, 2120. The series ends at member 73 as a partial eclipse on November 1, 2282. The longest duration of totality was 1 minutes, 45 seconds on June 7, 1453.[1]

Series members 52-62 occur between 1901 and 2100:

52 53 54
SE1904Mar17A.png
March 17, 1904
SE1922Mar28A.png
March 28, 1922
SE1940Apr07A.png
April 7, 1940
55 56 57
SE1958Apr19A.png
April 19, 1958
SE1976Apr29A.png
April 29, 1976
SE1994May10A.png
May 10, 1994
58 59 60
SE2012May20A.png
May 20, 2012
SE2030Jun01A.png
June 1, 2030
SE2048Jun11A.png
June 11, 2048
61 62
SE2066Jun22A.png
June 22, 2066
SE2084Jul03A.png
July 3, 2084

Metonic series[edit]

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).

This series has 21 eclipse events between June 1, 2011 and June 1, 2087.

May 31 – June 1 March 20 January 5–6 October 24–25 August 12–13
118 119 121 123 125
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
128 129 131 133 135
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
138 139 141 143 145
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
148 149 151 153 155
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
157
SE2087Jun01P.png
June 1, 2087

References[edit]

External links[edit]