Solar eclipse of June 1, 2030

An annular solar eclipse will occur on Saturday, 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.

Solar eclipse of June 1, 2030
Map
Type of eclipse
NatureAnnular
Gamma0.5626
Magnitude0.9443
Maximum eclipse
Duration321 sec (5 m 21 s)
Coordinates56.5°N 80.1°E / 56.5; 80.1
Max. width of band250 km (160 mi)
Times (UTC)
Greatest eclipse6:29:13
References
Saros128 (59 of 73)
Catalog # (SE5000)9575

An annular eclipse will start on the north of Africa and will cross Eurasian continent, will cross Algeria, Tunisia, Libya, Malta, Greece, Turkey, Bulgaria, Ukraine, Russia, Kazakhstan, China and Japan. An eclipse will pass through lot of large cities such as Tripoli, Athens, Istanbul, Krasnodar, Rostov-on-Don, Volgograd, Omsk, Krasnoyarsk and Sapporo.

Images


Animated path

Solar eclipses 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.[1]

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
118June 12, 2029

Partial
123December 5, 2029

Partial
128June 1, 2030

Annular
133November 25, 2030

Total
138May 21, 2031

Annular
143November 14, 2031

Hybrid
148May 9, 2032

Annular
153November 3, 2032

Partial

Saros 128

This eclipse is a member of the Solar Saros cycle 128, which includes 73 eclipses occurring in intervals of 18 years and 11 days. The series started with partial solar eclipse on August 29, 984 AD. From May 16, 1417 through June 18, 1471 the series produced total solar eclipses, followed by hybrid solar eclipses from June 28, 1489 through July 31, 1543, and annular solar eclipses from August 11, 1561 through July 25, 2120. The series ends at member 73 as a partial eclipse on November 1, 2282. All eclipses in this series occurs at the Moon’s descending node.

Series members 52–68 occur between 1901 and 2200
52 53 54

March 17, 1904

March 28, 1922

April 7, 1940
55 56 57

April 19, 1958

April 29, 1976

May 10, 1994
58 59 60

May 20, 2012

June 1, 2030

June 11, 2048
61 62 63

June 22, 2066

July 3, 2084

July 15, 2102
64 65 66

July 25, 2120
August 5, 2138 (Partial) August 16, 2156 (Partial)
67 68
August 27, 2174 (Partial) September 6, 2192 (Partial)

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.

21 eclipse events between June 1, 2011 and June 1, 2087
May 31 – June 1 March 19–20 January 5–6 October 24–25 August 12–13
118 120 122 124 126

June 1, 2011

March 20, 2015

January 6, 2019

October 25, 2022

August 12, 2026
128 130 132 134 136

June 1, 2030

March 20, 2034

January 5, 2038

October 25, 2041

August 12, 2045
138 140 142 144 146

May 31, 2049

March 20, 2053

January 5, 2057

October 24, 2060

August 12, 2064
148 150 152 154 156

May 31, 2068

March 19, 2072

January 6, 2076

October 24, 2079

August 13, 2083
158 160 162 164 166

June 1, 2087

October 24, 2098

References

  1. 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.


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