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Solar eclipse of June 1, 2030

 

Solar eclipse of June 1, 2030

Solar eclipse of June 1, 2030
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.

Contents

  • Images 1
  • Related eclipses 2
    • Solar eclipses 2029-2032 2.1
    • Saros 128 2.2
    • Metonic series 2.3
  • References 3
  • External links 4

Images


Animated path

Related eclipses

Solar eclipses 2029-2032

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

Partial
123 December 5, 2029

Partial
128 June 1, 2030

Annular
133 November 25, 2030

Total
138 May 21, 2031

Annular
143 November 14, 2031

Hybrid
148 May 9, 2032

Annular
153 November 3, 2032

Partial

Saros 128

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

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

June 22, 2066

July 3, 2084

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).

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

June 1, 2011

March 20, 2015

January 6, 2019

October 25, 2022

August 12, 2026
128 129 131 133 135

June 1, 2030

March 20, 2034

January 5, 2038

October 25, 2041

August 12, 2045
138 139 141 143 145

May 31, 2049

March 20, 2053

January 5, 2057

October 24, 2060

August 12, 2064
148 149 151 153 155

May 31, 2068

March 19, 2072

January 6, 2076

October 24, 2079

August 13, 2083
157

June 1, 2087

References

  1. ^ http://eclipse.gsfc.nasa.gov/SEsaros/SEsaros128.html

External links

  • NASA graphics


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