Solar eclipse of June 11, 2067
An annular solar eclipse will occur on June 11, 2067. 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 11, 2067 | |
---|---|
Map | |
Type of eclipse | |
Nature | Annular |
Gamma | -0.0387 |
Magnitude | 0.967 |
Maximum eclipse | |
Duration | 245 sec (4 m 5 s) |
Coordinates | 21°N 130.2°W |
Max. width of band | 119 km (74 mi) |
Times (UTC) | |
Greatest eclipse | 20:42:26 |
References | |
Saros | 138 (34 of 70) |
Catalog # (SE5000) | 9658 |
Related eclipses
Solar eclipses 2065–2069
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]
Solar eclipse series sets from 2065–2069 | ||||
---|---|---|---|---|
Descending node | Ascending node | |||
118 | July 3, 2065 Partial |
123 | December 27, 2065 Partial | |
128 | June 22, 2066 Annular |
133 | December 17, 2066 Total | |
138 | June 11, 2067 Annular |
143 | December 6, 2067 Hybrid | |
148 | May 31, 2068 Total |
153 | November 24, 2068 Partial | |
158 | May 20, 2069 Partial |
Saros 138
It is a part of Saros cycle 138, repeating every 18 years, 11 days, containing 70 events. The series started with partial solar eclipse on June 6, 1472. It contains annular eclipses from August 31, 1598 through February 18, 2482 with a hybrid eclipse on March 1, 2500. It has total eclipses from March 12, 2518 through April 3, 2554. The series ends at member 70 as a partial eclipse on July 11, 2716. The longest duration of totality will be only 56 seconds on April 3, 2554.
Series members 25–35 occur between 1901 and 2100: | ||
---|---|---|
25 | 26 | 27 |
March 6, 1905 |
March 17, 1923 |
March 27, 1941 |
28 | 29 | 30 |
April 8, 1959 |
April 18, 1977 |
April 29, 1995 |
31 | 32 | 33 |
May 10, 2013 |
May 21, 2031 |
May 31, 2049 |
34 | 35 | |
June 11, 2067 |
June 22, 2085 |
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 1901 and 2100 | |||
---|---|---|---|
September 21, 1903 (Saros 123) |
August 21, 1914 (Saros 124) |
July 20, 1925 (Saros 125) | |
June 19, 1936 (Saros 126) |
May 20, 1947 (Saros 127) |
April 19, 1958 (Saros 128) | |
March 18, 1969 (Saros 129) |
February 16, 1980 (Saros 130) |
January 15, 1991 (Saros 131) | |
December 14, 2001 (Saros 132) |
November 13, 2012 (Saros 133) |
October 14, 2023 (Saros 134) | |
September 12, 2034 (Saros 135) |
August 12, 2045 (Saros 136) |
July 12, 2056 (Saros 137) | |
June 11, 2067 (Saros 138) |
May 11, 2078 (Saros 139) |
April 10, 2089 (Saros 140) | |
March 10, 2100 (Saros 141) |
Metonic cycle
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).
21 eclipse events between June 12, 2029 and June 12, 2105 | ||||
---|---|---|---|---|
June 11–12 | March 30–31 | January 16 | November 4–5 | August 23–24 |
118 | 120 | 122 | 124 | 126 |
June 12, 2029 |
March 30, 2033 |
January 16, 2037 |
November 4, 2040 |
August 23, 2044 |
128 | 130 | 132 | 134 | 136 |
June 11, 2048 |
March 30, 2052 |
January 16, 2056 |
November 5, 2059 |
August 24, 2063 |
138 | 140 | 142 | 144 | 146 |
June 11, 2067 |
March 31, 2071 |
January 16, 2075 |
November 4, 2078 |
August 24, 2082 |
148 | 150 | 152 | 154 | |
June 11, 2086 |
March 31, 2090 |
January 16, 2094 |
November 4, 2097 |
References
- 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.
External links
- Earth visibility chart and eclipse statistics Eclipse Predictions by Fred Espenak, NASA/GSFC