Solar eclipse of June 11, 2067
Solar eclipse of June 11, 2067 | |
---|---|
Type of eclipse | |
Nature | Annular |
Gamma | −0.0387 |
Magnitude | 0.967 |
Maximum eclipse | |
Duration | 245 s (4 min 5 s) |
Coordinates | 21°00′N 130°12′W / 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 |
An annular solar eclipse will occur at the Moon's descending node of orbit on Saturday, June 11, 2067, with a magnitude of 0.967. 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.
Related eclipses[edit]
Eclipses in 2067[edit]
- A penumbral lunar eclipse on May 28, 2067.
- An annular solar eclipse on June 11, 2067.
- A penumbral lunar eclipse on June 27, 2067.
- A penumbral lunar eclipse on November 21, 2067.
- A hybrid solar eclipse on December 6, 2067.
Metonic[edit]
- Preceded by: Solar eclipse of August 24, 2063
- Followed by: Solar eclipse of March 31, 2071
Tzolkinex[edit]
- Preceded by: Solar eclipse of April 30, 2060
- Followed by: Solar eclipse of July 24, 2074
Half-Saros[edit]
- Preceded by: Lunar eclipse of June 6, 2058
- Followed by: Lunar eclipse of June 17, 2076
Tritos[edit]
- Preceded by: Solar eclipse of July 12, 2056
- Followed by: Solar eclipse of May 11, 2078
Solar Saros 138[edit]
- Preceded by: Solar eclipse of May 31, 2049
- Followed by: Solar eclipse of June 22, 2085
Inex[edit]
- Preceded by: Solar eclipse of July 2, 2038
- Followed by: Solar eclipse of May 22, 2096
Triad[edit]
- Preceded by: Solar eclipse of August 10, 1980
- Followed by: Solar eclipse of April 12, 2154
Solar eclipses of 2065–2069[edit]
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 to 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[edit]
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[edit]
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 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).
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[edit]
- ^ 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[edit]
- Earth visibility chart and eclipse statistics Eclipse Predictions by Fred Espenak, NASA/GSFC