| Solar eclipse of June 11, 2067 | |
|---|---|
 Map | |
| 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 / 21; -130.2 |
| 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. Occurring about 4.3 days before apogee (on June 16, 2067, at 4:05 UTC), the Moon's apparent diameter will be smaller.
The path of annularity will be visible from parts of Kiribati, Ecuador, northern Peru, extreme southern Colombia, and extreme western Brazil. A partial solar eclipse will also be visible for parts of Oceania, Hawaii, southern North America, Central America, the Caribbean, and western South America.
Eclipse details
Shown below are two tables displaying details about this particular solar eclipse. The first table outlines times at which the moon's penumbra or umbra attains the specific parameter, and the second table describes various other parameters pertaining to this eclipse.
| Event | Time (UTC) |
|---|---|
| First Penumbral External Contact | 2067 June 11 at 17:41:42.1 UTC |
| First Umbral External Contact | 2067 June 11 at 18:45:02.0 UTC |
| First Central Line | 2067 June 11 at 18:46:37.3 UTC |
| First Umbral Internal Contact | 2067 June 11 at 18:48:12.5 UTC |
| First Penumbral Internal Contact | 2067 June 11 at 19:51:38.7 UTC |
| Greatest Eclipse | 2067 June 11 at 20:42:26.4 UTC |
| Equatorial Conjunction | 2067 June 11 at 20:42:35.2 UTC |
| Ecliptic Conjunction | 2067 June 11 at 20:42:53.4 UTC |
| Greatest Duration | 2067 June 11 at 20:43:57.1 UTC |
| Last Penumbral Internal Contact | 2067 June 11 at 21:33:13.1 UTC |
| Last Umbral Internal Contact | 2067 June 11 at 22:36:38.6 UTC |
| Last Central Line | 2067 June 11 at 22:38:16.2 UTC |
| Last Umbral External Contact | 2067 June 11 at 22:39:53.8 UTC |
| Last Penumbral External Contact | 2067 June 11 at 23:43:15.9 UTC |
| Parameter | Value |
|---|---|
| Eclipse Magnitude | 0.96702 |
| Eclipse Obscuration | 0.93513 |
| Gamma | −0.03865 |
| Sun Right Ascension | 05h20m58.3s |
| Sun Declination | +23°07'36.6" |
| Sun Semi-Diameter | 15'45.1" |
| Sun Equatorial Horizontal Parallax | 08.7" |
| Moon Right Ascension | 05h20m58.0s |
| Moon Declination | +23°05'29.3" |
| Moon Semi-Diameter | 15'00.0" |
| Moon Equatorial Horizontal Parallax | 0°55'03.2" |
| ΔT | 95.6 s |
Eclipse season
See also: Eclipse cycleThis eclipse is part of an eclipse season, a period, roughly every six months, when eclipses occur. Only two (or occasionally three) eclipse seasons occur each year, and each season lasts about 35 days and repeats just short of six months (173 days) later; thus two full eclipse seasons always occur each year. Either two or three eclipses happen each eclipse season. In the sequence below, each eclipse is separated by a fortnight. The first and last eclipse in this sequence is separated by one synodic month.
| May 28 Ascending node (full moon) |
June 11 Descending node (new moon) |
June 27 Ascending node (full moon) |
|---|---|---|
 |
|
|
| Penumbral lunar eclipse Lunar Saros 112 |
Annular solar eclipse Solar Saros 138 |
Penumbral lunar eclipse Lunar Saros 150 |
Related eclipses
Eclipses in 2067
- A penumbral lunar eclipse on May 28.
- An annular solar eclipse on June 11.
- A penumbral lunar eclipse on June 27.
- A penumbral lunar eclipse on November 21.
- A hybrid solar eclipse on December 6.
Metonic
- Preceded by: Solar eclipse of August 24, 2063
- Followed by: Solar eclipse of March 31, 2071
Tzolkinex
- Preceded by: Solar eclipse of April 30, 2060
- Followed by: Solar eclipse of July 24, 2074
Half-Saros
- Preceded by: Lunar eclipse of June 6, 2058
- Followed by: Lunar eclipse of June 17, 2076
Tritos
- Preceded by: Solar eclipse of July 12, 2056
- Followed by: Solar eclipse of May 11, 2078
Solar Saros 138
- Preceded by: Solar eclipse of May 31, 2049
- Followed by: Solar eclipse of June 22, 2085
Inex
- Preceded by: Solar eclipse of July 2, 2038
- Followed by: Solar eclipse of May 22, 2096
Triad
- Preceded by: Solar eclipse of August 10, 1980
- Followed by: Solar eclipse of April 12, 2154
Solar eclipses of 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.
The partial solar eclipses on February 5, 2065 and August 2, 2065 occur in the previous lunar year eclipse set, and the partial solar eclipses on April 21, 2069 and October 15, 2069 occur in the next lunar year eclipse set.
| Solar eclipse series sets from 2065 to 2069 | ||||||
|---|---|---|---|---|---|---|
| Descending node | Ascending node | |||||
| Saros | Map | Gamma | Saros | Map | Gamma | |
| 118 | July 3, 2065 Partial |
1.4619 | 123 | December 27, 2065 Partial |
−1.0688 | |
| 128 | June 22, 2066 Annular |
0.733 | 133 | December 17, 2066 Total |
−0.4043 | |
| 138 | June 11, 2067 Annular |
−0.0387 | 143 | December 6, 2067 Hybrid |
0.2845 | |
| 148 | May 31, 2068 Total |
−0.797 | 153 | November 24, 2068 Partial |
1.0299 | |
| 158 | May 20, 2069 Partial |
−1.4852 | ||||
Saros 138
This eclipse is a part of Saros series 138, repeating every 18 years, 11 days, and containing 70 events. The series started with a partial solar eclipse on June 6, 1472. It contains annular eclipses from August 31, 1598 through February 18, 2482; a hybrid eclipse on March 1, 2500; and total eclipses from March 12, 2518 through April 3, 2554. The series ends at member 70 as a partial eclipse on July 11, 2716. Its eclipses are tabulated in three columns; every third eclipse in the same column is one exeligmos apart, so they all cast shadows over approximately the same parts of the Earth.
The longest duration of annularity was produced by member 23 at 8 minutes, 2 seconds on February 11, 1869, and the longest duration of totality will be produced by member 61 at 56 seconds on April 3, 2554. All eclipses in this series occur at the Moon’s descending node of orbit.
| Series members 20–41 occur between 1801 and 2200: | ||
|---|---|---|
| 20 | 21 | 22 |
 January 10, 1815 |
 January 20, 1833 |
 February 1, 1851 |
| 23 | 24 | 25 |
 February 11, 1869 |
 February 22, 1887 |
 March 6, 1905 |
| 26 | 27 | 28 |
 March 17, 1923 |
 March 27, 1941 |
 April 8, 1959 |
| 29 | 30 | 31 |
 April 18, 1977 |
 April 29, 1995 |
 May 10, 2013 |
| 32 | 33 | 34 |
 May 21, 2031 |
 May 31, 2049 |
June 11, 2067 |
| 35 | 36 | 37 |
 June 22, 2085 |
 July 4, 2103 |
 July 14, 2121 |
| 38 | 39 | 40 |
 July 25, 2139 |
 August 5, 2157 |
 August 16, 2175 |
| 41 | ||
 August 26, 2193 | ||
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.
| 22 eclipse events between June 12, 2029 and November 4, 2116 | ||||
|---|---|---|---|---|
| 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 | 156 |
 June 11, 2086 |
 March 31, 2090 |
 January 16, 2094 |
 November 4, 2097 |
 August 24, 2101 |
| 158 | 160 | 162 | 164 | |
 June 12, 2105 |
 November 4, 2116 | |||
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 1801 and 2200 | ||||
|---|---|---|---|---|
 June 26, 1805 (Saros 114) |
 May 27, 1816 (Saros 115) |
 April 26, 1827 (Saros 116) |
 March 25, 1838 (Saros 117) |
 February 23, 1849 (Saros 118) |
 January 23, 1860 (Saros 119) |
 December 22, 1870 (Saros 120) |
 November 21, 1881 (Saros 121) |
 October 20, 1892 (Saros 122) |
 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) |
 February 8, 2111 (Saros 142) |
 January 8, 2122 (Saros 143) |
 December 7, 2132 (Saros 144) |
 November 7, 2143 (Saros 145) |
 October 7, 2154 (Saros 146) |
 September 5, 2165 (Saros 147) |
 August 4, 2176 (Saros 148) |
 July 6, 2187 (Saros 149) |
 June 4, 2198 (Saros 150) | |||
Inex series
This eclipse is a part of the long period inex cycle, repeating at alternating nodes, every 358 synodic months (≈ 10,571.95 days, or 29 years minus 20 days). Their appearance and longitude are irregular due to a lack of synchronization with the anomalistic month (period of perigee). However, groupings of 3 inex cycles (≈ 87 years minus 2 months) comes close (≈ 1,151.02 anomalistic months), so eclipses are similar in these groupings.
| Series members between 1801 and 2200 | ||
|---|---|---|
 December 10, 1806 (Saros 129) |
 November 20, 1835 (Saros 130) |
 October 30, 1864 (Saros 131) |
 October 9, 1893 (Saros 132) |
 September 21, 1922 (Saros 133) |
 September 1, 1951 (Saros 134) |
 August 10, 1980 (Saros 135) |
 July 22, 2009 (Saros 136) |
 July 2, 2038 (Saros 137) |
June 11, 2067 (Saros 138) |
 May 22, 2096 (Saros 139) |
 May 3, 2125 (Saros 140) |
 April 12, 2154 (Saros 141) |
 March 23, 2183 (Saros 142) |
|
References
- "June 11, 2067 Annular Solar Eclipse". timeanddate. Retrieved 19 August 2024.
- "Moon Distances for London, United Kingdom, England". timeanddate. Retrieved 19 August 2024.
- "Annular Solar Eclipse of 2067 Jun 11". EclipseWise.com. Retrieved 19 August 2024.
- 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.
- "NASA - Catalog of Solar Eclipses of Saros 138". eclipse.gsfc.nasa.gov.
External links
- Earth visibility chart and eclipse statistics Eclipse Predictions by Fred Espenak, NASA/GSFC
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