| Annular eclipse | |
 Map | |
| Gamma | −0.0387 |
|---|---|
| Magnitude | 0.967 |
| Maximum eclipse | |
| Duration | 245 s (4 min 5 s) |
| Coordinates | 21°00′N130°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 annularsolar eclipse will occur at the Moon'sdescending node of orbit on Saturday, June 11, 2067,[1] with amagnitude of 0.967. Asolar eclipse occurs when theMoon passes betweenEarth and theSun, thereby totally or partly obscuring the image of the Sun for a viewer on Earth. An annular solar eclipse occurs when the Moon'sapparent diameter is smaller than the Sun's, blocking most of the Sun's light and causing the Sun to look like anannulus (ring). An annular eclipse appears as a partial eclipse over a region of the Earth thousands of kilometres wide. Occurring about 4.3 days beforeapogee (on June 16, 2067, at 4:05 UTC), the Moon's apparent diameter will be smaller.[2]
This solar eclipse is notable as it is the closest eclipse inSaros 138 to thesubsolar point with an eclipsegamma of -0.0387.
The path of annularity will be visible from parts ofKiribati,Ecuador, northernPeru, extreme southernColombia, and extreme westernBrazil. A partial solar eclipse will also be visible for parts ofOceania,Hawaii, southernNorth America,Central America, theCaribbean, and westernSouth America.
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.[3]
| 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 |
This eclipse is part of aneclipse 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 afortnight. The first and last eclipse in this sequence is separated by onesynodic 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 |
This eclipse is a member of asemester series. An eclipse in a semester series of solar eclipses repeats approximately every 177 days and 4 hours (a semester) at alternatingnodes of the Moon's orbit.[4]
The partial solar eclipses onFebruary 5, 2065 andAugust 2, 2065 occur in the previous lunar year eclipse set, and the partial solar eclipses onApril 21, 2069 andOctober 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 | ||||
This eclipse is a part ofSaros 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 oneexeligmos 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’sdescending node of orbit.[5]
| 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 | ||
Themetonic 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 | |||
This eclipse is a part of atritos cycle, repeating at alternating nodes every 135synodic months (≈ 3986.63 days, or 11 years minus 1 month). Their appearance and longitude are irregular due to a lack of synchronization with theanomalistic 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) | |||
This eclipse is a part of the long periodinex cycle, repeating at alternating nodes, every 358synodic months (≈ 10,571.95 days, or 29 years minus 20 days). Their appearance and longitude are irregular due to a lack of synchronization with theanomalistic 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) | |
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