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Future annular solar eclipse From Wikipedia, the free encyclopedia
An annular solar eclipse will occur at the Moon's ascending node of orbit on Wednesday, February 28, 2063,[1] with a magnitude of 0.9293. 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 2.7 days after apogee (on February 25, 2063, at 16:30 UTC), the Moon's apparent diameter will be smaller.[2]
The path of annularity will be visible from parts of the Prince Edward Islands, western Indonesia, Malaysia, Brunei, and the southern Philippines. A partial solar eclipse will also be visible for parts of Southern Africa, Antarctica, Australia, and Southeast Asia.
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 | 2063 February 28 at 04:42:05.6 UTC |
| First Umbral External Contact | 2063 February 28 at 05:49:10.0 UTC |
| First Central Line | 2063 February 28 at 05:52:20.5 UTC |
| First Umbral Internal Contact | 2063 February 28 at 05:55:31.6 UTC |
| First Penumbral Internal Contact | 2063 February 28 at 07:12:40.5 UTC |
| Equatorial Conjunction | 2063 February 28 at 07:22:27.6 UTC |
| Greatest Duration | 2063 February 28 at 07:28:49.9 UTC |
| Ecliptic Conjunction | 2063 February 28 at 07:39:28.8 UTC |
| Greatest Eclipse | 2063 February 28 at 07:43:30.0 UTC |
| Last Penumbral Internal Contact | 2063 February 28 at 08:14:50.6 UTC |
| Last Umbral Internal Contact | 2063 February 28 at 09:31:42.9 UTC |
| Last Central Line | 2063 February 28 at 09:34:52.1 UTC |
| Last Umbral External Contact | 2063 February 28 at 09:38:00.6 UTC |
| Last Penumbral External Contact | 2063 February 28 at 10:44:59.0 UTC |
| Parameter | Value |
|---|---|
| Eclipse Magnitude | 0.92926 |
| Eclipse Obscuration | 0.86352 |
| Gamma | −0.33604 |
| Sun Right Ascension | 22h45m11.8s |
| Sun Declination | -07°54'42.4" |
| Sun Semi-Diameter | 16'08.9" |
| Sun Equatorial Horizontal Parallax | 08.9" |
| Moon Right Ascension | 22h45m46.2s |
| Moon Declination | -08°10'47.1" |
| Moon Semi-Diameter | 14'47.6" |
| Moon Equatorial Horizontal Parallax | 0°54'17.7" |
| ΔT | 92.6 s |
This 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.
| February 27 Ascending node (new moon) | March 14 Descending node (full moon) |
|---|---|
| |
| Annular solar eclipse Solar Saros 131 | Partial lunar eclipse Lunar Saros 143 |
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.[4]
The partial solar eclipses on July 3, 2065 and December 27, 2065 occur in the next lunar year eclipse set.
| Solar eclipse series sets from 2062 to 2065 | ||||||
|---|---|---|---|---|---|---|
| Ascending node | Descending node | |||||
| Saros | Map | Gamma | Saros | Map | Gamma | |
| 121 | March 11, 2062 Partial |
−1.0238 | 126 | September 3, 2062 Partial |
1.0191 | |
| 131 | February 28, 2063 Annular |
−0.336 | 136 | August 24, 2063 Total |
0.2771 | |
| 141 | February 17, 2064 Annular |
0.3597 | 146 | August 12, 2064 Total |
−0.4652 | |
| 151 | February 5, 2065 Partial |
1.0336 | 156 | August 2, 2065 Partial |
−1.2759 | |
This eclipse is a part of Saros series 131, repeating every 18 years, 11 days, and containing 70 events. The series started with a partial solar eclipse on August 1, 1125. It contains total eclipses from March 27, 1522 through May 30, 1612; hybrid eclipses from June 10, 1630 through July 24, 1702; and annular eclipses from August 4, 1720 through June 18, 2243. The series ends at member 70 as a partial eclipse on September 2, 2369. 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 totality was produced by member 28 at 58 seconds on May 30, 1612, and the longest duration of annularity was produced by member 50 at 7 minutes, 54 seconds on January 26, 2009. All eclipses in this series occur at the Moon’s ascending node of orbit.[5]
| Series members 39–60 occur between 1801 and 2200: | ||
|---|---|---|
| 39 | 40 | 41 |
 September 28, 1810 |
 October 9, 1828 |
 October 20, 1846 |
| 42 | 43 | 44 |
 October 30, 1864 |
 November 10, 1882 |
 November 22, 1900 |
| 45 | 46 | 47 |
 December 3, 1918 |
 December 13, 1936 |
 December 25, 1954 |
| 48 | 49 | 50 |
 January 4, 1973 |
 January 15, 1991 |
 January 26, 2009 |
| 51 | 52 | 53 |
 February 6, 2027 |
 February 16, 2045 |
February 28, 2063 |
| 54 | 55 | 56 |
 March 10, 2081 |
 March 21, 2099 |
 April 2, 2117 |
| 57 | 58 | 59 |
 April 13, 2135 |
 April 23, 2153 |
 May 5, 2171 |
| 60 | ||
 May 15, 2189 | ||
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 ascending node.
| 21 eclipse events between July 23, 2036 and July 23, 2112 | ||||
|---|---|---|---|---|
| July 23–24 | May 11 | February 27–28 | December 16–17 | October 4–5 |
| 117 | 119 | 121 | 123 | 125 |
 July 23, 2036 |
 May 11, 2040 |
 February 28, 2044 |
 December 16, 2047 |
 October 4, 2051 |
| 127 | 129 | 131 | 133 | 135 |
 July 24, 2055 |
 May 11, 2059 |
February 28, 2063 |
 December 17, 2066 |
 October 4, 2070 |
| 137 | 139 | 141 | 143 | 145 |
 July 24, 2074 |
 May 11, 2078 |
 February 27, 2082 |
 December 16, 2085 |
 October 4, 2089 |
| 147 | 149 | 151 | 153 | 155 |
 July 23, 2093 |
 May 11, 2097 |
 February 28, 2101 |
 December 17, 2104 |
 October 5, 2108 |
| 157 | ||||
 July 23, 2112 | ||||
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 | ||||
|---|---|---|---|---|
 March 14, 1801 (Saros 107) |
 February 12, 1812 (Saros 108) |
 January 12, 1823 (Saros 109) |
 November 10, 1844 (Saros 111) | |
 August 9, 1877 (Saros 114) |
 July 9, 1888 (Saros 115) |
 June 8, 1899 (Saros 116) | ||
 May 9, 1910 (Saros 117) |
 April 8, 1921 (Saros 118) |
 March 7, 1932 (Saros 119) |
 February 4, 1943 (Saros 120) |
 January 5, 1954 (Saros 121) |
 December 4, 1964 (Saros 122) |
 November 3, 1975 (Saros 123) |
 October 3, 1986 (Saros 124) |
 September 2, 1997 (Saros 125) |
 August 1, 2008 (Saros 126) |
 July 2, 2019 (Saros 127) |
 June 1, 2030 (Saros 128) |
 April 30, 2041 (Saros 129) |
 March 30, 2052 (Saros 130) |
February 28, 2063 (Saros 131) |
 January 27, 2074 (Saros 132) |
 December 27, 2084 (Saros 133) |
 November 27, 2095 (Saros 134) |
 October 26, 2106 (Saros 135) |
 September 26, 2117 (Saros 136) |
 August 25, 2128 (Saros 137) |
 July 25, 2139 (Saros 138) |
 June 25, 2150 (Saros 139) |
 May 25, 2161 (Saros 140) |
 April 23, 2172 (Saros 141) |
 March 23, 2183 (Saros 142) |
 February 21, 2194 (Saros 143) | |||
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 | ||
|---|---|---|
 August 28, 1802 (Saros 122) |
 August 7, 1831 (Saros 123) |
 July 18, 1860 (Saros 124) |
 June 28, 1889 (Saros 125) |
 June 8, 1918 (Saros 126) |
 May 20, 1947 (Saros 127) |
 April 29, 1976 (Saros 128) |
 April 8, 2005 (Saros 129) |
 March 20, 2034 (Saros 130) |
February 28, 2063 (Saros 131) |
 February 7, 2092 (Saros 132) |
 January 19, 2121 (Saros 133) |
 December 30, 2149 (Saros 134) |
 December 9, 2178 (Saros 135) |
|
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