Solar eclipse of March 21, 2099 | |
---|---|
Type of eclipse | |
Nature | Annular |
Gamma | −0.4016 |
Magnitude | 0.93 |
Maximum eclipse | |
Duration | 452 sec (7 m 32 s) |
Coordinates | 20°S149°W / 20°S 149°W |
Max. width of band | 275 km (171 mi) |
Times (UTC) | |
Greatest eclipse | 22:54:32 |
References | |
Saros | 131 (55 of 70) |
Catalog # (SE5000) | 9731 |
An annular solar eclipse will occur on Saturday, March 21, 2099. 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.
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 eclipses 2098–2100 | |||||
---|---|---|---|---|---|
121 | April 1, 2098 Partial | 126 | September 25, 2098 Partial | ||
131 | March 21, 2099 Annular | 136 | September 14, 2099 Total | ||
141 | March 10, 2100 Annular | 146 | September 4, 2100 Total |
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.
Inex series members between 1901 and 2100: | ||
---|---|---|
July 20, 1925 (Saros 125) | June 30, 1954 (Saros 126) | June 11, 1983 (Saros 127) |
May 20, 2012 (Saros 128) | April 30, 2041 (Saros 129) | April 11, 2070 (Saros 130) |
March 21, 2099 (Saros 131) |
It is a part of Saros cycle 131, repeating every 18 years, 11 days, containing 70 events. The series started with partial solar eclipse on August 1, 1125. It contains total eclipses from March 27, 1522 through May 30, 1612 and 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. The longest duration of totality was only 58 seconds on May 30, 1612. All eclipses in this series occurs at the Moon’s ascending node.
Series members 33–70 occur between 1702 and 2369 | ||
---|---|---|
33 | 34 | 35 |
July 24, 1702 | August 4, 1720 | August 15, 1738 |
36 | 37 | 38 |
August 25, 1756 | September 6, 1774 | September 16, 1792 |
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 | 61 | 62 |
May 15, 2189 | May 27, 2207 | June 6, 2225 |
63 | 64 | 65 |
June 18, 2243 | June 28, 2261 | July 9, 2279 |
66 | 67 | 68 |
July 20, 2297 | August 1, 2315 | August 11, 2333 |
69 | 70 | |
August 22, 2351 | September 2, 2369 |
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