Solar eclipse of April 8, 2005 | |
---|---|
Type of eclipse | |
Nature | Hybrid |
Gamma | -0.3473 |
Magnitude | 1.0074 |
Maximum eclipse | |
Duration | 42 sec (0 m 42 s) |
Coordinates | 10°36′S119°00′W / 10.6°S 119°W |
Max. width of band | 27 km (17 mi) |
Times (UTC) | |
Greatest eclipse | 20:36:51 |
References | |
Saros | 129 (51 of 80) |
Catalog # (SE5000) | 9519 |
A total solar eclipse occurred at the Moon's ascending node on April 8, 2005. 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. A total solar eclipse occurs when the Moon's apparent diameter is larger than the Sun's, blocking all direct sunlight, turning day into darkness. Totality occurs in a narrow path across Earth's surface, with the partial solar eclipse visible over a surrounding region thousands of kilometres wide. This eclipse is a hybrid event, a narrow total eclipse, and beginning and ending as an annular eclipse.[ citation needed ]
It was visible within a narrow corridor in the Pacific Ocean. The path of the eclipse started south of New Zealand and crossed the Pacific Ocean in a diagonal path and ended in the extreme northwestern part of South America. The total solar eclipse was not visible on any land, while the annular solar eclipse was visible in the southern tip of Puntarenas Province of Costa Rica, Panama, Colombia and Venezuela. [1]
The exact time of the greatest took place on Friday, April 8, 2005, at 08:35:45.9 p.m. UTC, but occurring 4.4 days after perigee (Perigee on Monday, April 4, 2005), the Moon's apparent diameter was 0.7% larger than average. The Moon's distance from the Earth at greatest eclipse was 377,086 km (234,310 mi).
This is the first eclipse this season.
Second eclipse this season: 24 April 2005 Penumbral Lunar Eclipse
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. [2]
Ascending node | Descending node | |||||
---|---|---|---|---|---|---|
Saros | Map | Gamma | Saros | Map | Gamma | |
119 | 2004 April 19 Partial (south) | -1.13345 | 124 | 2004 October 14 Partial (north) | 1.03481 | |
129 Partial from Naiguatá | 2005 April 08 Hybrid | -0.34733 | 134 Annular from Madrid, Spain | 2005 October 03 Annular | 0.33058 | |
139 Total from Side, Turkey | 2006 March 29 Total | 0.38433 | 144 Partial from São Paulo, Brazil | 2006 September 22 Annular | -0.40624 | |
149 From Jaipur, India | 2007 March 19 Partial (north) | 1.07277 | 154 From Córdoba, Argentina | 2007 September 11 Partial (south) | -1.12552 |
It is a part of Saros cycle 129, repeating every 18 years, 11 days, containing 80 events. The series started with partial solar eclipse on October 3, 1103. It contains annular eclipses on May 6, 1464 through March 18, 1969, hybrid eclipses from March 29, 1987 through April 20, 2023 and total eclipses from April 30, 2041 through July 26, 2185. The series ends at member 80 as a partial eclipse on February 21, 2528. The longest duration of totality was 3 minutes, 43 seconds on June 25, 2131 . All eclipses in this series occurs at the Moon’s ascending node. [3]
Series members 46–56 occur between 1901 and 2100: | ||
---|---|---|
46 | 47 | 48 |
February 14, 1915 | February 24, 1933 | March 7, 1951 |
49 | 50 | 51 |
March 18, 1969 | March 29, 1987 | April 8, 2005 |
52 | 53 | 54 |
April 20, 2023 | April 30, 2041 | May 11, 2059 |
55 | 56 | |
May 22, 2077 | June 2, 2095 |
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 June 21, 1982, and June 21, 2058 | ||||
---|---|---|---|---|
June 21 | April 8–9 | January 26 | November 13–14 | September 1–2 |
107 | 109 | 111 | 113 | 115 |
June 21, 1963 | April 9, 1967 | January 26, 1971 | November 14, 1974 | September 2, 1978 |
117 | 119 | 121 | 123 | 125 |
June 21, 1982 | April 9, 1986 | January 26, 1990 | November 13, 1993 | September 2, 1997 |
127 | 129 | 131 | 133 | 135 |
June 21, 2001 | April 8, 2005 | January 26, 2009 | November 13, 2012 | September 1, 2016 |
137 | 139 | 141 | 143 | 145 |
June 21, 2020 | April 8, 2024 | January 26, 2028 | November 14, 2031 | September 2, 2035 |
147 | 149 | 151 | 153 | 155 |
June 21, 2039 | April 9, 2043 | January 26, 2047 | November 14, 2050 | September 2, 2054 |
157 | ||||
June 21, 2058 |
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