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Solar eclipse of April 19, 2004

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Solar eclipse of April 19, 2004
Map
Type of eclipse
NaturePartial
Gamma−1.1335
Magnitude0.7367
Maximum eclipse
Coordinates61°36′S 44°18′E / 61.6°S 44.3°E / -61.6; 44.3
Times (UTC)
Greatest eclipse13:35:05
References
Saros119 (65 of 71)
Catalog # (SE5000)9517

A partial solar eclipse took place on Monday, 19 April 2004. 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 partial solar eclipse occurs in the polar regions of the Earth when the center of the Moon's shadow misses the Earth. It was largely visible over the south Atlantic Ocean and north shores of Antarctica, most prominently the Antarctic Peninsula. The eclipse was deep enough to be seen from a large portion of southern Africa, with over 50% totality at Cape Town, South Africa at approximately 4:10 PM. However, the eclipse remained visible to cities such as Harare, Maseru, Durban, and Bloemfontein, although to a much lesser extent.

The greatest eclipse of the Sun took place over a nigh inaccessible strip of ocean off the Antarctic coast; the maximum point displayed 73.5% totality, as compared to Cape Town's 51% totality.

Images


Animated eclipse path

Solar eclipses 2004–2007

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 eclipse series sets from 2004 to 2007
Ascending node   Descending node
Saros Map Gamma Saros Map Gamma
119 April 19, 2004

Partial
−1.13345 124 October 14, 2004

Partial
1.03481
129

Partial in Naiguatá, Venezuela
April 8, 2005

Hybrid
−0.34733 134

Annularity in Madrid, Spain
October 3, 2005

Annular
0.33058
139

Totality in Side, Turkey
March 29, 2006

Total
0.38433 144

Partial in São Paulo, Brazil
September 22, 2006

Annular
−0.40624
149

Partial in Jaipur, India
March 19, 2007

Partial
1.07277 154

Partial in Córdoba, Argentina
September 11, 2007

Partial
−1.12552

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 ascending node.

21 eclipse events between July 1, 2000 and July 1, 2076
July 1–2 April 19–20 February 5–7 November 24–25 September 12–13
117 119 121 123 125

July 1, 2000

April 19, 2004

February 7, 2008

November 25, 2011

September 13, 2015
127 129 131 133 135

July 2, 2019

April 20, 2023

February 6, 2027

November 25, 2030

September 12, 2034
137 139 141 143 145

July 2, 2038

April 20, 2042

February 5, 2046

November 25, 2049

September 12, 2053
147 149 151 153 155

July 1, 2057

April 20, 2061

February 5, 2065

November 24, 2068

September 12, 2072
157

July 1, 2076


  1. ^ 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.