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PIM Press Release March 29, 2006 philadelphiamedicine.com | March 29, 2006 | Newsletters emhealth.com | Alcor News #50, April 29, 2006 alcor.org | October 29, 2006 Race Results carrolltonrunners.com |
Totality from Side, Turkey, 10:55 UTC
A total solar eclipse occurred on March 29, 2006, visible from a narrow corridor which traversed half the Earth. The magnitude, that is, the ratio between the apparent sizes of the Moon and that of the Sun, was 1.052, and it was part of Saros 139.
[edit] VisibilityThe path of totality of the Moon's shadow began at sunrise in Brazil and extended across the Atlantic to Africa, traveling across Ghana, Togo, Benin, Nigeria, Niger, Chad, Libya, and a small corner of Egypt, from there across the Mediterranean Sea to Greece (Kastellórizo) and Turkey, then across the Black Sea via Georgia, Russia, and Kazakhstan to Western Mongolia, where it ended at sunset. A partial eclipse was seen from the much broader path of the Moon's penumbra, including the northern two-thirds of Africa, the whole of Europe, and Central Asia. [edit] ObservationsPeople gathered in large areas where solar eclipse is visible around the World to view the event. Manchester Astronomical Society, the Malaysian Space Agency, the Astronomical Society of the Pacific, as well as dozens of tour groups met at the Apollo temple and the theater in Side, Turkey. The San Francisco Exploratorium featured a live webcast from the site, where thousands took their seats in the ancient, Roman-style theater.[1] Almost all actively visited areas in the path of totality had perfect weather. Many observers reported an unusually beautiful eclipse, with many or all effects visible, and a very nice corona despite proximity to solar minimum. The partial phase of the eclipse was also visible from the International Space Station, while the astronauts on board took spectacular pictures of the shadow on the Earth's surface. At first, it looked as though an orbit correction in the middle of March would bring the ISS in the path of totality, but this correction was postponed.
[edit] Notable times and coordinates
[edit] Type of the eclipse
[edit] Solar Eclipse in Turkey
[edit] Satellite failureMain article: Optus fleet of satellites#Failures The satellite responsible for SKY Network Television, a New Zealand pay TV company, failed the day after this eclipse at around 1900 local time. While SKY didn't directly attribute the failure to the eclipse, they said in a media release that it took longer to resolve the issue because of it, but this claim was refuted by astronomers. The main reason for the failure was because of an aging and increasingly faulty satellite.[2] [edit] Images[edit] Related eclipsesThis solar eclipse was preceded by the penumbral lunar eclipse on March 14, 2006. [edit] Solar eclipses 2004-2008This set of solar eclipses repeat approximately every 177 days and 4 hours at alternating nodes of the moon's orbit.
[edit] Saros 139It is a part of Saros cycle 139, repeating every 18 year, 11 days, containing 71 events. The series started with partial solar eclipse on May 17, 1501. It contains hybrid eclipses on August 11, 1627 through December 9, 1825 and total eclipses from December 21, 1843 through March 26, 2601. The series ends at member 71 as a partial eclipse on July 3, 2763. The solar eclipse of June 13, 2132 will be the next longest total solar eclipse at 6 minutes, 55 seconds. The longest duration of totality will be 7 minutes, 29 seconds on Jul 16, 2186.[3] This is the longest solar eclipse computed between 2000BC and 3000AD.[4] Series members 24-39 occur between 1901 and 2200:
[edit] Metonic seriesThe 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). This series has 20 eclipse events between June 10, 1964 and August 21, 2036.
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