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List Of Saros Series For Solar Eclipses
Solar eclipse, Solar eclipses are grouped by their Saros (astronomy), saros number, each series lasts between 1200 and 1600 years and contains from 69 to 87 solar eclipses (most often 70 to 73). Solar eclipses in odd series exist at the ascending Lunar node, node of the Moon's orbit, and even series occur at the descending nodes. Each series begins with partial eclipses, transitions into umbral eclipses (which includes annular, hybrid, and total eclipses), and then reverses back to partial. The counts for each type and their order are listed below. Ongoing saros series are highlighted according to the type of eclipses currently being produced. Series have been indexed as -13 to 190 (active between roughly 2000 BCE and 3000 CE), with events summarized: See also * List of saros series for lunar eclipses * Lists of solar eclipses References {{DEFAULTSORT:Saros series for solar eclipses Solar saros series, * Solar eclipses ... [...More Info...] [...Related Items...] OR: [Wikipedia] [Google] [Baidu] |
Solar Eclipse
A solar eclipse occurs when the Moon passes between Earth and the Sun, thereby obscuring the view of the Sun from a small part of Earth, totally or partially. Such an alignment occurs approximately every six months, during the eclipse season in its new moon phase, when the Moon's orbital plane is closest to Ecliptic, the plane of Earth's orbit. In a total eclipse, the disk of the Sun is fully obscured by the Moon. In #Types, partial and annular eclipses, only part of the Sun is obscured. Unlike a lunar eclipse, which may be viewed from anywhere on the night side of Earth, a solar eclipse can only be viewed from a relatively small area of the world. As such, although total solar eclipses occur somewhere on Earth every 18 months on average, they recur at any given place only once every 360 to 410 years. If the Moon were in a perfectly circular orbit and in the same orbital plane as Earth, there would be total solar eclipses once a month, at every new moon. Instead, because the Mo ... [...More Info...] [...Related Items...] OR: [Wikipedia] [Google] [Baidu] |
Solar Saros 119
Saros cycle series 119 for solar eclipses occurs at the Moon's ascending node, repeating every 18 years, 11 days, containing 71 eclipses, including 54 umbral eclipses (2 total, 1 hybrid, and 51 annular). The first eclipse was on 15 May 850 and the last will be on 24 June 2112. The most recent eclipse was a partial eclipse on 30 April 2022 and the next will be a partial eclipse on 11 May 2040. The longest duration of totality was only 32 seconds on August 20, 1012. The longest duration of annularity was 7 minutes, 37 seconds on September 1, 1625. Umbral eclipses Umbral eclipses (annular, total and hybrid) can be further classified as either: 1) Central (two limits), 2) Central (one limit) or 3) Non-Central (one limit). The statistical distribution of these classes in Saros series 119 appears in the following table. All eclipses Note: Dates are given in the Julian calendar prior to 15 October 1582, and in the Gregorian calendar The Gregorian calendar is the calendar u ... [...More Info...] [...Related Items...] OR: [Wikipedia] [Google] [Baidu] |
Solar Eclipse Of November 25, 2011
A partial solar eclipse occurred at the Moon’s ascending node of orbit on Friday, November 25, 2011, with a magnitude of 0.9047. 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. This was the last of four partial solar eclipses in 2011, with the others occurring on January 4, June 1, and July 1. This eclipse was visible across Antarctica in its summer 24-hour day sunlight, and New Zealand at sunset with less than 20% of the Sun obscured. Parts of the western Antarctic Peninsula experienced nearly 90% obscuration of the Sun, while South Africa and Tasmania experienced a very small partial eclipse. Images Animated path Eclipse details Shown below are two tables displaying details about this particular solar eclipse. The first table outlines times at which the ... [...More Info...] [...Related Items...] OR: [Wikipedia] [Google] [Baidu] |
Solar Saros 123
Saros cycle series 123 for solar eclipses occurs at the Moon's ascending lunar node, node, repeating every 18 years, 11 days, containing 70 eclipses, 44 of which are umbral (27 annular, 3 hybrid, 14 total). The first eclipse in the series was on 29 April 1074 and the last will be on 31 May 2318. The most recent eclipse was a partial eclipse on Solar eclipse of November 25, 2011, 25 November 2011 and the next will be a partial eclipse on Solar eclipse of December 5, 2029, 5 December 2029. The longest totality was 3 minutes 27 seconds on 27 July 1813, the longest annular was 8 minutes 7 seconds on 9 November 1398, and the longest hybrid eclipse was 1 minute 32 seconds on 22 May 1705. This solar saros is linked to Lunar Saros 116. Umbral eclipses Umbral eclipses (annular, total and hybrid) can be further classified as either: 1) Central (two limits), 2) Central (one limit) or 3) Non-Central (one limit). The statistical distribution of these classes in Saros series 123 appears in t ... [...More Info...] [...Related Items...] OR: [Wikipedia] [Google] [Baidu] |
