Solar Saros 154
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Solar Saros 154
Saros cycle series 154 for 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 the Earth, totally or partially. Such an alignment occurs during an eclipse season, approximately every six mon ...s occurs at the Moon's descending node, repeating every 18 years, 11 days, containing 71 events, with 61 before 3000 AD. All eclipses in this series occurs at the Moon's descending node. 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 154 appears in the following table. Events References * http://eclipse.gsfc.nasa.gov/SEsaros/SEsaros154.html External linksSaros cycle 154 - Information and visualization {{Solar eclipses Solar saros series ...
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Saros Cycle
The saros () is a period of exactly 223 synodic months, approximately 6585.3211 days, or 18 years, 10, 11, or 12 days (depending on the number of leap years), and 8 hours, that can be used to predict eclipses of the Sun and Moon. One saros period after an eclipse, the Sun, Earth, and Moon return to approximately the same relative geometry, a near straight line, and a nearly identical eclipse will occur, in what is referred to as an eclipse cycle. A sar is one half of a saros. A series of eclipses that are separated by one saros is called a ''saros series''. It corresponds to: *6,585.321347 solar days *18.029 years *223 synodic months *241.999 draconic months *18.999 eclipse years (38 eclipse seasons) *238.992 anomalistic months The 19 eclipse years means that if there is a solar eclipse (or lunar eclipse), then after one saros a new moon will take place at the same node of the orbit of the Moon, and under these circumstances another eclipse can occur. History The earliest d ...
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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 the Earth, totally or partially. Such an alignment occurs during an eclipse season, approximately every six months, during the new moon phase, when the Moon's orbital plane is closest to the plane of the Earth's orbit. In a total eclipse, the disk of the Sun is fully obscured by the Moon. In 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 Moon ...
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Gamma (solar Eclipse)
Gamma (denoted as γ) of an eclipse describes how centrally the shadow of the Moon or Earth strikes the other body. This distance, measured at the moment when the axis of the shadow cone passes closest to the center of the Earth or Moon, is stated as a fraction of the equatorial radius of the Earth or Moon. Sign The sign of gamma defines, for a solar eclipse, if the axis of the shadow passes north or south of the center of the Earth; a positive value means north. The Earth is defined as that half which is exposed to the Sun (this changes with the seasons and is not related directly to the Earth's poles or equator; thus, the Earth's center is wherever the Sun is directly overhead). For a lunar eclipse, it defines whether the axis of the Earth's shadow passes north or south of the Moon; a positive value means south. Gamma changes monotonically throughout any single saros series. The change in gamma is larger when Earth is near its aphelion (June to July) than when it is near ...
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Magnitude Of Eclipse
The magnitude of eclipse is the fraction of the angular diameter of a celestial body being eclipsed. This applies to all celestial eclipses. The magnitude of a partial or annular solar eclipse is always between 0.0 and 1.0, while the magnitude of a total solar eclipse is always greater than or equal to 1.0. This measure is strictly a ratio of diameters and should not be confused with the covered fraction of the apparent area (disk) of the eclipsed body. Neither should it be confused with the astronomical magnitude scale of apparent brightness. Effect of the magnitude on a solar eclipse The apparent sizes of the Moon and Sun are both approximately 0.5°, or 30', but both vary because the distance between Earth and Moon varies. (The distance between Earth and Sun also varies, but the effect is slight in comparison.) In an annular solar eclipse, the magnitude of the eclipse is the ratio between the apparent angular diameters of the Moon and that of the Sun during the maximu ...
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Solar Eclipse Of July 19, 1917
This is a list of solar eclipses in the 20th century. During the period 1901 to 2000 there were 228 solar eclipses of which 78 were partial, 73 were annular (two non-central), 71 were total (three non-central) and 6 were hybrids. The greatest number of eclipses in one year was five, in 1935, and one month, July 2000, had two eclipses. Notable eclipses of the 20th century * 29 May 1919: this total eclipse was photographed by Arthur Eddington to verify general relativity (see Eddington experiment) * 20 June 1955: longest total eclipse between 1901 and 2000, lasting a maximum of 7 minutes and 8 seconds * 30 June 1973: a Concorde jet flew along the path, thereby extending the length of totality to 74 min. * 29 March 1987: second hybrid eclipse in less than one year, the first being on 3 October 1986. * 11 July 1991: Solar eclipse with the shortest gamma, of only −0.00412. * 31 July 2000: the second solar eclipse within one calendar month, the first being on 1 July 2000. T ...
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Solar Eclipse Of July 30, 1935
This is a list of solar eclipses in the 20th century. During the period 1901 to 2000 there were 228 solar eclipses of which 78 were partial, 73 were annular (two non-central), 71 were total (three non-central) and 6 were hybrids. The greatest number of eclipses in one year was five, in 1935, and one month, July 2000, had two eclipses. Notable eclipses of the 20th century * 29 May 1919: this total eclipse was photographed by Arthur Eddington to verify general relativity (see Eddington experiment) * 20 June 1955: longest total eclipse between 1901 and 2000, lasting a maximum of 7 minutes and 8 seconds * 30 June 1973: a Concorde jet flew along the path, thereby extending the length of totality to 74 min. * 29 March 1987: second hybrid eclipse in less than one year, the first being on 3 October 1986. * 11 July 1991: Solar eclipse with the shortest gamma, of only −0.00412. * 31 July 2000: the second solar eclipse within one calendar month, the first being on 1 July 2000. T ...
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Solar Eclipse Of August 9, 1953
A partial solar eclipse occurred on August 9, 1953. A solar eclipse occurs when the Moon passes between Earth and the Sun The Sun is the star at the center of the Solar System. It is a nearly perfect ball of hot plasma, heated to incandescence by nuclear fusion reactions in its core. The Sun radiates this energy mainly as light, ultraviolet, and infrared radi ..., 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. Related eclipses Solar eclipses of 1950–1953 References External links * http://eclipse.gsfc.nasa.gov/SEplot/SEplot1951/SE1953Aug09P.GIF 1953 8 9 1953 in science 1953 8 9 August 1953 events {{Solar-eclipse-stub ...
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Solar Eclipse Of August 20, 1971
A partial solar eclipse occurred on August 20–21, 1971. A solar eclipse occurs when the Moon passes between Earth and the Sun The Sun is the star at the center of the Solar System. It is a nearly perfect ball of hot plasma, heated to incandescence by nuclear fusion reactions in its core. The Sun radiates this energy mainly as light, ultraviolet, and infrared radi ..., 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 visible near sunrise on August 21 over parts of Australia. Related eclipses Solar eclipses of 1968–1971 References External links 1971 8 20 1971 in science 1971 8 20 August 1971 events {{solar-eclipse-stub ...
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Solar Eclipse Of August 31, 1989
A partial solar eclipse occurred on August 31, 1989. A solar eclipse occurs when the Moon passes between Earth and the Sun The Sun is the star at the center of the Solar System. It is a nearly perfect ball of hot plasma, heated to incandescence by nuclear fusion reactions in its core. The Sun radiates this energy mainly as light, ultraviolet, and infrared radi ..., 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. Related eclipses Eclipses of 1989 * A total lunar eclipse on February 20. * A partial solar eclipse on March 7. * A total lunar eclipse on August 17. * A partial solar eclipse on August 31. Solar eclipses of 1986–1989 Metonic series References External links 1989 8 31 1989 in science 1989 8 31 August 1989 events {{Solar-eclipse-stub ...
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Solar Eclipse Of September 11, 2007
A partial solar eclipse occurred at the Moon’s descending node of the orbit on September 11, 2007. 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. Eclipse season This is the second eclipse this season, the first being the August 2007 lunar eclipse. Images Gallery Eclipse (1360220276).jpg, Niterói, Brazil, 11:21 UTC Eclipse parcial do sol - 11 09 2007 (1386625631).jpg, Rio de Janeiro, Brazil, 11:40 UTC Giumaiolini - Partial Solar Eclipse - Brazil - 2007 (by).jpg, Composition from Campinas, Brazil Related eclipses Eclipses of 2007 * A total lunar eclipse on March 3. * A partial solar eclipse on March 19. * A total lunar eclipse on August 28. * A partial solar eclipse on September 11. Solar eclipses 2004–2007 Metonic series References ...
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Solar Eclipse Of September 21, 2025
A partial solar eclipse will occur on September 21, 2025. A solar eclipse occurs when the Moon passes between the Earth and the Sun The Sun is the star at the center of the Solar System. It is a nearly perfect ball of hot plasma, heated to incandescence by nuclear fusion reactions in its core. The Sun radiates this energy mainly as light, ultraviolet, and infrared radi ..., 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. Images Animated path Related eclipses Eclipses of 2025 * A total lunar eclipse on March 14. * A partial solar eclipse on March 29. * A total lunar eclipse on September 7. * A partial solar eclipse on September 21. Solar eclipses of 2022–2025 Metonic series References External links 2025 9 21 2025 in science September 2025 events 2025 9 21 2025 9 21 {{Solar-eclipse-stub ...
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Solar Eclipse Of October 3, 2043
An annular solar eclipse will occur on Saturday, October 3, 2043. 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 Annulus (or anulus) or annular indicates a ring- or donut-shaped area or structure. It may refer to: Human anatomy * ''Anulus fibrosus disci intervertebralis'', spinal structure * Annulus of Zinn, a.k.a. annular tendon or ''anulus tendineus com ... (ring). An annular eclipse appears as a partial eclipse over a region of the Earth thousands of kilometres wide. Images Animated path Related eclipses Solar eclipses of 2040–2043 Metonic cycle References External links * http://eclipse.gsfc.nasa.gov/SEplot/SEplot2001/SE2043Oct03A.GIF 2043 10 3 2043 in science 2043 10 3 2043 10 3 ...
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