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October 1949 Lunar Eclipse
A total lunar eclipse A lunar eclipse occurs when the Moon moves into the Earth's shadow. Such alignment occurs during an eclipse season, approximately every six months, during the full moon phase, when the Moon's orbital plane is closest to the plane of the Earth ... took place on Friday, October 7, 1949, the second of two lunar eclipses in 1949. Visibility Related lunar eclipses Lunar year series Saros series Half-Saros cycle A lunar eclipse will be preceded and followed by solar eclipses by 9 years and 5.5 days (a half saros).Mathematical Astronomy Morsels, Jean Meeus, p.110, Chapter 18, ''The half-saros'' This lunar eclipse is related to two total solar eclipses of Solar Saros 133. Tritos * Preceded: Lunar eclipse of November 7, 1938 * Followed: Lunar eclipse of September 5, 1960 Tzolkinex * Preceded: Lunar eclipse of August 26, 1942 * Followed: Lunar eclipse of November 18, 1956 See also * List of lunar eclipses * List of 20th-century lunar ecl ...
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Lunar Eclipse Chart Close-1949Oct07
Lunar most commonly means "of or relating to the Moon". Lunar may also refer to: Arts and entertainment * ''Lunar'' (series), a series of video games * "Lunar" (song), by David Guetta * "Lunar", a song by Priestess from the 2009 album ''Prior to the Fire'' * Lunars, a fictional race in the series ''The Lunar Chronicles'' by Marissa Meyer Other uses * Lunar Magic, Super Mario World level editor * Lunar Design, or LUNAR, a San Francisco-based design consultancy * Hasselblad Lunar, a digital camera * Lunar, a brandname of Ethinylestradiol/cyproterone acetate, a birth control pill * Lunar C (Jake Brook, born 1990), English rapper See also * * * Lunar calendar, based upon the monthly cycles of the Moon's phase ** Lunar day, in such calendars ** Lunar month In lunar calendars, a lunar month is the time between two successive syzygies of the same type: new moons or full moons. The precise definition varies, especially for the beginning of the month. Variations In Shona, Midd ...
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Solar Eclipse Of October 12, 1958
A total solar eclipse occurred on October 12, 1958. 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. Totality was visible in Tokelau, Cook Islands, French Polynesia, Chile and Argentina. This solar eclipse occurred over 3 months after the final game of 1958 FIFA World Cup The 1958 FIFA World Cup was the sixth FIFA World Cup, a quadrennial football tournament for men's senior national teams, and was played in Sweden from 8 to 29 June 1958. It was the first FIFA World Cup to be played in a Nordic country. Brazil be .... Related eclipses Solar eclipses of 1957–1960 Saros ...
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List Of 20th-century Lunar Eclipses
A total of 229 lunar eclipses took place in the 20th century: 83 penumbral, 65 partial and 81 total. See also: Lists of lunar eclipses, List of 19th-century lunar eclipses and List of 21st-century lunar eclipses List Eclipses from 2001 to 2002 are included on the end to complete the final set. References This list was compiled with data calculated by Fred Espenak of NASA The National Aeronautics and Space Administration (NASA ) is an independent agency of the US federal government responsible for the civil space program, aeronautics research, and space research. NASA was established in 1958, succeedi ...'s GSFC. {{DEFAULTSORT:20th-century lunar eclipses Lunar eclipses Lunar eclipses Lunar eclipses by time ...
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List Of Lunar Eclipses
There are several lists of lunar eclipses On the Moon, by the Earth ; Type * List of central lunar eclipses * Total penumbral lunar eclipse A total penumbral lunar eclipse is a lunar eclipse that occurs when the Moon becomes completely immersed in the penumbral cone of the Earth without touching the umbra. The path for the Moon to pass within the penumbra and outside the umbra is ve ... ; Classification * List of saros series for lunar eclipses * Tetrad (astronomy) contains lists of tetrads in the late-20th and 21st centuries ; By era * Lunar eclipses by century * Historically significant lunar eclipses On Earth, by the Moon {{DEFAULTSORT:Lunar eclipses ...
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November 1956 Lunar Eclipse
A total lunar eclipse took place on Sunday, November 18, 1956. Visibility Related lunar eclipses Lunar year series Tritos series Half-Saros cycle A lunar eclipse will be preceded and followed by solar eclipses by 9 years and 5.5 days (a half saros).Mathematical Astronomy Morsels, Jean Meeus, p.110, Chapter 18, ''The half-saros'' This lunar eclipse is related to two annular solar eclipses of Solar Saros 132. Tzolkinex * Preceded: Lunar eclipse of October 7, 1949 * Followed: Lunar eclipse of December 30, 1963 See also *List of lunar eclipses *List of 20th-century lunar eclipses A total of 229 lunar eclipses took place in the 20th century: 83 penumbral, 65 partial and 81 total. See also: Lists of lunar eclipses, List of 19th-century lunar eclipses and List of 21st-century lunar eclipses List Eclipses from 2001 to ... Notes External links * 1956-11 1956 in science November 1956 events {{lunar-eclipse-stub ...
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August 1942 Lunar Eclipse
A total lunar eclipse took place on Wednesday, August 26, 1942. The moon passed through the List of central lunar eclipses, center of the Earth's shadow. This is the 38th member of Lunar Saros 127. The previous event is the August 1924 lunar eclipse. The next event is the September 1960 lunar eclipse. Visibility Related lunar eclipses Inex series Saros series Lunar saros cycle, saros series 127, repeating every 18 years and 11 days, has a total of 72 lunar eclipse events including 54 umbral lunar eclipses (38 partial lunar eclipses and 16 total lunar eclipses). Solar Saros 134 interleaves with this lunar saros with an event occurring every 9 years 5 days alternating between each saros series. Tritos * Preceded: September 1931 lunar eclipse, Lunar eclipse of September 26, 1931 * Followed: July 1953 lunar eclipse, Lunar eclipse of July 26, 1953 Tzolkinex * Preceded: July 1935 lunar eclipse, Lunar eclipse of July 16, 1935 * Followed: October 1949 lunar eclipse, ...
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September 1960 Lunar Eclipse
A total lunar eclipse took place on Monday, September 5, 1960. The moon passed through the center of the Earth's shadow. This is the 39th member of Lunar Saros 127. The previous event is the August 1942 lunar eclipse. The next event is the September 1978 lunar eclipse. Visibility It was visible over the Pacific Ocean, and seen rising over Asia and Australia, and setting over North and South America. Related lunar eclipses Lunar year series Saros series Lunar saros series 127, repeating every 18 years and 11 days, has a total of 72 lunar eclipse events including 54 umbral lunar eclipses (38 partial lunar eclipses and 16 total lunar eclipses). Solar Saros 134 interleaves with this lunar saros with an event occurring every 9 years 5 days alternating between each saros series. Tritos * Preceded: Lunar eclipse of October 7, 1949 * Followed: Lunar eclipse of October 18, 1967 Tzolkinex * Preceded: Lunar eclipse of July 27, 1953 * Followed: Lunar eclipse ...
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November 1938 Lunar Eclipse
A total lunar eclipse took place at the Moon's descending node of the orbit on Monday, November 7, 1938, the second of two lunar eclipses in 1938, with an umbral eclipse magnitude of 1.35251. It was visible in the Americas, Europe, Asia, Asia and west in Oceania. The Moon was plunged into darkness for 1 hour, 21 minutes and 25.9 seconds, in a deep total eclipse which saw the Moon 35.251% of its diameter inside the Earth's umbral shadow. The visual effect of this depends on the state of the Earth's atmosphere, but the Moon may have been stained a deep red colour. The partial eclipse lasted for 3 hours, 30 minutes and 12.5 seconds in total. Occurring only 3.2 days before perigee (Perigee on Friday, November 11, 1938), the Moon's apparent diameter was 2% larger than average. Visibility Related lunar eclipses Half-Saros cycle A lunar eclipse will be preceded and followed by solar eclipses by 9 years and 5.5 days (a half saros).Mathematical Astronomy Morsels, Jean Meeus, p.110, C ...
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Solar Eclipse Of October 1, 1940
A total solar eclipse occurred on October 1, 1940. 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. Totality was visible from Colombia, Brazil, Venezuela and South Africa South Africa, officially the Republic of South Africa (RSA), is the southernmost country in Africa. It is bounded to the south by of coastline that stretch along the South Atlantic and Indian Oceans; to the north by the neighbouring count .... Related eclipses Solar eclipses 1939–1942 Saros 133 Metonic series Notes References 1940 10 01 1940 10 01 1940 in science October 1940 events ...
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Umbra
The umbra, penumbra and antumbra are three distinct parts of a shadow, created by any light source after impinging on an opaque object. Assuming no diffraction, for a collimated beam (such as a point source) of light, only the umbra is cast. These names are most often used for the shadows cast by celestial bodies, though they are sometimes used to describe levels, such as in sunspots. Umbra The umbra (Latin for "shadow") is the innermost and darkest part of a shadow, where the light source is completely blocked by the occluding body. An observer within the umbra experiences a total eclipse. The umbra of a round body occluding a round light source forms a right circular cone. When viewed from the cone's apex, the two bodies appear the same size. The distance from the Moon to the apex of its umbra is roughly equal to that between the Moon and Earth: . Since Earth's diameter is 3.7 times the Moon's, its umbra extends correspondingly farther: roughly . Penumbra T ...
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