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July 1963 Lunar Eclipse
A partial lunar eclipse occurred at the Moon’s descending node of orbit on Saturday, July 6, 1963, with an umbral magnitude of 0.7060. A lunar eclipse occurs when the Moon moves into the Earth's shadow, causing the Moon to be darkened. A partial lunar eclipse occurs when one part of the Moon is in the Earth's umbra, while the other part is in the Earth's penumbra. Unlike a solar eclipse, which can only be viewed from a relatively small area of the world, a lunar eclipse may be viewed from anywhere on the night side of Earth. Occurring about 5.7 days after apogee (on July 1, 1963, at 6:30 UTC), the Moon's apparent diameter was smaller. Visibility The eclipse was completely visible over Africa, much of Europe, the Middle East, and Antarctica, seen rising over eastern North America, South America, and western Europe and setting over much of Asia and Australia. Eclipse details Shown below is a table displaying details about this particular solar eclipse. It describes various p ... [...More Info...] [...Related Items...] OR: [Wikipedia] [Google] [Baidu] |
Lunar Eclipse
A lunar eclipse is an astronomical event that occurs when the Moon moves into the Earth's shadow, causing the Moon to be darkened. Such an alignment occurs during an eclipse season, approximately every six months, during the full moon phase, when the Moon's orbital plane is closest to Ecliptic, the plane of the Earth's orbit. This can occur only when the Sun, Earth, and Moon are exactly or very closely aligned (in syzygy (astronomy), syzygy) with Earth between the other two, which can happen only on the night of a full moon when the Moon is near either lunar node. The type and length of a lunar eclipse depend on the Moon's proximity to the lunar node. When the Moon is totally eclipsed by the Earth (a "deep eclipse"), "What is a deep eclipse? The smaller star is behind the bigger star" it takes on a reddish color that is caused by the planet when it completely blocks direct sunlight from reaching the Moon's surface, as the only light that is diffuse reflection, reflected from ... [...More Info...] [...Related Items...] OR: [Wikipedia] [Google] [Baidu] |
Lunar Eclipse From Moon-1963Jul06
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'' * Lunar Drive-in Theatre, in Dandenong, Victoria, Australia * Lunars, a fictional race in the series ''The Lunar Chronicles'' by Marissa Meyer Other uses * Lunar dynasty, a legendary house of warrior–rulers in ancient Indian texts * 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 * LUNAR (software) (1970–1972), question-answering system by Bill Woods (computer scientist) See also * * * Lunar calendar, based upon the monthly cycles of the Moon's phase ** Lunar day, in such calendars ** Lunar ... [...More Info...] [...Related Items...] OR: [Wikipedia] [Google] [Baidu] |
May 1956 Lunar Eclipse
A partial lunar eclipse occurred at the Moon’s ascending node of orbit on Thursday, May 24, 1956, with an umbral magnitude of 0.9647. A lunar eclipse occurs when the Moon moves into the Earth's shadow, causing the Moon to be darkened. A partial lunar eclipse occurs when one part of the Moon is in the Earth's umbra, while the other part is in the Earth's penumbra. Unlike a solar eclipse, which can only be viewed from a relatively small area of the world, a lunar eclipse may be viewed from anywhere on the night side of Earth. Occurring about 4.3 days before apogee (on May 28, 1956, at 22:10 UTC), the Moon's apparent diameter was smaller. This lunar eclipse was the first of an almost tetrad, with the others being on November 18, 1956 (total); May 13, 1957 (total); and November 7, 1957 (total). This was the first eclipse of the last partial set in Lunar Saros 120. Visibility The eclipse was completely visible over east Asia, Australia, and Antarctica, seen rising over centr ... [...More Info...] [...Related Items...] OR: [Wikipedia] [Google] [Baidu] |
April 1967 Lunar Eclipse
A total lunar eclipse occurred at the Moon’s descending node of orbit on Monday, April 24, 1967, with an umbral magnitude of 1.3356. A lunar eclipse occurs when the Moon moves into the Earth's shadow, causing the Moon to be darkened. A total lunar eclipse occurs when the Moon's near side entirely passes into the Earth's umbral shadow. Unlike a solar eclipse, which can only be viewed from a relatively small area of the world, a lunar eclipse may be viewed from anywhere on the night side of Earth. A total lunar eclipse can last up to nearly two hours, while a total solar eclipse lasts only a few minutes at any given place, because the Moon's shadow is smaller. Occurring only about 16 hours after perigee (on April 23, 1967, at 20:00 UTC), the Moon's apparent diameter was larger. This lunar eclipse was the first of a tetrad, with four total lunar eclipses in series, the others being on October 18, 1967; April 13, 1968; and October 6, 1968. The Surveyor 3 probe was active on the M ... [...More Info...] [...Related Items...] OR: [Wikipedia] [Google] [Baidu] |
September 1959 Lunar Eclipse
A penumbral lunar eclipse occurred at the Moon’s Lunar node, descending node of orbit on Thursday, September 17, 1959, with an umbral Magnitude of eclipse, magnitude of −0.0495. A lunar eclipse occurs when the Moon moves into the Earth's shadow, causing the Moon to be darkened. A penumbral lunar eclipse occurs when part or all of the Moon's near side passes into the Earth's penumbra. Unlike a solar eclipse, which can only be viewed from a relatively small area of the world, a lunar eclipse may be viewed from anywhere on the night side of Earth. Occurring about 6.1 days before Apsis, apogee (on September 23, 1959, at 2:30 UTC), the Moon's apparent diameter was smaller. Visibility The eclipse was completely visible over South America, Africa, and Europe, seen rising over North America and the eastern Pacific Ocean and setting over the western half of Asia. Eclipse details Shown below is a table displaying details about this particular solar eclipse. It describes various pa ... [...More Info...] [...Related Items...] OR: [Wikipedia] [Google] [Baidu] |
December 1963 Lunar Eclipse
A total lunar eclipse occurred at the Moon’s Lunar node, ascending node of orbit on Monday, December 30, 1963, with an umbral Magnitude of eclipse, magnitude of 1.3350. A lunar eclipse occurs when the Moon moves into the Earth's shadow, causing the Moon to be darkened. A total lunar eclipse occurs when the Moon's near side entirely passes into the Earth's umbral shadow. Unlike a solar eclipse, which can only be viewed from a relatively small area of the world, a lunar eclipse may be viewed from anywhere on the night side of Earth. A total lunar eclipse can last up to nearly two hours, while a total solar eclipse lasts only a few minutes at any given place, because the Moon's Umbra, penumbra and antumbra, shadow is smaller. Occurring about 1.5 days after Apsis, perigee (on December 29, 1963, at 0:10 UTC), the Moon's apparent diameter was larger. Visibility The eclipse was completely visible over northeast Asia and much of North America, seen rising over much of Asia and Australi ... [...More Info...] [...Related Items...] OR: [Wikipedia] [Google] [Baidu] |
Solar Eclipse Of January 25, 1963
An annular solar eclipse occurred at the Moon's descending node of orbit on Friday, January 25, 1963, with a magnitude of 0.9951. 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 (ring). An annular eclipse appears as a partial eclipse over a region of the Earth thousands of kilometres wide. The Moon's apparent diameter was near the average diameter because it occurred 8.2 days after apogee (on January 17, 1963, at 8:00 UTC) and 3.7 days before perigee (on January 29, 1963, at 7:20 UTC). The moon's apparent diameter was 4.8 arcseconds larger than the July 20, 1963 total solar eclipse. This was an annular solar eclipse because it occurred in January and the earth is near its perihelion (closest approach to the Sun) ... [...More Info...] [...Related Items...] OR: [Wikipedia] [Google] [Baidu] |
January 1963 Lunar Eclipse
A penumbral lunar eclipse occurred at the Moon’s ascending node of orbit on Wednesday, January 9, 1963, with an umbral magnitude of −0.0184. It was a relatively rare total penumbral lunar eclipse, with the Moon passing entirely within the penumbral shadow without entering the darker umbral shadow. A lunar eclipse occurs when the Moon moves into the Earth's shadow, causing the Moon to be darkened. A penumbral lunar eclipse occurs when part or all of the Moon's near side passes into the Earth's penumbra. Unlike a solar eclipse, which can only be viewed from a relatively small area of the world, a lunar eclipse may be viewed from anywhere on the night side of Earth. Occurring about 5.6 days after perigee (on January 4, 1963, at 8:25 UTC), the Moon's apparent diameter was larger. Visibility The eclipse was completely visible over northeastern North America, Europe, Africa, and the western half of Asia, seen rising over North and South America and setting over east and southeast ... [...More Info...] [...Related Items...] OR: [Wikipedia] [Google] [Baidu] |
Total Eclipse
An eclipse is an astronomical event which occurs when an astronomical object or spacecraft is temporarily obscured, by passing into the shadow of another body or by having another body pass between it and the viewer. This alignment of three celestial objects is known as a ''syzygy''. An eclipse is the result of either an '' occultation'' (completely hidden) or a ''transit'' (partially hidden). A "deep eclipse" (or "deep occultation") is when a small astronomical object is behind a bigger one. "What is a deep eclipse? The smaller star is behind the bigger star" The term ''eclipse'' is most often used to describe either a solar eclipse, when the Moon's shadow crosses the Earth's surface, or a lunar eclipse, when the Moon moves into the Earth's shadow. However, it can also refer to such events beyond the Earth–Moon system: for example, a planet moving into the shadow cast by one of its moons, a moon passing into the shadow cast by its host planet, or a moon passing into the ... [...More Info...] [...Related Items...] OR: [Wikipedia] [Google] [Baidu] |
Lunar Eclipse
A lunar eclipse is an astronomical event that occurs when the Moon moves into the Earth's shadow, causing the Moon to be darkened. Such an alignment occurs during an eclipse season, approximately every six months, during the full moon phase, when the Moon's orbital plane is closest to Ecliptic, the plane of the Earth's orbit. This can occur only when the Sun, Earth, and Moon are exactly or very closely aligned (in syzygy (astronomy), syzygy) with Earth between the other two, which can happen only on the night of a full moon when the Moon is near either lunar node. The type and length of a lunar eclipse depend on the Moon's proximity to the lunar node. When the Moon is totally eclipsed by the Earth (a "deep eclipse"), "What is a deep eclipse? The smaller star is behind the bigger star" it takes on a reddish color that is caused by the planet when it completely blocks direct sunlight from reaching the Moon's surface, as the only light that is diffuse reflection, reflected from ... [...More Info...] [...Related Items...] OR: [Wikipedia] [Google] [Baidu] |
Solar Eclipse Of July 20, 1963
A total solar eclipse occurred at the Moon's Lunar node, ascending node of orbit between Saturday, July 20 and Sunday, July 21, 1963, with a Magnitude of eclipse, magnitude of 1.0224. 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 at least the same size as the Sun's or larger, blocking all direct sunlight, turning day into darkness. Totality occurs in a narrow path across Earth's surface, with a partial solar eclipse visible over the surrounding region thousands of kilometres wide. Occurring about 4.1 days after Apsis, perigee (on July 16, 1963, at 19:20 UTC), the Moon's apparent diameter was larger. Astronomer Charles H. Smiley observed the eclipse from a U.S. Air Force Lockheed F-104 Starfighter, F-104D Starfighter supersonic aircraft that was "racing the Moon's shadow" at extending the duration of totality to ... [...More Info...] [...Related Items...] OR: [Wikipedia] [Google] [Baidu] |
