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March 1941 Lunar Eclipse
A partial lunar eclipse occurred at the Moon’s ascending node of orbit on Thursday, March 13, 1941, with an umbral magnitude of 0.3226. 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 1.5 days before perigee (on March 14, 1941, at 23:05 UTC), the Moon's apparent diameter was larger. Visibility The eclipse was completely visible over northeast Asia, eastern Australia, and western North America, seen rising over much of Asia and western Australia and setting over much of North and South America. Eclipse details Shown below is a table displaying details about this particular solar eclipse. It describes various parame ... [...More Info...] [...Related Items...] OR: [Wikipedia] [Google] [Baidu] |
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's orbit. This can occur only when the Sun, Earth, and Moon are exactly or very closely aligned (in 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, it takes on a reddish color that is caused by the planet when it completely blocks direct sunlight from reaching the Moon surface, as only the light reflected from the lunar surface has been refracted by Earth's atmosphere. This light appears reddish due to the Rayleigh scattering of blue light, the same reason sunrise and sunsets are more orange than during the day. ... [...More Info...] [...Related Items...] OR: [Wikipedia] [Google] [Baidu] |
March 1941 Lunar Eclipse
A partial lunar eclipse occurred at the Moon’s ascending node of orbit on Thursday, March 13, 1941, with an umbral magnitude of 0.3226. 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 1.5 days before perigee (on March 14, 1941, at 23:05 UTC), the Moon's apparent diameter was larger. Visibility The eclipse was completely visible over northeast Asia, eastern Australia, and western North America, seen rising over much of Asia and western Australia and setting over much of North and South America. Eclipse details Shown below is a table displaying details about this particular solar eclipse. It describes various parame ... [...More Info...] [...Related Items...] OR: [Wikipedia] [Google] [Baidu] |
April 1930 Lunar Eclipse
A partial 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 Sunday, April 13, 1930. Visibility Related lunar eclipses Saros series Lunar Saros 111, repeating every 18 years and 11 days, has a total of 71 lunar eclipse events including 11 total lunar eclipses. The first total lunar eclipse of this series was on April 19, 1353, and last was on August 4, 1533. The longest occurrence of this series was on June 12, 1443 when the totality lasted 106 minutes. See also * List of lunar eclipses * List of 20th-century lunar eclipses Notes External links * {{DEFAULTSORT:Lunar eclipse 1930-04 1930-04 1930 in science ... [...More Info...] [...Related Items...] OR: [Wikipedia] [Google] [Baidu] |
Solar Eclipse Of March 18, 1950
An annular solar eclipse occurred on March 18, 1950. 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. While it was an annular solar eclipse, it was a ''non-central'' solar eclipse (when the gamma is 0.9972 or larger). Related eclipses Solar eclipses of 1950–1953 Saros 119 It is a part of Saros cycle 119, repeating every 18 years, 11 days, ... [...More Info...] [...Related Items...] OR: [Wikipedia] [Google] [Baidu] |
Solar Eclipse Of March 7, 1932
An annular solar eclipse occurred on March 7, 1932. 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. Related eclipses Solar eclipses 1931–1935 Saros 119 It is a part of Saros cycle 119, repeating every 18 years, 11 days, containing 71 events. The series started with partial solar eclipse on May 15, 850 AD. It contains total eclipses on Augu ... [...More Info...] [...Related Items...] OR: [Wikipedia] [Google] [Baidu] |
April 1948 Lunar Eclipse
A partial lunar eclipse took place on Friday, April 23, 1948. A tiny bite out of the Moon may have been visible at maximum, though just exactly 2.3% of the Moon was shadowed in a partial eclipse which lasted for 34 minutes and 18 seconds. A shading across the moon from the Earth's penumbral shadow should have been visible at maximum eclipse. Visibility Related lunar eclipses Lunar year series Saros series Lunar Saros 111, repeating every 18 years and 11 days, has a total of 71 lunar eclipse events including 11 total lunar eclipses. The first total lunar eclipse of this series was on April 19, 1353, and last was on August 4, 1533. The longest occurrence of this series was on June 12, 1443 when the totality lasted 106 minutes. 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 annula ... [...More Info...] [...Related Items...] OR: [Wikipedia] [Google] [Baidu] |
January 1934 Lunar Eclipse
A partial lunar eclipse occurred at the Moon’s descending node of orbit on Tuesday, January 30, 1934, with an umbral magnitude of 0.1120. 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 2.9 days after apogee (on January 27, 1934, at 18:55 UTC), the Moon's apparent diameter was smaller. Visibility The eclipse was completely visible over Asia and Australia, seen rising over Africa and Europe and setting over western North America and the central Pacific Ocean. Eclipse details Shown below is a table displaying details about this particular solar eclipse. It describes various parameters pertaining to this eclipse. ... [...More Info...] [...Related Items...] OR: [Wikipedia] [Google] [Baidu] |
December 1944 Lunar Eclipse
A penumbral lunar eclipse took place on Friday, December 29, 1944. In a rare total penumbral eclipse, the entire Moon was partially shaded by the Earth (though none of it was in complete shadow), and the shading across the Moon should have been quite visible at maximum eclipse. The penumbral phase lasted for 4 hours and 27 minutes in all, though for most of it, the eclipse was extremely difficult or impossible to see. Visibility Related lunar eclipses Lunar year series Saros series Lunar Saros series 114, repeating every 18 years and 11 days, has a total of 71 lunar eclipse events including 13 total lunar eclipses. First Penumbral Lunar Eclipse: 0971 May 13 First Partial Lunar Eclipse: 1115 Aug 07 First Total Lunar Eclipse: 1458 Feb 28 First Central Lunar Eclipse: 1530 Apr 12 Greatest Eclipse of Lunar Saros 114: 1584 May 24 Last Central Lunar Eclipse: 1638 Jun 26 Last Total Lunar Eclipse: 1674 Jul 17 Last Partial Lunar Eclipse: 1890 Nov 26 Last Penumbral Lunar Ecli ... [...More Info...] [...Related Items...] OR: [Wikipedia] [Google] [Baidu] |
May 1937 Lunar Eclipse
A penumbral lunar eclipse occurred at the Moon’s ascending node of orbit on Tuesday, May 25, 1937, with an umbral magnitude of −0.3033. 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 only about 18 hours after apogee (on May 24, 1937, at 13:30 UTC), the Moon's apparent diameter was smaller. Visibility The eclipse was completely visible over much of North America, western and central South America, and Antarctica, seen rising over Australia and setting over northeastern North America, eastern South America, and west Africa. Eclipse details Shown below is a table displaying details about this particular solar eclipse. It describes various par ... [...More Info...] [...Related Items...] OR: [Wikipedia] [Google] [Baidu] |
Solar Eclipse Of September 21, 1941
A total solar eclipse occurred on September 21, 1941. 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. The path of totality crossed the Soviet Union (today's Russia, Kazakhstan and Kyrgyzstan), China, Taiwan, Okinawa Prefecture and South Seas Mandate (the parts now belonging to Northern Mariana and Marshall Islands) in Japan Japan ( ja, 日本, or , and formally , ''Nihonkoku'') is an island country in East Asia. It is situated in the northwest Pacific Ocean, and is bordered on the west by the Sea of Japan, while extending from the Sea of Okhotsk in the north ..., and ... [...More Info...] [...Related Items...] OR: [Wikipedia] [Google] [Baidu] |
September 1941 Lunar Eclipse
A partial lunar eclipse took place on Friday, September 5, 1941. It was a shallow partial lunar eclipse, with less than 10% of the Moon covered in Earth's shadow. Fortnight Aug 31, 1941 = Sunday Sep 1, 1941 = Monday Sep 2, 1941 = Tuesday Sep 3, 1941 = Wednesday Sep 4, 1941 = Thursday Sep 5, 1941 = Friday Sep 6, 1941 = Saturday Sep 7, 1941 = Sunday Sep 8, 1941 = Monday Sep 9, 1941 = Tuesday Sep 10, 1941 = Wednesday Sep 11, 1941 = Thursday Sep 12, 1941 = Friday Sep 13, 1941 = Saturday 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, Chapter 18, ''The half-saros'' This lunar eclipse is related to two total solar eclipses of Solar Saros 124. See also *List of lunar eclipses and List of 21st-century lunar eclipses There will be 230 lunar eclipses in the 21st century (2001–2100): 87 p ... [...More Info...] [...Related Items...] OR: [Wikipedia] [Google] [Baidu] |
Total Eclipse
An eclipse is an astronomical event that 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. Apart from syzygy, the term eclipse is also used when a spacecraft reaches a position where it can observe two celestial bodies so aligned. An eclipse is the result of either an occultation (completely hidden) or a transit (partially hidden). 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 shadow of another moon. A binary star system can a ... [...More Info...] [...Related Items...] OR: [Wikipedia] [Google] [Baidu] |
