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Lyudmila Chernykh
Lyudmila Ivanovna Chernykh (russian: Людми́ла Ива́новна Черны́х, June 13, 1935 in Shuya, Ivanovo Oblast, Shuya, Ivanovo Oblast – July 28, 2017) was a Russian-born Soviet Union, Soviet astronomer, wife and colleague of Nikolai Stepanovich Chernykh, and a prolific discoverer of minor planets. Professional career In 1959 she graduated from Pedagogical Institute of Irkutsk State University, Irkutsk State Pedagogical Institute (now Pedagogical Institute of Irkutsk State University). Between 1959 and 1963 she worked in the Time and Frequency Laboratory of the All-Union Research Institute of Physico-Technical and Radiotechnical Measurements in Irkutsk, where she did astrometry, astrometrical observations for the Time Service. Between 1964 and 1998 she was a scientific worker at the Institute of Theoretical Astronomy of the USSR Academy of Sciences (Russian Academy of Science since 1991), working at the observation base of the institute at the Crimean Astroph ... [...More Info...] [...Related Items...] OR: [Wikipedia] [Google] [Baidu] |
Minor Planet
According to the International Astronomical Union (IAU), a minor planet is an astronomical object in direct orbit around the Sun that is exclusively classified as neither a planet nor a comet. Before 2006, the IAU officially used the term ''minor planet'', but that year's meeting reclassified minor planets and comets into dwarf planets and small Solar System bodies (SSSBs).Press release, IAU 2006 General Assembly: Result of the IAU Resolution votes International Astronomical Union, August 24, 2006. Accessed May 5, 2008. Minor planets include asteroids ( |
Tamara Smirnova
Tamara Mikhaylovna Smirnova (russian: Тама́ра Миха́йловна Смирно́ва; 1935–2001) was a Soviet Union, Soviet/Russian astronomer and a discoverer of minor planets and comets. Career From 1966 to 1988, Smirnova was a staff member of the Institute of Theoretical Astronomy at Saint Petersburg, Leningrad. She is credited by the Minor Planet Center with the discovery of 135 numbered minor planets during 1966–1984. She also co-discovered the periodic comet 74P/Smirnova-Chernykh, along with Nikolai Stepanovich Chernykh. The main-belt asteroid 5540 Smirnova, discovered by herself in 1971, was named in her honor following a proposal by the ''Institute of Theoretical Astronomy''. Naming citation was published on 17 March 1995 (). List of discovered minor planets See also * References 1935 births 2001 deaths Soviet women scientists Discoverers of asteroids Discoverers of comets Discoveries by Tamara Mikha ... [...More Info...] [...Related Items...] OR: [Wikipedia] [Google] [Baidu] |
1790 Volkov
1790 Volkov, provisional designation , is a stony Florian asteroid from the inner regions of the asteroid belt, approximately 8 kilometers in diameter. It was discovered on 9 March 1967, by Russian astronomer Lyudmila Chernykh at Crimean Astrophysical Observatory in Nauchnyj, on the Crimean peninsula, and named after cosmonaut Vladislav Volkov. Orbit and classification ''Volkov'' is a stony S-type asteroid and member of the Flora family, one of the largest populations of inner main-belt asteroids. It orbits the Sun in the inner main-belt at a distance of 2.0–2.5 AU once every 3 years and 4 months (1,223 days). Its orbit has an eccentricity of 0.10 and an inclination of 5 ° with respect to the ecliptic. First identified as at Heidelberg Observatory, ''Volkov''s observation arc is extended by 41 years prior to its official discovery observation. Physical characteristics Rotation period Two rotational lightcurves of ''Volkov'' were obtained from photometric observ ... [...More Info...] [...Related Items...] OR: [Wikipedia] [Google] [Baidu] |
1789 Dobrovolsky
1789 Dobrovolsky ( ''prov. designation'': ) is a Flora asteroid from the inner regions of the asteroid belt, approximately 8 kilometers in diameter. It was discovered on 19 August 1966, by Russian astronomer Lyudmila Chernykh at the Crimean Astrophysical Observatory in Nauchnyj on the Crimean peninsula. The asteroid was named after cosmonaut Georgy Dobrovolsky. Orbit and classification ''Dobrovolsky'' is a member of the Flora family, a large group of stony S-type asteroids in the inner main-belt. It orbits the Sun in the inner main-belt at a distance of 1.8–2.6 AU once every 3 years and 3 months (1,203 days). Its orbit has an eccentricity of 0.19 and an inclination of 2 ° with respect to the ecliptic. First identified as at Johannesburg, the body's first used observation was taken at Nice Observatory in 1943, when ''Dobrovolsky'' was identified as , extending its observation arc by 23 years prior to its official discovery observation. Naming This minor planet was ... [...More Info...] [...Related Items...] OR: [Wikipedia] [Google] [Baidu] |
1772 Gagarin
1772 Gagarin ( ''prov. designation'': ) is a stony background asteroid from the central region of the asteroid belt, approximately 9 kilometers in diameter. It was discovered on 6 February 1968, by Russian astronomer Lyudmila Chernykh at the Crimean Astrophysical Observatory in Nauchnyj, on the Crimean peninsula. The asteroid was named after cosmonaut Yuri Gagarin. Orbit and classification ''Gagarin'' orbits the Sun in the central main-belt at a distance of 2.3–2.8 AU once every 4.02 years (1,467 days). Its orbit has an eccentricity of 0.11 and an inclination of 6 ° with respect to the ecliptic. ''Gagarin'' first observation is a precovery that was taken at Turku Observatory in 1940, extending the body's observation arc by 28 years prior to its official discovery observation. Physical characteristics ''Gagarin'' has been characterized as a rare L-type asteroid by PanSTARRS photometric survey. Rotation period In February 1984, a rotational lightcurve of ''Gagarin'' ... [...More Info...] [...Related Items...] OR: [Wikipedia] [Google] [Baidu] |
1771 Makover
1771 Makover, provisional designation , is a carbonaceous asteroid from the outer region of the asteroid belt, approximately 50 kilometers in diameter. It was discovered on 24 January 1968, by Russian astronomer Lyudmila Chernykh at the Crimean Astrophysical Observatory in Nauchnyj on the Crimean peninsula. It was named after Russian astronomer Samuel Makover. Orbit and classification The dark C-type asteroid orbits the Sun in the outer main-belt at a distance of 2.6–3.7 AU once every 5 years and 6 months (2,015 days). Its orbit has an eccentricity of 0.18 and an inclination of 11 ° with respect to the ecliptic. At Johannesburg Observatory, ''Makover'' was first identified as in 1937. Its first used observation was made at the same observatory one year later, when it was identified as , extending the body's observation arc by 30 years prior to its official discovery observation. Physical characteristics In December 2011, a rotational lightcurve of ''Makover'' was ... [...More Info...] [...Related Items...] OR: [Wikipedia] [Google] [Baidu] |
1737 Severny
1737 Severny, provisional designation , is a stony Eoan asteroid from the outer region of the asteroid belt, approximately 21 kilometers in diameter. It was discovered on 13 October 1966, by Russian astronomer Lyudmila Chernykh at the Crimean Astrophysical Observatory in Nauchnyj, on the Crimean peninsula, who named after Soviet astronomer Andrei Severny. Classification and orbit ''Severny'' is a member of the Eos family. It orbits the Sun in the outer main-belt at a distance of 2.9–3.2 AU once every 5 years and 3 months (1,908 days). Its orbit has an eccentricity of 0.05 and an inclination of 9 ° with respect to the ecliptic. First identified as at Turku, the asteroid's first used observation was made at Heidelberg Observatory in 1950, extending ''Severny''s observation arc by 16 years prior to its official discovery observation. Physical characteristics ''Severny'' has been characterized as a common stony S-type asteroid. Lightcurves A rotational lightcurv ... [...More Info...] [...Related Items...] OR: [Wikipedia] [Google] [Baidu] |
Apollo Asteroid
The Apollo asteroids are a group of near-Earth asteroids named after 1862 Apollo, discovered by German astronomer Karl Reinmuth in the 1930s. They are Earth-crossing asteroids that have an orbital semi-major axis greater than that of the Earth (a > 1 AU) but perihelion distances less than the Earth's aphelion distance (q < 1.017 AU). , the number of known Apollo asteroids is 10,485, making the class the largest group of s (''cf''. the , Amor and Atira asteroids), [...More Info...] [...Related Items...] OR: [Wikipedia] [Google] [Baidu] |
Near-Earth Object
A near-Earth object (NEO) is any small Solar System body whose orbit brings it into proximity with Earth. By convention, a Solar System body is a NEO if its closest approach to the Sun (perihelion) is less than 1.3 astronomical units (AU). If a NEO's orbit crosses the Earth's orbit, and the object is larger than across, it is considered a potentially hazardous object (PHO). Most known PHOs and NEOs are asteroids, but a small fraction are comets. There are over 30,503 known near-Earth asteroids (NEAs) and over a hundred known short-period near-Earth comets (NECs). A number of solar-orbiting meteoroids were large enough to be tracked in space before striking the Earth. It is now widely accepted that collisions in the past have had a significant role in shaping the geological and biological history of the Earth. Asteroids as small as in diameter can cause significant damage to the local environment and human populations. Larger asteroids penetrate the atmosphere to the surf ... [...More Info...] [...Related Items...] OR: [Wikipedia] [Google] [Baidu] |
2212 Hephaistos
2212 Hephaistos (1978 SB) is an Apollo asteroid and a NEO discovered on 27 September 1978 by L. I. Chernykh at the Crimean Astrophysical Observatory. It is named after the Greek god Hephaestus. It is the largest member of the Hephaistos asteroid group. It makes close approaches to all of the inner planets and will pass from Mercury Mercury commonly refers to: * Mercury (planet), the nearest planet to the Sun * Mercury (element), a metallic chemical element with the symbol Hg * Mercury (mythology), a Roman god Mercury or The Mercury may also refer to: Companies * Merc ... on 2032-Sep-16. Other potential members of the Hephaistos group include (85182) 1991 AQ, 4486 Mithra, and D/1766 G1 (Helfenzrieder). References External links * * * 002212 Discoveries by Lyudmila Chernykh Named minor planets 002212 19780927 {{NE-asteroid-stub ... [...More Info...] [...Related Items...] OR: [Wikipedia] [Google] [Baidu] |
Tanya Savicheva
Tatyana Nikolayevna Savicheva (russian: Татья́на Никола́евна Са́вичева), commonly referred to as Tanya Savicheva (23 January 1930 – 1 July 1944), was a Russian child diary, diarist who endured the siege of Leningrad during World War II. During the siege, Savicheva recorded the successive deaths of each member of her family in her diary, with her final entry indicating her belief to be the sole living family member. Although Savicheva was rescued and transferred to a hospital, she succumbed to intestinal tuberculosis in July 1944 at age 14. Savicheva's image and the pages from her diary became symbolic of the human cost of the siege of Leningrad, and she is remembered in St. Petersburg with a memorial complex on the Green Belt of Glory along the Road of Life. Her diary was used during the Nuremberg Trials as evidence of the Nazis’ crimes. Early life Savicheva was born on 23 January 1930, the youngest child in the family of a baker father, Nikolay ... [...More Info...] [...Related Items...] OR: [Wikipedia] [Google] [Baidu] |
2127 Tanya
2127 Tanya, provisional designation , is a carbonaceous asteroid from the outer region of the asteroid belt, approximately 40 kilometers in diameter. It was discovered on 29 May 1971, by Russian astronomer Lyudmila Chernykh at the Crimean Astrophysical Observatory in Nauchnij, on the Crimean peninsula. It was named in memory of Tanya Savicheva, a Russian child diarist during World War II. Orbit ''Tanya'' is a carbonaceous C-type asteroid, that orbits the Sun in the outer main-belt at a distance of 3.1–3.3 AU once every 5 years and 9 months (2,101 days). Its orbit has an eccentricity of 0.03 and an inclination of 13 ° with respect to the ecliptic. It was first identified as at Goethe Link Observatory in 1953, extending the body's observation arc by 18 years prior to its official discovery at Nauchnij. Lightcurve In October 2013, a rotational lightcurve of ''Tanya'' was obtained from photometric observations at the Palomar Transient Factory in California. Lightcurve ... [...More Info...] [...Related Items...] OR: [Wikipedia] [Google] [Baidu] |
