Vladimir Albitsky
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Vladimir Albitsky
Vladimir Aleksandrovich Albitzky (russian: Владимир Александрович Альбицкий) (16 June 1891 – 15 June 1952) was a Soviet/Russian astronomer and discoverer of minor planets. In modern English transliteration, his surname would be given as Al'bitskii or Al'bitsky. In the literature, he is sometimes referred to as W. A. Albizkij, however his surname usually appears in the literature as "Albitzky". His asteroid discoveries are credited as "V. Albitskij". He came to the Simeiz Observatory (Симеиз) in Crimea in 1922, working with G. A. Shajn and G. N. Neujmin, and became head of the observatory in 1934. The Minor Planet Center credits him with the discovery of 10 asteroids during 1923–1925. The Eunomia In Greek mythology, Eunomia ( grc, Εὐνομία) was a minor goddess of law and legislation (her name can be translated as "good order", "governance according to good laws"), as well as the spring-time goddess of green pastures (''eû'' means ...
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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 (

1022 Olympiada
1022 Olympiada, provisional designation , is a background asteroid from the central regions of the asteroid belt, approximately in diameter. It was discovered at the Simeiz Observatory on the Crimean peninsula on 23 June 1924, by Soviet astronomer Vladimir Albitsky, who named it after his mother, Olimpiada Albitskaya. The X-type asteroid has a short rotation period of 3.83 hours. Orbit and classification ''Olympiada'' is a non-family asteroid from the main belt's background population. It orbits the Sun in the central asteroid belt at a distance of 2.3–3.3  AU once every 4 years and 8 months (1,716 days; semi-major axis of 2.81 AU). Its orbit has an eccentricity of 0.17 and an inclination of 21 ° with respect to the ecliptic. The body's observation arc begins with its first observation as at Heidelberg Observatory in July 1910, or nearly 14 years prior to its official discovery observation at Simeiz. Naming This minor planet was named after Olimpiada Albits ...
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1952 Deaths
Year 195 ( CXCV) was a common year starting on Wednesday (link will display the full calendar) of the Julian calendar. At the time, it was known as the Year of the Consulship of Scrapula and Clemens (or, less frequently, year 948 ''Ab urbe condita''). The denomination 195 for this year has been used since the early medieval period, when the Anno Domini calendar era became the prevalent method in Europe for naming years. Events By place Roman Empire * Emperor Septimius Severus has the Roman Senate deify the previous emperor Commodus, in an attempt to gain favor with the family of Marcus Aurelius. * King Vologases V and other eastern princes support the claims of Pescennius Niger. The Roman province of Mesopotamia rises in revolt with Parthian support. Severus marches to Mesopotamia to battle the Parthians. * The Roman province of Syria is divided and the role of Antioch Antioch on the Orontes (; grc-gre, Ἀντιόχεια ἡ ἐπὶ Ὀρόντου, ''Antiókhei ...
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1891 Births
Events January–March * January 1 ** Paying of old age pensions begins in Germany. ** A strike of 500 Hungarian steel workers occurs; 3,000 men are out of work as a consequence. **Germany takes formal possession of its new African territories. * January 2 – A. L. Drummond of New York is appointed Chief of the Treasury Secret Service. * January 4 – The Earl of Zetland issues a declaration regarding the famine in the western counties of Ireland. * January 5 **The Australian shearers' strike, that leads indirectly to the foundation of the Australian Labor Party, begins. **A fight between the United States and Indians breaks out near Pine Ridge agency. ** Henry B. Brown, of Michigan, is sworn in as an Associate Justice of the Supreme Court. **A fight between railway strikers and police breaks out at Motherwell, Scotland. * January 6 – Encounters continue, between strikers and the authorities at Glasgow. * January 7 ** General Miles' force ...
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1330 Spiridonia
1330 Spiridonia, provisional designation , is a dark background asteroid of primitive composition, located in the outer regions of the asteroid belt, approximately 65 kilometers in diameter. It was discovered on 17 February 1925, by Soviet astronomer Vladimir Albitsky at the Simeiz Observatory on the Crimean peninsula. The asteroid was named after the discoverer's brother-in-law, Spiridon Zaslavskij. Orbit and classification ''Spiridonia'' is a non-family asteroid from the main belt's background population. It orbits the Sun in the outer asteroid belt at a distance of 2.9–3.4  AU once every 5 years and 8 months (2,061 days; semi-major axis of 3.17 AU). Its orbit has an eccentricity of 0.08 and an inclination of 16 ° with respect to the ecliptic. The asteroid was first identified as at Heidelberg Observatory in September 1922. The body's observation arc begins at Yerkes Observatory in October 1934, more than 9 years after its official discovery observation at Sime ...
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1283 Komsomolia
1283 Komsomolia ( ''prov. designation'': ) is a metallic background asteroid and potentially slow rotator from the outer regions of the asteroid belt. Discovered by Vladimir Albitsky in 1925, it was later named after Komsomol, a political youth organization of the former Soviet Union. The M-type asteroid has roughly a rotation period 96 hours of and measures approximately in diameter. Discovery ''Komsomolia'' was discovered on 25 September 1925, by Soviet astronomer Vladimir Albitsky at the Simeiz Observatory on the Crimean peninsula. It was independently discovered by German astronomer Karl Reinmuth at Heidelberg Observatory on 10 October 1925. Only the first discoverer is officially recognized. The asteroid was first observed as at Heidelberg in October 1902. Orbit and classification ''Komsomolia'' is a non-family asteroid of the main belt's background population when applying the hierarchical clustering method to its proper orbital elements. It orbits the Sun in the ...
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1071 Brita
1071 Brita, provisional designation , is a dark asteroid from the background population of the intermediate asteroid belt, approximately 50 kilometers in diameter. It was discovered on 3 March 1924, by Soviet astronomer Vladimir Albitsky at the Simeiz Observatory on the Crimean peninsula. The asteroid was named after the island of Great Britain. Orbit and classification ''Brita'' is a non-family asteroid from the main belt's background population. It orbits the Sun in the outer rim of the central asteroid belt at a distance of 2.5–3.1  AU once every 4 years and 8 months (1,712 days; semi-major axis of 2.80 AU). Its orbit has an eccentricity of 0.11 and an inclination of 5 ° with respect to the ecliptic. The asteroid was first identified as at Heidelberg Observatory in March 1910. The body's observation arc begins at Lowell Observatory in October 1931, more than 7 years after its official discovery observation Simeiz. Physical characteristics In the SMASS cla ...
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1059 Mussorgskia
1059 Mussorgskia, provisional designation , is a background asteroid from the central regions of the asteroid belt, approximately in diameter. It was discovered on 19 July 1925, by Soviet astronomer Vladimir Albitsky at the Simeiz Observatory on the Crimean peninsula. The asteroid was named for Russian composer Modest Mussorgsky. The X- or C-type asteroid has a rotation period of 5.636 hours. Orbit and classification ''Mussorgskia'' is a non-family asteroid from the main belt's background population. It orbits the Sun in the central asteroid belt at a distance of 2.1–3.1  AU once every 4 years and 3 months (1,567 days; semi-major axis of 2.64 AU). Its orbit has an eccentricity of 0.19 and an inclination of 10 ° with respect to the ecliptic. The asteroid was first observed as at Simeiz in May 1916. The body's observation arc begins as at Heidelberg Observatory in April 1920, or more than 5 years prior to its official discovery observation at Simeiz. Physical ...
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1034 Mozartia
1034 Mozartia, provisional designation , is a stony asteroid from the inner regions of the asteroid belt, approximately 8 kilometers in diameter. It was discovered on 7 September 1924, by Soviet Vladimir Albitsky at Simeiz Observatory on the Crimean peninsula, and named after Wolfgang Amadeus Mozart. Orbit and classification ''Mozartia'' orbits the Sun in the inner main-belt at a distance of 1.7–2.9  AU once every 3 years and 6 months (1,268 days). Its orbit has an eccentricity of 0.26 and an inclination of 4 ° with respect to the ecliptic. The body's observation arc begins with its official discovery observation in 1924. Physical characteristics In the SMASS classification, ''Mozartia'' is a common S-type asteroid. Diameter and albedo According to the survey carried out by NASA's Wide-field Infrared Survey Explorer with its subsequent NEOWISE mission, ''Mozartia'' measures 7.919 kilometers in diameter and its surface has an albedo of 0.250. Lightcurves As of ...
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1030 Vitja
1030 Vitja, provisional designation , is a dark background asteroid from the outer regions of the asteroid belt, approximately in diameter. It was discovered on 25 May 1924, by Soviet–Russian astronomer Vladimir Albitsky at the Simeiz Observatory on the Crimean peninsula. The asteroid was named in honor of Viktor Zaslavskij (1925–1944), a relative of the discoverer. Orbit and classification ''Vitja'' is a non-family asteroid from the main belt's background population. It orbits the Sun in the outer asteroid belt at a distance of 2.7–3.5  AU once every 5 years and 6 months (2,014 days; semi-major axis of 3.12 AU). Its orbit has an eccentricity of 0.12 and an inclination of 15 ° with respect to the ecliptic. The asteroid's first recorded observation was made a week after its official discovery at Heidelberg Observatory in June 1924, while its observation arc begins more than seven years later at Lowell Observatory in October 1931. Naming This minor planet w ...
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1028 Lydina
1028 Lydina, provisional designation , is a carbonaceous background asteroid and member of the Cybele group from the outermost regions of the asteroid belt, approximately in diameter. It was discovered at the Simeiz Observatory on the Crimean peninsula on 6 November 1923, by Soviet astronomer Vladimir Albitsky, who named it after his wife, Lydia Il'inichna Albitskaya. The dark C-type asteroid has a rotation period of 11.68 hours. Orbit and classification ''Lydina'' is a non-family asteroid from the main belt's background population when applying the hierarchical clustering method to its proper orbital elements. Based on osculating Keplerian orbital elements, the asteroid is considered a member of the dynamical Cybele group, which are asteroid with low orbital inclinations and eccentricities, and with a semi-major axis between 3.3 and 3.5  AU, near the 4:7 orbital resonance with Jupiter. It orbits the Sun in the outermost asteroid belt at a distance of 3.0–3.8 AU ...
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1007 Pawlowia
Pawlowia (minor planet designation: 1007 Pawlowia), provisional designation , is a background asteroid from the central regions of the asteroid belt, approximately 20 kilometers in diameter. It was discovered on 5 October 1923, by Soviet astronomer Vladimir Albitsky at the Simeiz Observatory on the Crimean peninsula. The asteroid was named after Russian physiologist and Nobelist Ivan Pavlov. Orbit and classification ''Pawlowia'' is a non-family asteroid from the main belt's background population. It orbits the Sun in the central asteroid belt at a distance of 2.4–3.0  AU once every 4 years and 5 months (1,627 days; semi-major axis of 2.71 AU). Its orbit has an eccentricity of 0.11 and an inclination of 3 ° with respect to the ecliptic. The asteroid was first imaged on a precovery taken at Lowell Observatory in December 1906. The body's observation arc begins at Simeiz on 30 October 1925, or 25 days after its official discovery observation (discovery record not li ...
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