Eugène Joseph Delporte
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Eugène Joseph Delporte
Eugène Joseph Delporte (10 January 1882 – 19 October 1955) was a Belgian astronomer born in Genappe. He discovered a total of sixty-six asteroids. Notable discoveries include 1221 Amor (which lent its name to the Amor asteroids) and the Apollo asteroid 2101 Adonis. He discovered or co-discovered some comets as well, including periodic comet 57P/du Toit-Neujmin-Delporte. He worked in the Observatoire Royal de Belgique (Belgian Royal Observatory), situated in the town of Uccle (after which the asteroid 1276 Ucclia is named). He started there in 1903 after receiving his doctorate that year from the Free University of Brussels. In 1930 he drew the modern boundaries between all of the constellations in the sky, along lines of right ascension and declination for the epoch B1875.0. The Florian asteroid 1274 Delportia 1274 Delportia, provisional designation , is a stony Florian asteroid from the inner regions of the asteroid belt, approximately 10 kilometers in diame ...
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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 (

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Constellation
A constellation is an area on the celestial sphere in which a group of visible stars forms Asterism (astronomy), a perceived pattern or outline, typically representing an animal, mythological subject, or inanimate object. The origins of the earliest constellations likely go back to prehistory. People used them to relate stories of their beliefs, experiences, creation myth, creation, or mythology. Different cultures and countries adopted their own constellations, some of which lasted into the early 20th century before today's constellations were internationally recognized. The recognition of constellations has changed significantly over time. Many changed in size or shape. Some became popular, only to drop into obscurity. Some were limited to a single culture or nation. The 48 traditional Western constellations are Greek. They are given in Aratus' work ''Phenomena'' and Ptolemy's ''Almagest'', though their origin probably predates these works by several centuries. Constellation ...
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1170 Siva
1170 Siva, provisional designation , is a stony Phocaea asteroid and large Mars-crosser from the innermost regions of the asteroid belt, approximately 10 kilometers in diameter. It was discovered on 29 September 1930, by Belgian astronomer Eugène Delporte at Uccle Observatory in Belgium, and later named after the Hindu deity Shiva. Orbit and classification ''Siva'' is a Mars-crossing asteroid, as it crosses the orbit of Mars at 1.666  AU. It is also a member of the Phocaea family (). It orbits the Sun at a distance of 1.6–3.0  AU once every 3 years and 7 months (1,296 days). Its orbit has an eccentricity of 0.30 and an inclination of 22 ° with respect to the ecliptic. ''Siva'' was first observed at the Japanese Kwasan Observatory, 3 days prior to is discovery. The body's observation arc begins at Uccle, two weeks after its official discovery observation. Naming This minor planet is named after Shiva, a Hindu deity often depicted with a third eye on his forehea ...
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1168 Brandia
1168 Brandia, provisional designation , is a stony Eunomian asteroid from the central regions of the asteroid belt, approximately 10 kilometers in diameter. Discovered by astronomer Eugène Delporte at Uccle Observatory in 1930, the asteroid was later named after mathematician Eugène Brand. Discovery ''Brandia'' was discovered on 25 August 1930, by astronomer Eugène Delporte at the Royal Observatory of Belgium in Uccle. Six nights later, the asteroid was independently discovered by Soviet astronomer Grigory Neujmin at Simeiz Observatory on 31 August 1930. The Minor Planet Center, however, only recognizes the first discoverer. The body's observation arc begins at Uccle, two nights after its official discovery observation. Orbit and classification This asteroid is a member of the Eunomia family (), a prominent family of stony asteroids and the largest one in the intermediate main belt with more than 5,000 members. ''Brandia'' orbits the Sun in the central main-belt at a ...
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1145 Robelmonte
1145 Robelmonte, provisional designation , is a Vestian asteroid from the inner regions of the asteroid belt, approximately 23 kilometers in diameter. It was discovered on 3 February 1929, by Belgian astronomer Eugène Delporte at the Royal Observatory of Belgium in Uccle. Through a glitch in the naming process, the asteroid received the name "Robelmonte" instead of "Mimi" as originally intended by the discoverer. Orbit and classification ''Robelmonte'' is a member of the Vesta family (), the main-belt's second-largest asteroid family by number of members. Vestian asteroids have a composition akin to the HED meteorites and are thought to have originated deep within 4 Vesta's crust, possibly from Rheasilvia, a large impact crater on its southern hemisphere near the South pole, formed as a result of a subcatastrophic collision. Vesta is the main belt's second-largest and second-most-massive body after Ceres. ''Robelmonte'' orbits the Sun in the inner main-belt at a dista ...
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1128 Astrid
1128 Astrid, provisional designation , is a carbonaceous Astridian asteroid from the central region of the asteroid belt. It is the parent body of the Astrid family and measures approximately 40 kilometers in diameter. The asteroid was discovered by Belgian astronomer Eugène Delporte at the Royal Observatory of Belgium in Uccle on 10 March 1929, and later named for Astrid of Sweden, Queen consort of the Belgians. Orbit and classification ''Astrid'' is the parent body of the Astrid family (), a smaller asteroid family of nearly 500 carbonaceous members. It is located in the outermost central main-belt, near a prominent Kirkwood gap, that marks the 5:2 orbital resonance with Jupiter, and divides the asteroid belt into a central and outer part. ''Astrid'' orbits the Sun at a distance of 2.7–2.9  AU once every 4 years and 8 months (1,700 days). Its orbit has an eccentricity of 0.05 and an inclination of 1 ° with respect to the ecliptic. The asteroid was first identi ...
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1124 Stroobantia
1124 Stroobantia, provisional designation , is a metallic asteroid from the outer region of the asteroid belt, approximately 25 kilometers in diameter. It was discovered on 6 October 1928, by Belgian astronomer Eugène Delporte at Uccle Observatory in Belgium. It is named for astronomer Paul Stroobant. Description ''Stroobantia'' orbits the Sun at a distance of 2.8–3.0  AU once every 5.01 years (1,829 days). Its orbit has an eccentricity of 0.03 and an inclination of 8 ° with respect to the ecliptic. First identified as at Heidelberg in 1926, the asteroid's observation arc begins at Algiers Observatory in 1931, or three years after its official discovery observation at Uccle. Physical characteristics In the Tholen taxonomy, ''Stroobantia'' is classified as a generic X-type asteroid. It was grouped it into the metallic subcategory of M-type asteroid by a spectroscopic survey of X-type asteroids using the TNG, NTT and IRTF telescopes. Rotation period Two fragme ...
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1122 Neith
1122 Neith ,that is, pronounced with two syllables, ''NEE-ith''. provisional designation , is a background asteroid from the central region of the asteroid belt, approximately 12 kilometers in diameter. It was discovered by Belgian astronomer Eugène Delporte at the Royal Observatory of Belgium in Uccle on 17 September 1928. The asteroid was named after the goddess Neith from Egyptian mythology. Orbit and classification ''Neith'' 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 1.9–3.3  AU once every 4 years and 3 months (1,536 days; semi-major axis of 2.61 AU). Its orbit has an eccentricity of 0.26 and an inclination of 5 ° with respect to the ecliptic. The body's observation arc begins with its observation as at Heidelberg Observatory in November 1924, almost four years prior to its official discovery observation at Uccle. Physical characteristics ''Neith'' has been characte ...
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1068 Nofretete
1068 Nofretete (), provisional designation , is a stony asteroid from the background population in the outer asteroid belt, approximately 23 kilometers in diameter. It was discovered on 13 September 1926, by Belgian astronomer Eugène Delporte at the Royal Observatory of Belgium in Uccle. The asteroid was named after the Ancient Egyptian Queen Nefertiti by its German name "Nofretete". The near-Earth asteroid 3199 Nefertiti is also named after her. Orbit and classification ''Nofretete'' 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 2.6–3.2  AU once every 4 years and 12 months (1,810 days; semi-major axis of 2.91 AU). Its orbit has an eccentricity of 0.10 and an inclination of 5 ° with respect to the ecliptic. The body's observation arc begins at Uccle in September 1926, three nights after its official discovery observation. Physical characteristics ''Nofretete'' has bee ...
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1052 Belgica
1052 Belgica, provisional designation , is a binary Florian asteroid from the inner regions of the asteroid belt, approximately 10 kilometers in diameter. It was discovered on 15 November 1925, by Belgian astronomer Eugène Delporte at Uccle Observatory in Belgium. It was the first minor planet discovered at Uccle Observatory, after which the minor planet 1276 Ucclia was named. 1052 is named after the Western European state of Belgium. Classification and orbit ''Belgica'' is a member of the Flora family, one of the largest groups of stony asteroids in the main-belt. It orbits the Sun at a distance of 1.9–2.6  AU once every 3 years and 4 months (1,222 days). Its orbit has an eccentricity of 0.14 and an inclination of 5 ° with respect to the ecliptic. ''Belgica'' was first identified as at Heidelberg in 1908. The body's observation arc begins with its first used observation taken at Uccle/Bergedorf in 1933, or 8 years after its official discovery at Uccle. Physical c ...
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Delporte (crater)
Delporte is a lunar impact crater on the far side of the Moon. It overlies part of the northwestern rim of the huge walled plain Fermi, and the crater Litke is nearly attached to the southeastern rim. The crater is named after Eugène Joseph Delporte Eugène Joseph Delporte (10 January 1882 – 19 October 1955) was a Belgian astronomer born in Genappe. He discovered a total of sixty-six asteroids. Notable discoveries include 1221 Amor (which lent its name to the Amor asteroids) and th .... The rim of this crater is only marginally worn, although it is not quite circular and the edge is somewhat uneven. There is a shelf running along the northern inner wall. At the midpoint is a central ridge that extends to the northward. See also * 1274 Delportia, minor planet References * * * * * * * * * * * * Impact craters on the Moon {{Craters on the Moon: C-F ...
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1274 Delportia
1274 Delportia, provisional designation , is a stony Florian asteroid from the inner regions of the asteroid belt, approximately 10 kilometers in diameter. It was discovered on 28 November 1932, by Belgian astronomer Eugène Delporte at Uccle Observatory in Belgium. It was named after the discoverer himself. Orbit and classification ''Delportia'' is a stony S-type asteroid on the Tholen taxonomic scheme. As a member of the Flora family, one of the largest families of the main belt, 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 (1,216 days). Its orbit has an eccentricity of 0.11 and an inclination of 4 ° with respect to the ecliptic. It was first identified as at Heidelberg Observatory in 1918. The body's observation arc begins 6 years prior to its official discovery observation at Uccle, when it was identified as at Heidelberg in 1926. Physical characteristics Rotation period A rotational light curve of '' ...
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