Английская Википедия:764 Gedania

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764 Gedania (prov. designation: Шаблон:Mp or Шаблон:Mp) is a large background asteroid from the outer regions of the asteroid belt, approximately Шаблон:Convert in diameter. It was discovered on 26 September 1913, by German astronomer Franz Kaiser at the Heidelberg-Königstuhl State Observatory in southwest Germany. The carbonaceous C-type asteroid has a rotation period of 24.98 hours. It was named after the Polish city of Gdańsk where the discoverer was an assistant at the observatory during the 1920s.

Orbit and classification

Gedania 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 outer asteroid belt at a distance of 2.9–3.5 AU once every 5 years and 9 months (2,092 days; semi-major axis of 3.2 AU). Its orbit has an eccentricity of 0.09 and an inclination of 10° with respect to the ecliptic. The body's observation arc begins with its first observation as Шаблон:Mp at Heidelberg Observatory in November 1902, almost 11 years prior to its official discovery observation by Franz Kaiser.

Naming

This minor planet was named after the Latin name of the city of Gdańsk, Poland (formerly Free City of Danzig) where the discoverer, Franz Kaiser (1891–1962), was an assistant at the observatory during the early 1920s. The official naming citation was mentioned in The Names of the Minor Planets by Paul Herget in 1955 (Шаблон:Small). Asteroid 1419 Danzig was also named by its German name for the city of Gdańsk.

Physical characteristics

In the Tholen classification, Gedania is a common carbonaceous C-type asteroid. It has also been classified as an hydrated Ch-type and as a Caa type in the Tholen- and SMASS-like taxonomic variant of the Small Solar System Objects Spectroscopic Survey (S3OS2).

Rotation period

In February 2006, a rotational lightcurve of Gedania was obtained from photometric observations by collaborating astronomers Roberto Crippa, Federico Manzini Шаблон:Obscode, René Roy, Donn Starkey, Raoul Behrend and Laurent Bernasconi. Lightcurve analysis gave a rotation period of Шаблон:Val hours with a brightness variation of Шаблон:Val magnitude (Шаблон:Small). Observations by Aznar, Brinsfield and Pál, gave an alternative period determination of Шаблон:Val, Шаблон:Val and Шаблон:Val hours, respectively (Шаблон:Small).

Diameter and albedo

According to the surveys carried out by the Infrared Astronomical Satellite IRAS, the NEOWISE mission of NASA's Wide-field Infrared Survey Explorer and the Japanese Akari satellite, Gedania measures Шаблон:Val, Шаблон:Val and Шаблон:Val kilometers in diameter and its surface has an albedo of Шаблон:Val, Шаблон:Val and Шаблон:Val, respectively. The Collaborative Asteroid Lightcurve Link derives an albedo of 0.0754 and a diameter of 58.18 kilometers based on an absolute magnitude of 9.6. An alternative mean-diameter measurement published by the WISE team gave (Шаблон:Val) with corresponding albedo of (Шаблон:Val). On 5 February 2006, an asteroid occultation of Gedania gave a best-fit ellipse dimension of (Шаблон:Val), with a poor quality rating of 1. These timed observations are taken when the asteroid passes in front of a distant star.

External links

• Lightcurve Database Query (LCDB), at www.minorplanet.info
• Dictionary of Minor Planet Names, Google books
• Asteroids and comets rotation curves, CdR – Geneva Observatory, Raoul Behrend
• Discovery Circumstances: Numbered Minor Planets (1)-(5000) – Minor Planet Center
• Шаблон:AstDys
• Шаблон:JPL small body