Английская Википедия:1650 Heckmann
1650 Heckmann, provisional designation Шаблон:Mp, is a rare-type Nysian asteroid from the inner regions of the asteroid belt, approximately 29 kilometers in diameter. It was discovered on 11 October 1937, by German astronomer Karl Reinmuth at Heidelberg Observatory in southern Germany, and later named after astronomer Otto Heckmann.[1][2]
Classification and orbit
Heckmann is a member of the Polanian subgroup of the Nysa family of asteroids and shows a rare F-type spectrum in the Tholen classification scheme. It orbits the Sun in the inner main-belt at a distance of 2.0–2.8 AU once every 3 years and 10 months (1,389 days). Its orbit has an eccentricity of 0.16 and an inclination of 3° with respect to the ecliptic.[3] Heckmann was first identified as Шаблон:Mp at the discovering observatory in 1906. Its first used observation was taken at Heidelberg in 1909, when it was identified as Шаблон:Mp, extending the body's observation arc by 28 years prior to its official discovery observation.[2]
Rotation period
French amateur astronomer René Roy obtained the first rotational lightcurve of Heckmann in September 2005. It gave a rotation period of 12.05 hours with a brightness variation of 0.06 in magnitude (Шаблон:Small).[4] A more refined lightcurve with a period of 14.893 hours and an amplitude of 0.16 magnitude was obtained by Australian amateur astronomer David Higgins at the Hunters Hill Observatory and collaborating stations in March 2008 (Шаблон:Small).[5] In September 2013, photometric observations at the Palomar Transient Factory, California, gave a low rated lightcurve with a similar period of 14.9042 hours (Шаблон:Small).[6]
Diameter and albedo
According to the surveys carried out by the Infrared Astronomical Satellite IRAS, the Japanese Akari satellite, and NASA's Wide-field Infrared Survey Explorer with its subsequent NEOWISE mission, Heckmann measures between 24.93 and 35.15 kilometers in diameter, and its surface has an albedo between 0.034 and 0.06.[7][8][9][10][11] The Collaborative Asteroid Lightcurve Link agrees with the results obtained by IRAS, that is an albedo of 0.0497 and a diameter of 29.07 kilometers with an absolute magnitude of 11.56.[12]
Naming
This minor planet was named in honor of German astronomer Otto Heckmann (1901–1983), director of the Bergedorf Observatory in Hamburg, president of the International Astronomical Union (1967–1970) and the first director of ESO, the European Southern Observatory, which foundation had been initiated by him. He was active in the fields of cosmology and several aspects of fundamental astronomy.[1] The official Шаблон:MoMP was published by the Minor Planet Center on 20 February 1976 (Шаблон:Small).[13]
References
External links
- Asteroid Lightcurve Database (LCDB), query form (info Шаблон:Webarchive)
- Dictionary of Minor Planet Names, Google books
- Asteroids and comets rotation curves, CdR – Observatoire de Genève, Raoul Behrend
- Discovery Circumstances: Numbered Minor Planets (1)-(5000) – Minor Planet Center
- Шаблон:AstDys
- Шаблон:JPL small body
Шаблон:Use dmy dates Шаблон:Minor planets navigator Шаблон:Small Solar System bodies
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- Английская Википедия
- Nysa asteroids
- Discoveries by Karl Wilhelm Reinmuth
- Named minor planets
- F-type asteroids (Tholen)
- Astronomical objects discovered in 1937
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