Английская Википедия:1805 Dirikis
1805 Dirikis, provisional designation Шаблон:Mp, is a stony Themistian asteroid from the outer region of the asteroid belt, approximately 26 kilometers in diameter.
It was discovered on 1 April 1970, by Russian astronomer Lyudmila Chernykh at the Crimean Astrophysical Observatory in Nauchnyj on the Crimean peninsula.[1] It was named for Latvian astronomer Matiss Dirikis.[2]
Orbit and classification
The S-type asteroid is a member of the Themis family,[3] a dynamical population of outer-belt asteroids with nearly coplanar ecliptical orbits. It orbits the Sun at a distance of 2.8–3.5 AU once every 5 years and 7 months (2,034 days). Its orbit has an eccentricity of 0.11 and an inclination of 3° with respect to the ecliptic.[4]
It was first observed at the Finnish Turku Observatory during WWII in 1942. The body's first used observation was its identification as Шаблон:Mp at Goethe Link Observatory in 1955, extending the asteroid's observation arc by 15 years prior to its official discovery observation.[1]
Physical characteristics
Rotation period
A rotational lightcurve of Dirikis was obtained from photometric observations taken by French amateur astronomer René Roy In April 2003. It gave a rotation period of 23.0 hours with a brightness variation of 0.45 magnitude (Шаблон:Small).[5] A 2013-published period of 23.45 hours was derived in an international study (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, Dirikis measures between 22.05 and 28.10 kilometers in diameter, and its surface has an albedo between 0.089 and 0.145.[7][8][9][10] The Collaborative Asteroid Lightcurve Link derives an albedo of 0.075 and calculates a diameter of 25.53 kilometers with an absolute magnitude of 11.4.[3]
Naming
This minor planet was named for astronomer Matiss A. Dirikis (1923–1993), who was a member of the Astronomical Observatory at the University of Latvia, and chairman of the Latvian branch of the Astronomical–Geodetical Society of the U.S.S.R.. His work on the motion of small Solar System bodies also contributed to the field of theoretical astronomy.[2] The official Шаблон:MoMP was published by the Minor Planet Center on 1 January 1974 (Шаблон:Small).[11]
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
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- Discoveries by Lyudmila Chernykh
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