Английская Википедия:9549 Akplatonov

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9549 Akplatonov, provisional designation Шаблон:Mp, is an Eunomia asteroid from the central region of the asteroid belt, approximately Шаблон:Convert in diameter. It was discovered on 19 September 1985, by Soviet–Russian astronomer couple Nikolai and Lyudmila Chernykh at the Crimean Astrophysical Observatory in Nauchnyj, on the Crimean peninsula. The likely S-type asteroid has a relatively short rotation period of 2.8 hours. It was named for Russian computational mathematician Шаблон:MoMP.

Orbit and classification

Akplatonov is a core member of the Eunomia family, a large group of stony S-type asteroids and the most prominent family in the intermediate main-belt. Alternatively, in Nesvorný's HCM-analysis, the asteroid belong's to the main belt's background population, while in an earlier such analysis, Thais Mothé-Diniz considered Akplatonov to be the largest body in a small cluster or clump of its own. It orbits the Sun in the central asteroid belt at a distance of 2.3–2.9 AU once every 4 years and 3 months (1,537 days; semi-major axis of 2.61 AU). Its orbit has an eccentricity of 0.11 and an inclination of 11° with respect to the ecliptic. The body's observation arc begins 4 years prior to its official discovery observation, with its first identification as Шаблон:Mp at the discovering observatory in October 1981.

Naming

This minor planet was named in honor of Шаблон:MoMP (born 1931), a Russian computational mathematician, roboticist, astrodynamicist, and long-time member at the Keldysh Institute of Applied Mathematics. He pioneered the research in walking robots, the computation of satellite orbits around Earth, and the guidance of the flight path of spacecraft in the Solar System. The official Шаблон:MoMP was published by the Minor Planet Center on 24 June 2002 (Шаблон:Small).

Physical characteristics

Rotation period

A rotational lightcurve of Akplatonov was obtained from photometric observations using the 0.9-meter SARA telescope at Kitt Peak National Observatory in May 2009. It showed a rotation period of Шаблон:Val hours with a brightness variation of 0.15 magnitude (Шаблон:Small). A poorly rated period determination from a fragmentary lightcurve by astronomers at the Palomar Transient Factory in 2010 gave a period of 4.7 hours (Шаблон:Small).

Diameter and albedo

According to the survey carried out by the NEOWISE mission of NASA's space-based Wide-field Infrared Survey Explorer, Akplatonov measures 8.2 kilometers in diameter and its surface has an albedo of 0.285, while the Collaborative Asteroid Lightcurve Link (CALL) assumes an albedo of 0.21 – derived from 15 Eunomia, the family's largest member and namesake – and calculates a diameter of 9.17 kilometers using an absolute magnitude of 12.5.

External links

• Asteroid Lightcurve Database (LCDB), query form (info Шаблон:Webarchive)
• Dictionary of Minor Planet Names, Google books
• Discovery Circumstances: Numbered Minor Planets (5001)-(10000) – Minor Planet Center
• Шаблон:AstDys
• Шаблон:JPL small body