Английская Википедия:2672 Písek

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Шаблон:Use dmy dates Шаблон:Infobox planet

2672 Písek, provisional designation Шаблон:Mp, is a Eunomia asteroid from the central regions of the asteroid belt, approximately Шаблон:Convert in diameter. It was discovered on 31 May 1979, by Yugoslav astronomer Jaroslav Květoň at the Kleť Observatory in the Czech Republic.[1] The likely elongated asteroid is a suspected tumbler and a slow rotator with an exceptionally long period of 831 hours.[2] It was named after the Czech town of Písek.[3]

Orbit and classification

Písek is a core member of the Eunomia family (Шаблон:Small),[4] a prominent family of stony S-type asteroid and the largest one in the intermediate main belt with more than 5,000 members.[5] It orbits the Sun in the central main-belt at a distance of 2.2–3.0 AU once every 4 years and 3 months (1,543 days; semi-major axis of 2.61 AU). Its orbit has an eccentricity of 0.15 and an inclination of 14° with respect to the ecliptic.[6]

The asteroid was first observed as Шаблон:Mp at Johannesburg Observatory in July 1937. The body's observation arc begins with its observation as Шаблон:Mp at Goethe Link Observatory in March 1953, more than 26 years prior to its official discovery observation at Klet.[1]

Naming

This minor planet was named after the Czech town of Písek, located in the western South Bohemian Region known for its many prolific Czech writers and artists.[3] The official naming citation was published by the Minor Planet Center on 28 January 1983 (Шаблон:Small).[7]

Physical characteristics

Písek is an assumed S-type asteroid,[2] which agrees with the overall spectral type for members of the Eunomia family.[5]Шаблон:Rp Conversely, the space-based surveys found an albedo that is typical for a carbonaceous C-type or potentially darker D- and P-type asteroid (see below).

Rotation period

Between May and July 2017, a rotational lightcurve of Písek was obtained from photometric observations by Vladimir Benishek at Belgrade Astronomical Observatory in Serbia. Lightcurve analysis gave a rotation period of Шаблон:Val hours with a high brightness amplitude of 0.90 magnitude, indicative of a non-spherical shape (Шаблон:Small).[8][2]

Diameter and albedo

According to the survey carried out by the Infrared Astronomical Satellite IRAS, the Japanese Akari satellite, and the NEOWISE mission of NASA's Wide-field Infrared Survey Explorer, Písek measures between 20.18 and 29.60 kilometers in diameter and its surface has an albedo between 0.0294 and 0.091.[9][10][11][12]

The Collaborative Asteroid Lightcurve Link assumes a standard albedo of 0.21 – derived from 15 Eunomia, the parent body of the Eunomia family– and consequently calculates a much smaller diameter of 9.60 kilometers based on an absolute magnitude of 12.4.[2]

References

Шаблон:Reflist

External links

Шаблон:Minor planets navigator Шаблон:Small Solar System bodies Шаблон:Authority control

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