2123 Vltava

Classification and orbit

The S-type asteroid is a member of the Koronis family, which is named after 158 Koronis and consists of about 300 known bodies with nearly co-planar ecliptical orbits. The asteroid orbits the Sun in the outer main-belt at a distance of 2.6–3.1 AU once every 4 years and 10 months (1,767 days). Its orbit has an eccentricity of 0.08 and an inclination of 1° with respect to the ecliptic. A first precovery taken at Heidelberg in 1934, extends the body's observation arc by 39 years prior to its official discovery observation at Nauchnyj.

Physical characteristics

Rotation period

Between 1998 and 2005, a survey of members of the Koronis family by seven different observatories obtained a large number of rotational lightcurves from . For Vltava, the survey gave an ambiguous rotation period of 34.0 hours with a brightness variation of 0.21 in magnitude (). In 2014, photometric observations at the Palomar Transient Factory in California rendered a lightcurve with an alternative solution of hours, or about half the period previously found, with an amplitude of 0.19 magnitude ().

Diameter and albedo

According to the surveys carried out by the international Infrared Astronomical Satellite (IRAS), the Japanese Akari satellite, and the NEOWISE mission of NASA's Wide-field Infrared Survey Explorer, the asteroid measures between 14.4 and 15.1 kilometers in diameter and its surface has an albedo between 0.20 and 0.22.

Naming

This minor planet was named for the Vltava (Moldau), the longest river within the Czech Republic, running through the city of Prague. The approved naming citation was published by the Minor Planet Center on 1 April 1980 (M.P.C. 5283).

References

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