4979 Otawara
4979 Otawara is a small, rapidly rotating asteroid orbiting in the main asteroid belt. Discovered in 1949, the asteroid was named after Japanese photo artist and writer Akira Otawara. It is stony in composition, consisting of olivine and pyroxenes, and is estimated to be around in size. The asteroid was one of three originally planned targets for the Rosetta mission, but launch delays meant that it was abandoned.
Discovery and naming
Otawara was discovered on 2 August 1949 by German astronomer Karl Wilhelm Reinmuth at Heidelberg-Königstuhl State Observatory in Heidelberg, Baden-Württemberg, Germany. It was given the provisional designation 1949 PQ, and on 21 November 1991 it was numbered 4979 by the Minor Planet Center. The asteroid was named after Akira Otawara, a photo artist and writer. Together with astronomer Shuichi Nakano, he published two catalogs in 1983, Field Star Map 2000 and Star & Planet Catalogue 2000. Nakano proposed the name Otawara for the object; the name was published in Minor Planet Circular 22505 on 1 September 1993.Orbit
Otawara orbits with a semi-major axis of 2.17 astronomical units ; it is located in the main asteroid belt. It has a moderate orbital eccentricity of 0.15. Along its 3.19 year orbit, its distance from the Sun varies from 1.85 AU at perihelion to 2.48 AU at aphelion. Its orbit is closely aligned with the plane of the planets, with an orbital inclination of 0.91° with respect to the ecliptic plane.Physical characteristics
Otawara is a small asteroid; estimates of its size range around. Otawara's lightcurve, or variations in its observed apparent brightness, suggests that it is elongated, with an a/b axis ratio of. Initial analysis of Otawara's spectrum in 1999, conducted by a team of astronomers led by Alain Doressoundiram, was ambiguous on what asteroid taxonomic class it belonged to. Its spectrum was consistent with either an S-type asteroid rich in silicate minerals, a V-type asteroid associated with 4 Vesta, or an SV-type asteroid, with characteristics intermediate of the two. However, later analysis by a team led by Sonia Fornasier ruled out a V-type classification, and concluded that Otawara is an S-class asteroid rich in olivine and pyroxenes. Under the Gaffey classification scheme, Otawara belongs to the S subclass. S asteroids are probable candidates for parent bodies of ordinary chondrite meteorites; Otawara's spectral similarity to these meteorites suggests it is not differentiated. Otawara's density is constrained to be ≥1.9 g/cm3, although this is not valid if it is a solid object instead of a rubble pile.Analysis of Otawara's lightcurve suggests it rotates rapidly, with a rotation period of hours, classifying it as a fast rotating asteroid. Its rotation appears to be retrograde—rotating clockwise—with its north pole pointed towards the ecliptic south.