4055 Magellan

Orbit and classification

Magellan orbits the Sun in the inner main-belt at a distance of 1.2 - once every 2 years and 6 months (897 days). Its orbit has an eccentricity of 0.33 and an inclination of 23° with respect to the ecliptic.

The first observation was made at the Australian Siding Spring Observatory, extending the asteroid's observation arc by just one month prior to its official discovery observation at Palomar.

It has a minimum orbital intersection distance with Earth of 0.2398 AU, which corresponds to 93.4 lunar distances.

Physical characteristics

Being a V-type asteroid in the Tholen and SMASS taxonomy, Magellan is thought to have originated from the Rheasilvia crater, a large impact crater on the south-polar surface of 4 Vesta, which is the main-belt's second-most-massive asteroid after 1 Ceres.

Diameter and albedo

According to observations by the Keck Observatory and to the survey carried out by NASA's Wide-field Infrared Survey Explorer with its subsequent NEOWISE mission, Magellan measures between 2.2 and in diameter and its surface has a high albedo of 0.31 to 0.33. The Collaborative Asteroid Lightcurve Link (LCDB) agrees with the Keck observations, adopting an albedo of 0.31 and a diameter of 2.49 km.

Lightcurves

Between 2000 and 2015, six rotational lightcurves of Magellan were obtained from photometric observations by astronomers Petr Pravec and Brian D. Warner, as well as by the Mexican Asteroid Photometry Campaign and the Palomar Transient Factory. The highest rated lightcurve by LCDB's standards was obtained by French amateur astronomer David Romeuf in July 2015, which gave a rotation period of hours with a brightness variation of 0.45 magnitude (). The large variation suggests an elongated shape.

Naming

This minor planet was named after Portuguese navigator and explorer Ferdinand Magellan (Fernão de Magalhães; c. 1480–1521), who led and died on the first circumnavigation of the Earth during 1519–1522. The minor planet is also named after the modern Magellan spacecraft, which was launched by NASA in 1989 and went on to map the surface of Venus. The Portuguese navigator is also honored by the craters Magelhaens on Mars and Magelhaens on the Moon. The official naming citation was published by the Minor Planet Center on 2 December 1990 (M.P.C. 17466).

Notes

References

• Asteroid Lightcurve Database (LCDB), query form (info )
• Dictionary of Minor Planet Names, Google books
• Asteroids and comets rotation curves, CdR – Observatoire de Genève, Raoul Behrend

References

1. {{MW. Magellan