Volume 483, Number 2, May IV 2008
|Page(s)||L17 - L20|
|Published online||08 April 2008|
Letter to the Editor
Physical and dynamical properties of (12929) 1999 TZ1 suggest that it is a Trojan
LESIA-Observatoire de Paris, 5 place J. Janssen, 92195 Meudon, France e-mail: firstname.lastname@example.org
2 CSIC-Instituto de Astrofisíca de Andalusía, Granada, Spain
3 Observatoire de la Côte d'Azur, Nice, France
Accepted: 27 March 2008
Context. Small body (12929) 1999 TZ1 is listed by the Minor Planet Center (MPC) as a Centaur. However, its location close to the Lagrangian point L5 of Jupiter is typical of a Trojan object with large inclination.
Aims. The aim of this work is to provide a global physical and dynamical characterization of this object and to reassess its classification.
Methods. We obtained multi-wavelength observations with IRTF (Hawaii), OSN and IRAM-30 m (Spain), and performed a dynamical simulation of the evolution of its orbital parameters.
Results. Visible photometry monitoring shows a rotation curve with a period (if considered double-peaked) of 10.4 ± 0.1 h and an absolute R magnitude HR = 9.792 ± 0.025. Near-IR spectroscopy indicates a featureless reflectance spectra, with a low spectral slope of 7.2 ± 0.11%/100 nm. Thermal observations at 250 GHz provide a 4.5σ detection with a flux of 1.22 ± 0.27 mJy. The combination of the visible and millimeter datasets, assuming a standard thermal model, leads to a geometric albedo pv = and a mean diameter of 51.5 ± 5 km.
Conclusions. The low albedo and spectral slope measured are typical of Jupiter's Trojans, but cannot exclude a Centaur nature. However, the dynamical lifetime of the object was estimated to be longer than 1 Gy, which is unlikely for a Centaur and suggests that (12929) 1999 TZ1 is a Trojan asteroid.
Key words: minor planets, asteroids / radio continuum: solar system / infrared: solar system / celestial mechanics
© ESO, 2008
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