Broadband Linear Polarization of Jupiter Trojans
arXiv:1511.09271 · doi:10.1051/0004-6361/201526889
Abstract
Trojan asteroids orbit in the Lagrange points of the system Sun-planet-asteroid. Their dynamical stability make their physical properties important proxies for the early evolution of our solar system. To study their origin, we want to characterize the surfaces of Jupiter Trojan asteroids and check possible similarities with objects of the main belt and of the Kuiper Belt. We have obtained high-accuracy broad-band linear polarization measurements of six Jupiter Trojans of the L4 population and tried to estimate the main features of their polarimetric behaviour. We have compared the polarimetric properties of our targets among themselves, and with those of other atmosphere-less bodies of our solar system. Our sample show approximately homogeneous polarimetric behaviour, although some distinct features are found between them. In general, the polarimetric properties of Trojan asteroids are similar to those of D- and P-type main-belt asteroids. No sign of coma activity is detected in any of the observed objects. An extended polarimetric survey may help to further investigate the origin and the surface evolution of Jupiter Trojans.
Accepted for publication on A&A
References in corpus (8)
- Visible spectroscopic and photometric survey of Jupiter Trojans: final results on dynamical families
- The Properties of Jovian Trojan Asteroids Listed in SDSS Moving Object Catalog 3
- Taxonomy of asteroid families among the Jupiter Trojans: Comparison between spectroscopic data and the Sloan Digital Sky Survey colors
- Exploring the surface properties of Transneptunian Objects and Centaurs with polarimetric FORS1/VLT observations
- Polarimetric survey of asteroids with the Asiago telescope
- Simultaneous Linear and Circular Optical Polarimetry of Asteroid (4) Vesta
- Discovery of two distinct polarimetric behaviours of trans-Neptunian objects
- The Complex History of Trojan Asteroids
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