Bibcode
Licandro, J.; Campins, H.; Mothé-Diniz, T.; Pinilla-Alonso, N.; de León, J.
Referencia bibliográfica
Astronomy and Astrophysics, Volume 461, Issue 2, January II 2007, pp.751-757
Fecha de publicación:
1
2007
Revista
Número de citas
98
Número de citas referidas
89
Descripción
Context: The study of asteroids that present sporadic cometary activity
is of fundamental importance to address several astronomical problems
including the end states of comet nuclei, the abundance of water in main
belt asteroids, and its role as a possible source of terrestial water.
Aims: We studied the composition of the surface of asteroid (3200)
Phaethon, a paradigmatic case of asteroid-comet transition object, in
order to determine its cometary or asteroidal nature. Methods: We
report visible and near infrared spectra covering the 0.35-2.4 μm
spectral range, obtained with the 4.2 m William Herschel Telescope, the
2.5 m Nordic Optical Telescope, and the Italian 3.58 m Telescopio
Nazionale Galileo at "El Roque de los Muchachos" Observatory (La Palma,
Spain). Our spectrum is compared with those of meteorite samples and
man-made mineral mixtures to determine possible components, modeled
using multiple scattering formulations, and also compared with the
spectra of comet nuclei and other comet-asteroid transitional objects.
Results: Phaethon's spectrum does not show any sharp structure and
has a negative slope at wavelengths >0.43 μm, consistent with
B-type asteroids. Below 0.43 μm the reflectance decreases. The
spectral shape is similar to that of aqueously altered CI/CM meteorites
and of hydrated minerals. A surface composition with hydrated silicates
is also suggested by the models. A possible spectral variability in the
UV is suggested by the avaliable spectra, and is compatible with a
slightly different abundance of hydrated silicates. Finally, Phaethon's
spectrum shows important differences with the few comet nuclei properly
observed at these wavelengths and is similar to the spectra of other
peculiar comet-asteroid transition objects. Conclusions: .The
spectral properties and dynamical properties of (3200) Phaethon support
an asteroidal nature rather than a cometary one. Phaethon is more likely
an "activated" asteroid, similar to the population of activated
asteroids in the Main Belt Comets, than an extinct comet.