Add to ORKGIn this paper we search for photometric data of asteroids in the Hilda region in the Moving Object Catalogue of the Sloan Digital Sky Survey to find the spectral characteristics of small members of this group. We found that the correlation between size and spectral slope previously suggested for Hilda asteroids is correct only for large objects (H<12) but it is not supported by data obtained for the small ones. The best possibility to explain this behavior is that a space weathering process affecting the surface properties of these primitive objects is operating, modulated by a collisional resurfacing process affected by the lack of small projectiles in the population. Despite the intrinsic limitations of the few band photometry of the Sloa...
International audienceThe nature and origin of the asteroids orbiting in near-Earth space, including...
Thesis: S.B., Massachusetts Institute of Technology, Department of Earth, Atmospheric, and Planetary...
The Cybele and Hilda dynamical groups delimit the outer edge of the asteroid belt. Their composition...
In this paper we search for photometric data of asteroids in the Hilda region in the Moving Object C...
In this paper we search for photometric data of asteroids in the Hilda region in the Moving Object C...
In this paper we search for photometric data of asteroids in the outer region of the Hecuba gap in t...
Aims. We present a comparative analysis of the spectral slope and color distributions of Jupiter Tro...
Aims. We present a comparative analysis of the spectral slope and color distributions of Jupiter Tro...
Aims. We present a comparative analysis of the spectral slope and color distributions of Jupiter Tro...
We have used the 3.5 m New Technology Telescope at ESO, La Silla, to obtain spectra of 18 asteroids ...
Aims. We present the results of a taxonomic classification defined using multiband photometry of Hun...
We have combined the NEOWISE and Sloan Digital Sky Survey data to study the albedos of 24,353 astero...
Thesis: S.B., Massachusetts Institute of Technology, Department of Physics, 2003.Cataloged from PDF ...
Thesis (Ph.D.)--Massachusetts Institute of Technology, Dept. of Earth, Atmospheric, and Planetary Sc...
International audienceThe nature and origin of the asteroids orbiting in near-Earth space, including...
International audienceThe nature and origin of the asteroids orbiting in near-Earth space, including...
Thesis: S.B., Massachusetts Institute of Technology, Department of Earth, Atmospheric, and Planetary...
The Cybele and Hilda dynamical groups delimit the outer edge of the asteroid belt. Their composition...
In this paper we search for photometric data of asteroids in the Hilda region in the Moving Object C...
In this paper we search for photometric data of asteroids in the Hilda region in the Moving Object C...
In this paper we search for photometric data of asteroids in the outer region of the Hecuba gap in t...
Aims. We present a comparative analysis of the spectral slope and color distributions of Jupiter Tro...
Aims. We present a comparative analysis of the spectral slope and color distributions of Jupiter Tro...
Aims. We present a comparative analysis of the spectral slope and color distributions of Jupiter Tro...
We have used the 3.5 m New Technology Telescope at ESO, La Silla, to obtain spectra of 18 asteroids ...
Aims. We present the results of a taxonomic classification defined using multiband photometry of Hun...
We have combined the NEOWISE and Sloan Digital Sky Survey data to study the albedos of 24,353 astero...
Thesis: S.B., Massachusetts Institute of Technology, Department of Physics, 2003.Cataloged from PDF ...
Thesis (Ph.D.)--Massachusetts Institute of Technology, Dept. of Earth, Atmospheric, and Planetary Sc...
International audienceThe nature and origin of the asteroids orbiting in near-Earth space, including...
International audienceThe nature and origin of the asteroids orbiting in near-Earth space, including...
Thesis: S.B., Massachusetts Institute of Technology, Department of Earth, Atmospheric, and Planetary...
The Cybele and Hilda dynamical groups delimit the outer edge of the asteroid belt. Their composition...