Add to ORKGUp to now, only (4) Vesta has been thought of as a source of differentiated material, which has been discovered all around the Main Belt region. However, the investigations have shown that the objects, with the same spectral properties of Vesta and distributed beyond 2.5 AU, cannot be dynamically related to (4) Vesta. Thus, their origin seems to be linked to the break-up of large objects other than Vesta. Some evidences suggesting that V-types in the middle and outer main belt might have originated from the disruption of partly or totally differentiated parent bodies have been recently found, and dynamical studies allowed the identification of possible asteroidal families including basaltic asteroids. We started an observing campaign of ast...
Context. Most asteroid families are very homogeneous in physical properties. Some show greater diver...
We present near-infrared (0.78–2.45 µm) reflectance spectra for nine middle and outer main belt (a >...
Most of the currently known basaltic (V-type) asteroids are believed to be past or present members o...
Context. Basaltic asteroids (spectrally classified as V-types) are believed to be fragments of large...
We present new spectral observations using ground-based telescopes of 23 putative V-type asteroids, ...
In recent years, several small basaltic V-type asteroids have been identified all around the main be...
6 pages, 1 figure.-- Printed version published Sep 2009.Basaltic asteroids are small bodies connecte...
In the last twenty-five years several small basaltic V-type asteroids have been identified all aroun...
Context. The V-type asteroids are associated with basaltic composition. Apart from ( 1459) Magnya, a...
V-type asteroids are bodies whose surfaces are constituted of basalt. In the Main Asteroid Belt, mos...
Context. V-type asteroids in the inner main belt are thought to be genetically related to (4) Vesta ...
V-type asteroids, characterized by two absorption bands at 1.0 and 2.0 mu m, are usually thought to ...
Context. Most asteroid families are very homogeneous in physical properties. Some show greater diver...
Triangulated observations of fireballs allow us to determine orbits and fall positions for meteorite...
Context. Most asteroid families are very homogeneous in physical properties. Some show greater diver...
Context. Most asteroid families are very homogeneous in physical properties. Some show greater diver...
We present near-infrared (0.78–2.45 µm) reflectance spectra for nine middle and outer main belt (a >...
Most of the currently known basaltic (V-type) asteroids are believed to be past or present members o...
Context. Basaltic asteroids (spectrally classified as V-types) are believed to be fragments of large...
We present new spectral observations using ground-based telescopes of 23 putative V-type asteroids, ...
In recent years, several small basaltic V-type asteroids have been identified all around the main be...
6 pages, 1 figure.-- Printed version published Sep 2009.Basaltic asteroids are small bodies connecte...
In the last twenty-five years several small basaltic V-type asteroids have been identified all aroun...
Context. The V-type asteroids are associated with basaltic composition. Apart from ( 1459) Magnya, a...
V-type asteroids are bodies whose surfaces are constituted of basalt. In the Main Asteroid Belt, mos...
Context. V-type asteroids in the inner main belt are thought to be genetically related to (4) Vesta ...
V-type asteroids, characterized by two absorption bands at 1.0 and 2.0 mu m, are usually thought to ...
Context. Most asteroid families are very homogeneous in physical properties. Some show greater diver...
Triangulated observations of fireballs allow us to determine orbits and fall positions for meteorite...
Context. Most asteroid families are very homogeneous in physical properties. Some show greater diver...
Context. Most asteroid families are very homogeneous in physical properties. Some show greater diver...
We present near-infrared (0.78–2.45 µm) reflectance spectra for nine middle and outer main belt (a >...
Most of the currently known basaltic (V-type) asteroids are believed to be past or present members o...