Distribution and spectrophotometric classification of basaltic asteroids

Abstract

We aim to determine the distribution of basaltic asteroids (classified as V-types) based on the spectrophotometric data reported in the MOVIS-C catalogue. A total of 782 asteroids were identified. The observations with all four filters (Y, J, H, Ks), available for 297 of these candidates, allow a reliable comparison with the laboratory data of howardite, eucrite, and diogenite meteorites. We found that the majority of the basaltic candidates ($\approx$ 95$\%$) are located in the inner main belt, while only 29 ($\approx$ 4$\%$) and 8 ($\approx$ 1$\%$) are located in the middle and outer main belt, respectively. A fraction of $\approx$ 33$\%$ from the V-type candidates is associated with the Vesta family (with respect to AstDyS). We also identified four middle main belt V-type candidates belonging to (15) Eunomia family, and another four low inclination ones corresponding to (135) Hertha. We report differences between the color indices and albedo distributions of the V-type candidates located in the inner main belt compared to those from the middle and outer main belt. These results support the hypothesis of a different origin for the basaltic asteroids with a semi-major axis beyond 2.5 A.U. Furthermore, lithological differences are present between the vestoids and the inner low inclination basaltic asteroids. The data allow us to estimate the unbiased distribution of basaltic asteroids across the main asteroid belt. We highlight that at least 80$\%$ of the ejected basaltic material from (4) Vesta is missing or is not yet detected because it is fragmented in sizes smaller than 1 km.

References in corpus (9)

• Initial Performance of the NEOWISE Reactivation Mission
• Compositional distributions and evolutionary processes for the near-Earth object population: Results from the MIT-Hawaii Near-Earth Object Spectroscopic Survey (MITHNEOS
• The Visible and Infrared Survey Telescope for Astronomy (VISTA): Design, Technical Overview and Performance
• The VISTA Science Archive
• The Distribution of Basaltic Asteroids in the Main Belt
• The infrared colors of the Sun
• Near-Earth asteroids spectroscopic survey at Isaac Newton Telescope
• More chips off of Asteroid (4) Vesta: characterization of eight Vestoids and their HED meteorite analogs
• Scattering V-type asteroids during the giant planets instability: A step for Jupiter, a leap for basalt

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