학술논문
VADER: Probing the Dark Side of Dimorphos with LICIACube LUKE
Document Type
article
Author
Angelo Zinzi; P. H. A. Hasselmann; V. Della Corte; J. D. P. Deshapriya; I. Gai; A. Lucchetti; M. Pajola; A. Rossi; E. Dotto; E. Mazzotta Epifani; R. T. Daly; M. Hirabayashi; T. Farnham; C. M. Ernst; S. L. Ivanovski; J.-Y. Li; L. M. Parro; M. Amoroso; J. Beccarelli; I. Bertini; J. R. Brucato; A. Capannolo; S. Caporali; M. Ceresoli; G. Cremonese; M. Dall’Ora; L. Gomez Casajus; E. Gramigna; S. Ieva; G. Impresario; R. Lasagni Manghi; M. Lavagna; M. Lombardo; D. Modenini; B. Negri; P. Palumbo; D. Perna; S. Pirrotta; G. Poggiali; P. Tortora; F. Tusberti; M. Zannoni; G. Zanotti
Source
The Planetary Science Journal, Vol 5, Iss 4, p 103 (2024)
Subject
Language
English
ISSN
2632-3338
Abstract
The ASI cubesat LICIACube has been part of the first planetary defense mission DART, having among its scopes to complement the DRACO images to better constrain the Dimorphos shape. LICIACube had two different cameras, LEIA and LUKE, and to accomplish its goal, it exploited the unique possibility of acquiring images of the Dimorphos hemisphere not seen by DART from a vantage point of view, in both time and space. This work is indeed aimed at constraining the tridimensional shape of Dimorphos, starting from both LUKE images of the nonimpacted hemisphere of Dimorphos and the results obtained by DART looking at the impacted hemisphere. To this aim, we developed a semiautomatic Computer Vision algorithm, named VADER, able to identify objects of interest on the basis of physical characteristics, subsequently used as input to retrieve the shape of the ellipse projected in the LUKE images analyzed. Thanks to this shape, we then extracted information about the Dimorphos ellipsoid by applying a series of quantitative geometric considerations. Although the solution space coming from this analysis includes the triaxial ellipsoid found by using DART images, we cannot discard the possibility that Dimorphos has a more elongated shape, more similar to what is expected from previous theories and observations. The result of our work seems therefore to emphasize the unique value of the LICIACube mission and its images, making even clearer the need of having different points of view to accurately define the shape of an asteroid.