VADER:与 LICIACube LUKE 一起探索 Dimorphos 的黑暗面

A. Zinzi, P. Hasselmann, V. Della Corte, J. Deshapriya, I. Gai, A. Lucchetti, A. Pajola, A. Rossi, E. Dotto, E. Mazzotta Epifani, R. T. Daly, M. Hirabayashi, T. Farnham, C. M. Ernst, S. Ivanovski, J.-Y. Li, L. Parro, M. Amoroso, J. Beccarelli, I. Bertini, J. Brucato, Andrea 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
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引用次数: 0

摘要

意大利航天局的立方体卫星 LICIACube 是首次行星防御飞行任务 DART 的一部分,其瞄准镜之一是补充 DRACO 图像,以便更好地确定 Dimorphos 的形状。LICIACube 有两台不同的照相机,LEIA 和 LUKE,为了实现其目标,它利用了一种独特的可能性,即从时间和空间的有利角度获取 DART 没有看到的 Dimorphos 半球图像。实际上,这项工作的目的是根据 LUKE 拍摄的未受撞击的 Dimorphos 半球图像和 DART 拍摄的受撞击半球图像,确定 Dimorphos 的三维形状。为此,我们开发了一种名为 "VADER "的半自动计算机视觉算法,该算法能够根据物理特征识别出感兴趣的物体,然后将其作为输入,检索所分析的 LUKE 图像中投射的椭圆的形状。有了这个形状,我们就可以通过一系列定量的几何考量来提取有关 Dimorphos 椭圆体的信息。虽然分析得出的解空间包括利用 DART 图像找到的三轴椭球体,但我们不能排除迪莫非斯具有更细长形状的可能性,这与之前的理论和观测结果更加相似。因此,我们的工作结果似乎强调了 LICIACube 飞行任务及其图像的独特价值,使我们更加清楚地认识到需要从不同的角度来准确界定小行星的形状。
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VADER: Probing the Dark Side of Dimorphos with LICIACube LUKE
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.
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