Near-infrared Spectral Homogeneity of the Didymos System Before and After the DART Impact

Abstract We spectroscopically characterized the Didymos system, target of the Double Asteroid Redirection Test (DART)/Light Italian Cubesat for Imaging of Asteroids (LICIACube) space mission, close in time to the DART impact event, during six nights between 2022 August and November at Telescopio Naz...

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Published inThe planetary science journal Vol. 5; no. 10; p. 225
Main Authors Ieva, Simone, Mazzotta Epifani, E., Dotto, E., Petropoulou, V., Deshapriya, J. D. P., Hasselmann, P. H., Poggiali, G., Perna, D., Dall’Ora, M., Lucchetti, A., Pajola, M., Ivanovski, S. L., Rossi, A., Brucato, J. R., Palumbo, P., Della Corte, V., Zinzi, A., Thomas, C. A., de León, J., Kareta, T., Moskovitz, N., Chabot, N. L., Rivkin, A. S., Amoroso, M., Bertini, I., Capannolo, A., Caporali, S., Ceresoli, M., Cremonese, G., Gai, I., Gomez-Casajus, L., Gramigna, E., Impresario, G., Lasagni Manghi, R., Lavagna, M., Lombardo, M., Modenini, D., Pirrotta, S., Tortora, P., Tusberti, F., Zannoni, M., Zanotti, G.
Format Journal Article
LanguageEnglish
Published IOP Publishing 01.10.2024
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Summary:Abstract We spectroscopically characterized the Didymos system, target of the Double Asteroid Redirection Test (DART)/Light Italian Cubesat for Imaging of Asteroids (LICIACube) space mission, close in time to the DART impact event, during six nights between 2022 August and November at Telescopio Nazionale Galileo. Here, we show that near-infrared (NIR) spectra (0.75–2.25 μ m) look mostly similar within the same night and between different nights. They are in good agreement with the only spectrum previously available in the literature, observed almost 20 years before those reported in this paper. During one of the observing nights we also obtain spectroscopy information on the ejecta tail induced by the DART impact. The spectrum of the ejecta tail is also very similar to Didymos/Dimorphos itself. All of these aspects seem to suggest that the Didymos system in the NIR looks mostly homogeneous, with very subtle spectral variations.
ISSN:2632-3338
2632-3338
DOI:10.3847/PSJ/ad793e