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High-speed Boulders and the Debris Field in DART Ejecta

  • Authors: Tony L. Farnham, Jessica M. Sunshine, Masatoshi Hirabayashi, Carolyn M. Ernst, R. Terik Daly, Harrison F. Agrusa, Olivier S. Barnouin, Jian-Yang Li, Kathryn M. Kumamoto, Megan Bruck Syal, Sean E. Wiggins, Evan Bjonnes, Angela M. Stickle, Sabina D. Raducan, Andrew F. Cheng, David A. Glenar, Ramin Lolachi, Timothy J. Stubbs, Eugene G. Fahnstock, Marilena Amoroso, Ivano Bertini, John R. Brucato, Andrea Capannolo, Gabriele Cremonese, Massimo Dall'Ora, Vincenzo Della Corte, J. D. P. Deshapriya, Elisabetta Dotto, Igor Gai, Pedro H. Hasselmann, Simone Ieva, Gabriele Impresario, Stavro L. Ivanovski, Michèle Lavagna, Alice Lucchetti, Francesco Marzari, Elena Mazzotta Epifani, Dario Modenini, Maurizio Pajola, Pasquale Palumbo, Simone Pirrotta, Giovanni Poggiali, Alessandro Rossi, Paolo Tortora, Marco Zannoni, Giovanni Zanotti, Angelo Zinzi

Tony L. Farnham et al 2025 The Planetary Science Journal 6 .

  • Provider: AAS Journals

Caption: Figure 7.

(a) Image showing the walls of the ejecta cone, seen from nearly perpendicular to its axis, and (b) the same image with annotations highlighting the curvature of the walls. (c) Diagram illustrating how the curvature of Dimorphos’s surface causes the angle between the cone’s axis and the outflowing ejecta (θ) to increase with time as the crater grows, while the angle with respect to the local surface (α) remains constant. Panel (b) also highlights the dark ring at the base of the ejecta cone, which is caused by optically thick dust that blocks sunlight from penetrating through to the back of the cone.

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