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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 3.

The first four LUKE images, scaled to the same spacecraft range, showing the approach morphology and the large, rapidly expanding structures in the early ejecta. The top panels show the images with a log display, while the bottom panels have been enhanced by dividing out an azimuthally averaged radial profile to reveal the details in the dust cloud. The highlighted features, #1 and #2, have projected speeds of 340 and 240 m s⁻¹, respectively.

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