TY - JOUR
T1 - Macroscale Roughness Reveals the Complex History of Asteroids Didymos and Dimorphos
AU - Vincent, Jean Baptiste
AU - Asphaug, Erik
AU - Barnouin, Olivier
AU - Beccarelli, Joel
AU - Benavidez, Paula G.
AU - Campo-Bagatin, Adriano
AU - Chabot, Nancy L.
AU - Ernst, Carolyn M.
AU - Hasselmann, Pedro H.
AU - Hirabayashi, Masatoshi
AU - Ieva, Simone
AU - Karatekin, Özgür
AU - Kašpárek, Tomáš
AU - Kohout, Tomáš
AU - Lin, Zhong Yi
AU - Lucchetti, Alice
AU - Michel, Patrick
AU - Murdoch, Naomi
AU - Pajola, Maurizio
AU - Parro, Laura M.
AU - Raducan, Sabina D.
AU - Sunshine, Jessica
AU - Tancredi, Gonzalo
AU - Trigo-Rodriguez, Josep M.
AU - Zinzi, Angelo
N1 - Publisher Copyright:
© 2024. The Author(s). Published by the American Astronomical Society.
PY - 2024/10/1
Y1 - 2024/10/1
N2 - Morphological mapping is a fundamental step in studying the processes that shaped an asteroid surface. However, it is challenging and often requires multiple independent assessments by trained experts. Here we present fast methods to detect and characterize meaningful terrains from the topographic roughness: entropy of information, and local mean surface orientation. We apply our techniques to Didymos and Dimorphos, the target asteroids of NASA's Double Asteroid Redirection Test mission—the first attempt to deflect an asteroid. Our methods reliably identify morphological units at multiple scales. The comparative study reveals various terrain types, signatures of processes that transformed Didymos and Dimorphos. Didymos shows the most heterogeneity and morphology that indicate recent resurfacing events. Dimorphos is comparatively rougher than Didymos, which may result from the formation process of the binary pair and past interaction between the two bodies. Our methods can be readily applied to other bodies and data sets.
AB - Morphological mapping is a fundamental step in studying the processes that shaped an asteroid surface. However, it is challenging and often requires multiple independent assessments by trained experts. Here we present fast methods to detect and characterize meaningful terrains from the topographic roughness: entropy of information, and local mean surface orientation. We apply our techniques to Didymos and Dimorphos, the target asteroids of NASA's Double Asteroid Redirection Test mission—the first attempt to deflect an asteroid. Our methods reliably identify morphological units at multiple scales. The comparative study reveals various terrain types, signatures of processes that transformed Didymos and Dimorphos. Didymos shows the most heterogeneity and morphology that indicate recent resurfacing events. Dimorphos is comparatively rougher than Didymos, which may result from the formation process of the binary pair and past interaction between the two bodies. Our methods can be readily applied to other bodies and data sets.
UR - https://www.scopus.com/pages/publications/85214694730
UR - https://www.scopus.com/inward/citedby.url?scp=85214694730&partnerID=8YFLogxK
U2 - 10.3847/PSJ/ad7a01
DO - 10.3847/PSJ/ad7a01
M3 - Article
AN - SCOPUS:85214694730
SN - 2632-3338
VL - 5
JO - Planetary Science Journal
JF - Planetary Science Journal
IS - 10
M1 - 236
ER -