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arxiv: 2310.12089 · v1 · pith:KJE4SYUZnew · submitted 2023-10-18 · 🌌 astro-ph.EP

Ejecta Evolution Following a Planned Impact into an Asteroid: The First Five Weeks

Theodore Kareta (1) , Cristina Thomas (2) , Jian-Yang Li (3) , Matthew M. Knight (4) , Nicholas Moskovitz (1) , Agata Rozek (5) , Michele T. Bannister (6) , Simone Ieva (7)
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Colin Snodgrass (5) Petr Pravec (8) Eileen V. Ryan (9) William H. Ryan (9) Eugene G. Fahnestock (10) Andrew S. Rivkin (11) Nancy Chabot (11) Alan Fitzsimmons (12) David Osip (13) Tim Lister (14) Gal Sarid (15) Masatoshi Hirabayashi (16) Tony Farnham (17) Gonzalo Tancredi (18) Patrick Michel (19 20) Richard Wainscoat (21) Rob Weryk (22) Bonnie Burrati (10) Jana Pittichova (10) Ryan Ridden-Harper (6) Nicole J. Tan (6) Paul Tristram (23) Tyler Brown (6) Mariangela Bonavita (5) Martin Burgdorf (24) Elahe Khalouei (25) Penelope Longa (26) Markus Rabus (27) Sedighe Sajadian (28) Uffe Graae Jorgensen (29) Martin Dominik (30) Jean-Baptiste Kikwaya (31) Elena Mazzotta Epifani (7) Elisabetta Dotto (7) J.D. Prasanna Deshapriya (7) Pedro H. Hasselmann (7) Massimo Dall'Ora (32) Lyu Abe (19) Tristan Guillot (19) Djamel Mekarnia (19) Abdelkrim Agabi (19) Philippe Bendjoya (19) Olga Suarez (19) Amaury Triaud (33) Thomas Gasparetto (34) Maximillian N. Gunther (35) Michael Kueppers (35) Bruno Merin (35) Joseph Chatelain (14) Edward Gomez (14) Helen Usher (36) Cai Stoddard-Jones (37) Matthew Bartnik (38) Michael Bellaver (38) Brenna Chetan (38) Emma Dugan (38) Tori Fallon (38) Jeremy Fedewa (38) Caitlyn Gerhard (38) Seth A. Jacobson (38) Shane Painter (38) David-Michael Peterson (38) Joseph E. Rodriguez (38) Cody Smith (38) Kirill V. Sokolovsky (38) Hannah Sullivan (38) Kate Townley (38) Sarah Watson (38) Levi Webb (38) Josep M. Trigo-Rodr{\i}guez (39) Josep M. Llenas (40) Ignacio Perez-Garc{\i}a (41) A.J. Castro-Tirado (41) Jean-Baptiste Vincent (42) Alessandra Migliorini (43) Monica Lazzarin (44) Fiorangela La Forgia (44) Fabio Ferrari (45) Tom Polakis (1) Brian Skiff (1) ((1) Lowell Observatory. (2) Northern Arizona University. (3) Planetary Science Institute. (4) U.S. Naval Academy (5) Institute for Astronomy University of Edinburgh (6) University of Canterbury (7) INAF - Osservatorio Astronomico di Roma (8) Astronomical Institute Academy of Sciences of the Czech Republic (9) New Mexico Institute of Mining Technology / Magdalena Ridge Observatory (10) Jet Propulsion Laboratory (11) Johns Hopkins University Applied Physics Laboratory (12) Queen's University Belfast (13) Las Campanas Observatory (14) Las Cumbres Observatory (15) SETI Institute (16) Georgia Institute of Technology (17) University of Maryland (18) Depto. Astronomia Udelar (19) Universite Cote d'Azur Observatoire de la Cote d'Azur CNRS Laboratoire Lagrange (20) University of Tokyo (21) University of Hawai'i (22) Department of Physics Astronomy University of Western Ontario (23) MOA (24) Universitat Hamburg (25) Seoul National University (26) Universidad de Antofogasta (27) Universidad Catolica de la Santisima Concepcion (28) Isfahan University of Technology (29) University of Copenhagen (30) University of Saint Andrews (31) Vatican Observatory (32) INAF - Osservatorio Astronomico di Capodimonte (33) University of Birmingham (34) INAF - Trieste (35) European Space Agency (36) Open University (37) Cardiff University (38) Michigan State University (39) Institute of Space Sciences (CSIC-IEEC) (40) Pujalt Observatory (41) Instituto de Astrofisica de Andalucia IAA-CSIC (42) DLR Institute of Planetary Research (43) INAF - Institute for Space Astrophysics Planetology (44) Dipartmento di Fisica e Astronomia Padova University (45) Politecnico di Milano)
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keywords impactejectadaysfirstmagnitudesasteroidbrightnessdimming
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The impact of the DART spacecraft into Dimorphos, moon of the asteroid Didymos, changed Dimorphos' orbit substantially, largely from the ejection of material. We present results from twelve Earth-based facilities involved in a world-wide campaign to monitor the brightness and morphology of the ejecta in the first 35 days after impact. After an initial brightening of ~1.4 magnitudes, we find consistent dimming rates of 0.11-0.12 magnitudes/day in the first week, and 0.08-0.09 magnitudes/day over the entire study period. The system returned to its pre-impact brightness 24.3-25.3 days after impact through the primary ejecta tail remained. The dimming paused briefly eight days after impact, near in time to the appearance of the second tail. This was likely due to a secondary release of material after re-impact of a boulder released in the initial impact, through movement of the primary ejecta through the aperture likely played a role.

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