Morphology of ejecta features from the impact on asteroid Dimorphos

F Fabio Ferrari P Paolo Panicucci G Gianmario Merisio C Carmine Giordano M Mattia Pugliatti J Jian-Yang Li E Eugene G. Fahnestock S Sabina D. Raducan M Martin Jutzi S Stefania Soldini M Masatoshi Hirabayashi (Daniel Guggenheim School of Aerospace Engineering, Georgia Institute of Technology, Atlanta, GA, USA.) C Colby C. Merrill P Patrick Michel F Fernando Moreno G Gonzalo Tancredi J Jessica M. Sunshine (Department of Astronomy, Department of Geological, Environmental and Planetary Sciences, University of Maryland, College Park, MD, USA.) J Jens Ormö I Isabel Herreros H Harrison Agrusa (Université Côte d’Azur, Observatoire de la Côte d’Azur, French National Center for Scientific Research, Laboratoire Lagrange, Nice, France.) Özgür Karatekin Y Yun Zhang N Nancy L. Chabot A Andrew F. Cheng D Derek C. Richardson A Andrew S. Rivkin A Adriano Campo Bagatin T Tony L. Farnham S Stavro Ivanovski A Alice Lucchetti M Maurizio Pajola A Alessandro Rossi D Daniel J. Scheeres F Filippo Tusberti

Abstract

Abstract Hypervelocity impacts play a significant role in the evolution of asteroids, causing material to be ejected and partially reaccreted. However, the dynamics and evolution of ejected material in a binary asteroid system have never been observed directly. Observations of Double Asteroid Redirection Test (DART) impact on asteroid Dimorphos have revealed features on a scale of thousands of kilometers, including curved ejecta streams and a tail bifurcation originating from the Didymos system. Here we show that these features result naturally from the dynamical interaction of the ejecta with the binary system and solar radiation pressure. These mechanisms may be used to constrain the orbit of a secondary body, or to investigate the binary nature of an asteroid. Also, they may reveal breakup or fission events in active asteroids, and help determine the asteroid’s properties following an impact event. In the case of DART, our findings suggest that Dimorphos is a very weak, rubble-pile asteroid, with an ejecta mass estimated to be in the range of (1.1-5.5)×107 kg.

Article Details

Volume / Issue Vol. 16, Issue 1
Published February 14, 2025
ISSN 2041-1723
Publisher Nature Portfolio

Journal Info

Nature Communications

Nature Portfolio

ISSN: 2041-1723 Open Access Life Sciences

Authors (33)

F

Fabio Ferrari

P

Paolo Panicucci

G

Gianmario Merisio

C

Carmine Giordano

M

Mattia Pugliatti

J

Jian-Yang Li

E

Eugene G. Fahnestock

S

Sabina D. Raducan

M

Martin Jutzi

S

Stefania Soldini

M

Masatoshi Hirabayashi

Daniel Guggenheim School of Aerospace Engineering, Georgia Institute of Technology, Atlanta, GA, USA.

C

Colby C. Merrill

P

Patrick Michel

F

Fernando Moreno

G

Gonzalo Tancredi

J

Jessica M. Sunshine

Department of Astronomy, Department of Geological, Environmental and Planetary Sciences, University of Maryland, College Park, MD, USA.

J

Jens Ormö

I

Isabel Herreros

H

Harrison Agrusa

Université Côte d’Azur, Observatoire de la Côte d’Azur, French National Center for Scientific Research, Laboratoire Lagrange, Nice, France.

Özgür Karatekin

Y

Yun Zhang

N

Nancy L. Chabot

A

Andrew F. Cheng

D

Derek C. Richardson

A

Andrew S. Rivkin

A

Adriano Campo Bagatin

T

Tony L. Farnham

S

Stavro Ivanovski

A

Alice Lucchetti

M

Maurizio Pajola

A

Alessandro Rossi

D

Daniel J. Scheeres

F

Filippo Tusberti