When we knocked that asteroid moon off course, we may have completely changed its shape

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Credit: NASA/Johns Hopkins APL/Steve Gribben
Credit: NASA/Johns Hopkins APL/Steve Gribben

The asteroid moon Dimorphos may have been reshaped after NASA smashed a spacecraft called the DART (Double Asteroid Redirection Test) planetary defence demonstrator into it back in 2022, according to international scientists. As well as knocking the asteroid moon off course, the spacecraft also gathered information on its internal structure and the effects of the impact. The researchers used computer simulations to recreate the collision as closely as possible, and the closest match they could achieve was by simulating Dimorphos as a weak pile of rubble, which they suggest is material shed from its own asteroid, Didymos. The simulations also indicated that the impact wouldn't have left a crater, but could have reshaped the moon in its entirety, a process known as global deformation.

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From: Springer Nature

Dimorphos may have been reshaped following DART impact

The asteroid moon Dimorphos may have been reshaped following the impact from NASA’s Double Asteroid Redirection Test (DART), according to a paper published in Nature Astronomy. This result indicates that Dimorphos is potentially a weak rubble pile made up of material shed from its asteroid Didymos.

The DART planetary defence demonstrator accomplished its mission on September 26, 2022, when it impacted Dimorphos, the moon of near-Earth asteroid Didymos, and shortened its orbital period around the asteroid by 33 minutes. DART has important planetary defence applications, but the spacecraft also provided information on the internal structure of asteroids and the effect of an impact on their properties.

Sabina Raducan and colleagues modelled the DART impact with a state-of-the-art shock physics code, using realistic constraints on Dimorphos’s mechanical and compositional properties informed by DART’s first results. The simulations that were the closest match to observations of the impact suggest that Dimorphos is weak with a cohesive strength similar to the asteroids Bennu and Ryugu and has a lack of large boulders on its surface. The authors suggest that Dimorphos may be a rubble pile formed from rotational shedding and re-accumulation of ejected material from Didymos. The model also indicates that the DART impact may not have produced an impact crater but could have reshaped the moon in its entirety — a process known as global deformation — and caused resurfacing of Dimorphos with material from its interior.

The authors conclude that their findings offer additional insights into the formation and characteristics of binary asteroids and may have implications for future explorations, such as ESA’s upcoming Hera mission, and asteroid deflection efforts.

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Nature Astronomy
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Organisation/s: University of Bern, Switzerland
Funder: S.D.R. and M.J. acknowledge support from the Swiss National Science Foundation (Project No. 200021_207359). This work was supported by the DART mission (NASA Contract No. 80MSFC20D0004). G.S.C. and T.M.D. acknowledge support from the UK Science and Technology Facilities Council (Grant No. ST/S000615/1). F.F. acknowledges funding from the Swiss National Science Foundation (Ambizione Grant No. 193346). Portions of this work by K.M.K., M.B.S. and J.M.O. were performed at Lawrence Livermore National Laboratory (US Department of Environment Contract No. DE-AC52-07NA27344 and Grant No. LLNL-JRNL-846795). P.M. acknowledges financial support from the French National Centre for Scientific Research through the exploratory research programme of the Mission for Transversal and Interdisciplinary Initiatives, from the European Space Agency and from the University of Tokyo. P.M., R.L., K.W., N.M. and C.Q.R. acknowledge support from the European Union’s Horizon 2020 research and innovation programme (Grant Agreement No. 870377 and Project NEO-MAPP). N.M., C.Q.R. and P.M. acknowledge funding support from the French National Centre for Space Studies. R.N. acknowledges support from Future Investigators in NASA Earth and Space Science and Technology (NNH20ZDA001N/80NSSC21K1527). E.D., E.M.E., P.H.H., S.I., A.L., M.P., A.R. and F.T. acknowledge financial support from the Italian Space Agency (Contract No. 2019-31-HH.0). M.P., A.L. and F.T. also acknowledge support from the Italian Space Agency (Contract No. 2022-8-HH.0). Work by E.G.F. was carried out at the Jet Propulsion Laboratory, California Institute of Technology, under a contract with NASA (Grant No. 80NM0018D0004). J.O. acknowledges support from the Spanish Ministry for Science and Innovation and the Spanish Research Agency (Grant No. PID2021- 125883NB-C22, Project 10.13039/501100011033) and from the European Regional Development Fund under the project A way of making Europe. J.O., I.H., S.R., M.J., R.L. and K.W. acknowledge support from the Spanish National Research Council (Project ILINK22061). The work by P.P. was supported by the Grant Agency of the Czech Republic (Grant No. 20-04431S).
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