Physical properties of asteroid Dimorphos as derived from the DART impact
Abstract
On 26 September 2022, NASA’s Double Asteroid Redirection Test (DART) mission successfully impacted Dimorphos, the natural satellite of the binary near-Earth asteroid (65803) Didymos. Numerical simulations of the impact provide a means to find the surface material properties and structures of the target that are consistent with the observed momentum deflection efficiency, ejecta cone geometry and ejected mass. Our simulation that best matches the observations indicates that Dimorphos is weak, with a cohesive strength of less than a few pascals, like asteroids (162173) Ryugu and (101955) Bennu. We find that the bulk density of Dimorphos ρB is lower than ~2,400 kg m–3 and that it has a low volume fraction of boulders (≲40 vol%) on the surface and in the shallow subsurface, which are consistent with data measured by the DART experiment. These findings suggest that Dimorphos is a rubble pile that might have formed through rotational mass shedding and reaccumulation from Didymos. Our simulations indicate that the DART impact caused global deformation and resurfacing of Dimorphos. ESA’s upcoming Hera mission may find a reshaped asteroid rather than a well-defined crater.
- Authors:
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- Univ. of Bern (Switzerland)
- Johns Hopkins Univ., Laurel, MD (United States)
- Univ. of Maryland, College Park, MD (United States)
- Imperial College, London (United Kingdom)
- Politecnico di Milano (Italy)
- Georgia Institute of Technology, Atlanta, GA (United States); Auburn Univ., AL (United States)
- Lawrence Livermore National Laboratory (LLNL), Livermore, CA (United States)
- Universite Cote d'Azur, Nice (France); Univ. of Tokyo (Japan)
- Univ. of Toulouse (France)
- National Institute for Astrophysics (INAF) (Italy). Astronomical Observatory of Padova (OAPD)
- National Research Council (CNR) (Italy). Institute of Applied Physics "Nello Carrara" (IFAC)
- Univ. of Maryland, College Park, MD (United States); Universite Cote d'Azur, Nice (France)
- NASA Goddard Space Flight Center (GSFC), Greenbelt, MD (United States)
- Istituto Nazionale di Astrofisica (INAF), Roma (Italy)
- California Institute of Technology (CalTech), Pasadena, CA (United States)
- Spanish National Research Council and National Institute of Aerospace Technology (CSIC-INTA) (Spain). Centro de Astrobiología (CAB)
- Istituto Nazionale di Fisica Nucleare (INFN), Trieste (Italy). Osservatorio Astronomico di Trieste
- Planetary Science Institute, Tucson, AZ (United States)
- Leibniz Institute for Evolution and Biodiversity Science, Berlin (Germany)
- Czech Academy of Sciences (CAS) (Czech Republic). Astronomical Institute
- Univ. of Colorado, Boulder, CO (United States)
- Agenzia Spaziale Italiana (ASI), Rome (Italy). Space Science Data Center
- London Stereoscopic Company (United Kingdom)
- Publication Date:
- Research Org.:
- Lawrence Livermore National Laboratory (LLNL), Livermore, CA (United States)
- Sponsoring Org.:
- USDOE National Nuclear Security Administration (NNSA)
- OSTI Identifier:
- 2318792
- Report Number(s):
- LLNL-JRNL-846795
Journal ID: ISSN 2397-3366; 1071231
- Grant/Contract Number:
- AC52-07NA27344
- Resource Type:
- Accepted Manuscript
- Journal Name:
- Nature Astronomy
- Additional Journal Information:
- Journal Name: Nature Astronomy; Journal ID: ISSN 2397-3366
- Publisher:
- Springer Nature
- Country of Publication:
- United States
- Language:
- English
- Subject:
- 79 ASTRONOMY AND ASTROPHYSICS; asteroids; comets; Kuiper belt
Citation Formats
Raducan, S. D., Jutzi, M., Cheng, A. F., Zhang, Y., Barnouin, O., Collins, G. S., Daly, R. T., Davison, T. M., Ernst, C. M., Farnham, T. L., Ferrari, F., Hirabayashi, M., Kumamoto, K. M., Michel, P., Murdoch, N., Nakano, R., Pajola, M., Rossi, A., Agrusa, H. F., Barbee, B. W., Syal, M. Bruck, Chabot, N. L., Dotto, E., Fahnestock, E. G., Hasselmann, P. H., Herreros, I., Ivanovski, S., Li, J. -Y., Lucchetti, A., Luther, R., Ormö, J., Owen, M., Pravec, P., Rivkin, A. S., Robin, C. Q., Sánchez, P., Tusberti, F., Wünnemann, K., Zinzi, A., Epifani, E. Mazzotta, Manzoni, C., and May, B. H. Physical properties of asteroid Dimorphos as derived from the DART impact. United States: N. p., 2024.
Web. doi:10.1038/s41550-024-02200-3.
Raducan, S. D., Jutzi, M., Cheng, A. F., Zhang, Y., Barnouin, O., Collins, G. S., Daly, R. T., Davison, T. M., Ernst, C. M., Farnham, T. L., Ferrari, F., Hirabayashi, M., Kumamoto, K. M., Michel, P., Murdoch, N., Nakano, R., Pajola, M., Rossi, A., Agrusa, H. F., Barbee, B. W., Syal, M. Bruck, Chabot, N. L., Dotto, E., Fahnestock, E. G., Hasselmann, P. H., Herreros, I., Ivanovski, S., Li, J. -Y., Lucchetti, A., Luther, R., Ormö, J., Owen, M., Pravec, P., Rivkin, A. S., Robin, C. Q., Sánchez, P., Tusberti, F., Wünnemann, K., Zinzi, A., Epifani, E. Mazzotta, Manzoni, C., & May, B. H. Physical properties of asteroid Dimorphos as derived from the DART impact. United States. https://doi.org/10.1038/s41550-024-02200-3
Raducan, S. D., Jutzi, M., Cheng, A. F., Zhang, Y., Barnouin, O., Collins, G. S., Daly, R. T., Davison, T. M., Ernst, C. M., Farnham, T. L., Ferrari, F., Hirabayashi, M., Kumamoto, K. M., Michel, P., Murdoch, N., Nakano, R., Pajola, M., Rossi, A., Agrusa, H. F., Barbee, B. W., Syal, M. Bruck, Chabot, N. L., Dotto, E., Fahnestock, E. G., Hasselmann, P. H., Herreros, I., Ivanovski, S., Li, J. -Y., Lucchetti, A., Luther, R., Ormö, J., Owen, M., Pravec, P., Rivkin, A. S., Robin, C. Q., Sánchez, P., Tusberti, F., Wünnemann, K., Zinzi, A., Epifani, E. Mazzotta, Manzoni, C., and May, B. H. Mon .
"Physical properties of asteroid Dimorphos as derived from the DART impact". United States. https://doi.org/10.1038/s41550-024-02200-3. https://www.osti.gov/servlets/purl/2318792.
@article{osti_2318792,
title = {Physical properties of asteroid Dimorphos as derived from the DART impact},
author = {Raducan, S. D. and Jutzi, M. and Cheng, A. F. and Zhang, Y. and Barnouin, O. and Collins, G. S. and Daly, R. T. and Davison, T. M. and Ernst, C. M. and Farnham, T. L. and Ferrari, F. and Hirabayashi, M. and Kumamoto, K. M. and Michel, P. and Murdoch, N. and Nakano, R. and Pajola, M. and Rossi, A. and Agrusa, H. F. and Barbee, B. W. and Syal, M. Bruck and Chabot, N. L. and Dotto, E. and Fahnestock, E. G. and Hasselmann, P. H. and Herreros, I. and Ivanovski, S. and Li, J. -Y. and Lucchetti, A. and Luther, R. and Ormö, J. and Owen, M. and Pravec, P. and Rivkin, A. S. and Robin, C. Q. and Sánchez, P. and Tusberti, F. and Wünnemann, K. and Zinzi, A. and Epifani, E. Mazzotta and Manzoni, C. and May, B. H.},
abstractNote = {On 26 September 2022, NASA’s Double Asteroid Redirection Test (DART) mission successfully impacted Dimorphos, the natural satellite of the binary near-Earth asteroid (65803) Didymos. Numerical simulations of the impact provide a means to find the surface material properties and structures of the target that are consistent with the observed momentum deflection efficiency, ejecta cone geometry and ejected mass. Our simulation that best matches the observations indicates that Dimorphos is weak, with a cohesive strength of less than a few pascals, like asteroids (162173) Ryugu and (101955) Bennu. We find that the bulk density of Dimorphos ρB is lower than ~2,400 kg m–3 and that it has a low volume fraction of boulders (≲40 vol%) on the surface and in the shallow subsurface, which are consistent with data measured by the DART experiment. These findings suggest that Dimorphos is a rubble pile that might have formed through rotational mass shedding and reaccumulation from Didymos. Our simulations indicate that the DART impact caused global deformation and resurfacing of Dimorphos. ESA’s upcoming Hera mission may find a reshaped asteroid rather than a well-defined crater.},
doi = {10.1038/s41550-024-02200-3},
journal = {Nature Astronomy},
number = ,
volume = ,
place = {United States},
year = {Mon Feb 26 00:00:00 EST 2024},
month = {Mon Feb 26 00:00:00 EST 2024}
}
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