Orbital period change of Dimorphos due to the DART kinetic impact
Author:
Thomas Cristina A.ORCID, Naidu Shantanu P.ORCID, Scheirich PeterORCID, Moskovitz Nicholas A., Pravec Petr, Chesley Steven R.ORCID, Rivkin Andrew S.ORCID, Osip David J., Lister Tim A.ORCID, Benner Lance A. M., Brozović Marina, Contreras Carlos, Morrell NidiaORCID, Rożek AgataORCID, Kušnirák Peter, Hornoch KamilORCID, Mages Declan, Taylor Patrick A., Seymour Andrew D., Snodgrass Colin, Jørgensen Uffe G.ORCID, Dominik MartinORCID, Skiff Brian, Polakis Tom, Knight Matthew M.ORCID, Farnham Tony L.ORCID, Giorgini Jon D., Rush Brian, Bellerose Julie, Salas Pedro, Armentrout William P., Watts Galen, Busch Michael W., Chatelain Joseph, Gomez Edward, Greenstreet Sarah, Phillips LizORCID, Bonavita Mariangela, Burgdorf Martin J.ORCID, Khalouei Elahe, Longa-Peña Penélope, Rabus Markus, Sajadian Sedighe, Chabot Nancy L.ORCID, Cheng Andrew F.ORCID, Ryan William H., Ryan Eileen V., Holt Carrie E., Agrusa Harrison F.
Abstract
AbstractThe Double Asteroid Redirection Test (DART) spacecraft successfully performed the first test of a kinetic impactor for asteroid deflection by impacting Dimorphos, the secondary of near-Earth binary asteroid (65803) Didymos, and changing the orbital period of Dimorphos. A change in orbital period of approximately 7 min was expected if the incident momentum from the DART spacecraft was directly transferred to the asteroid target in a perfectly inelastic collision1, but studies of the probable impact conditions and asteroid properties indicated that a considerable momentum enhancement (β) was possible2,3. In the years before impact, we used lightcurve observations to accurately determine the pre-impact orbit parameters of Dimorphos with respect to Didymos4–6. Here we report the change in the orbital period of Dimorphos as a result of the DART kinetic impact to be −33.0 ± 1.0 (3σ) min. Using new Earth-based lightcurve and radar observations, two independent approaches determined identical values for the change in the orbital period. This large orbit period change suggests that ejecta contributed a substantial amount of momentum to the asteroid beyond what the DART spacecraft carried.
Publisher
Springer Science and Business Media LLC
Subject
Multidisciplinary
Reference43 articles.
1. Cheng, A. F. et al. AIDA DART asteroid deflection test: planetary defense and science objectives. Planet. Space Sci. 157, 104–115 (2018). 2. Stickle, A. M. et al. Effects of impact and target parameters on the results of a kinetic impactor: predictions for the Double Asteroid Redirection Test (DART) mission. Planet. Sci. J. 3, 248 (2022). 3. Raducan, S. D. & Jutzi, M. Global-scale reshaping and resurfacing of asteroids by small-scale impacts, with applications to the DART and Hera missions. Planet. Sci. J. 3, 128 (2022). 4. Pravec, P. et al. Photometric observations of the binary near-Earth asteroid (65803) Didymos in 2015–2021 prior to DART impact. Planet. Sci. J. 3, 175 (2022). 5. Naidu, S. P. et al. Anticipating the DART impact: orbit estimation of Dimorphos using a simplified model. Planet. Sci. J. 3, 234 (2022).
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