Orbital Period Change of Dimorphos Due to the DART Kinetic Impact
arXiv:2303.02077 · doi:10.1038/s41586-023-05805-2
Abstract
The 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 minutes was expected if the incident momentum from the DART spacecraft was directly transferred to the asteroid target in a perfectly inelastic collision, but studies of the probable impact conditions and asteroid properties indicated that a considerable momentum enhancement () was possible. In the years prior to impact, we used lightcurve observations to accurately determine the pre-impact orbit parameters of Dimorphos with respect to Didymos. 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 (3) minutes. 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 significant amount of momentum to the asteroid beyond what the DART spacecraft carried.
arXiv commentAccepted by Nature
References in corpus (13)
- Gaia Data Release 2. Summary of the contents and survey properties
- The VizieR database of Astronomical Catalogues
- Las Cumbres Observatory Global Telescope Network
- Astrometry.net: Blind astrometric calibration of arbitrary astronomical images
- Real-time processing of the imaging data from the network of Las Cumbres Observatory Telescopes using BANZAI
- Gaia Data Release 3: The Galaxy in your preferred colours. Synthetic photometry from Gaia low-resolution spectra
- PHOTOMETRYPIPELINE: An Automated Pipeline for Calibrated Photometry
- Rotation of Cometary Nuclei: New Lightcurves and an Update of the Ensemble Properties of Jupiter-Family Comets
- The binary near-Earth asteroid (175706) 1996 FG3 - An observational constraint on its orbital evolution
- Near-Earth Binaries and Triples: Origin and Evolution of Spin-Orbital Properties
- NEOExchange -- An online portal for NEO and Solar System science
- Anticipating the DART impact: Orbit estimation of Dimorphos using a simplified model
- A satellite orbit drift in binary near-Earth asteroids (66391) 1999 KW4 and (88710) 2001 SL9 -- Indication of the BYORP effect
Cited by in corpus (21)
- Successful Kinetic Impact into an Asteroid for Planetary Defense
- Momentum Transfer from the DART Mission Kinetic Impact on Asteroid Dimorphos
- Ejecta from the DART-produced active asteroid Dimorphos
- Physical properties of asteroid Dimorphos as derived from the DART impact
- The Dynamical State of the Didymos System Before and After the DART Impact
- Dimorphos orbit determination from mutual events photometry
- Lessons learned from NASA's DART impact about disrupting rubble-pile asteroids
- The Hera Radio Science Experiment at Didymos
- Photometry and Polarimetry of 2010 XC: Observational Confirmation of E-type Near-Earth Asteroid Pair
- High-Speed Boulders and the Debris Field in DART Ejecta
- Delivery of DART Impact Ejecta to Mars and Earth: Opportunity for Meteor Observations
- HyperScout-H: the hyperspectral imager for the ESA Hera mission
- 2021 occultations and transits of Linus orbiting (22) Kalliope: I. Polygonal and `cliptracing' algorithm
- Thermal and Optical Characterization of Near-Earth Objects: Science Commissioning of the Recently Upgraded Mid-Infrared Camera MIRSI on the NASA Infrared Telescope Facility
- ASTERIA -- Thermal Inertia Evaluation of asteroid Didymos
- A 3D thermophysical model for binary asteroid systems: Application to the BYORP effect on (175706) 1996 FG3
- A change of the rotation period of asteroid (65803) Didymos caused by the DART impact
- Placing the Near-Earth Object Impact Probability in Context
- Analytical theory of the spin-orbit state of a binary asteroid deflected by a kinetic impactor
- The Material Point Method (MPM) for simulating hypervelocity impact on asteroids
- Near-Earth asteroids in Main Belt-crossing orbits