Predictions for the Dynamical States of the Didymos System before and after the Planned DART Impact

Abstract

NASA's Double Asteroid Redirection Test (DART) spacecraft is planned to impact the natural satellite of (65803) Didymos, Dimorphos, around 23:14 UTC on 26 September 2022, causing a reduction in its orbital period that will be measurable with ground-based observations. This test of kinetic impactor technology will provide the first estimate of the momentum transfer enhancement factor $\beta$ at a realistic scale, wherein ejecta from the impact provides an additional deflection to the target. Earth-based observations, the LICIACube spacecraft (to be detached from DART prior to impact), and ESA's follow-up Hera mission to launch in 2024, will provide additional characterization of the deflection test. Together Hera and DART comprise the Asteroid Impact and Deflection Assessment (AIDA) cooperation between NASA and ESA. Here the predicted dynamical states of the binary system upon arrival and after impact are presented. The assumed dynamically relaxed state of the system will be excited by the impact, leading to an increase in eccentricity and slight tilt of the orbit together with enhanced libration of Dimorphos with amplitude dependent on the currently poorly known target shape. Free rotation around the moon's long axis may also be triggered and the orbital period will experience variations from seconds to minutes over timescales of days to months. Shape change of either body due to cratering or mass wasting triggered by crater formation and ejecta may affect $\beta$ but can be constrained through additional measurements. Both BYORP and gravity tides may cause measurable orbital changes on the timescale of Hera's rendezvous.

arXiv comment23 pages, 13 figures, published in PSJ

References in corpus (26)

• Scaling forces to asteroid surfaces: The role of cohesion
• Tidal Evolution of Rubble Piles
• Fragment properties at the catastrophic disruption threshold: The effect of the parent body's internal structure
• SPH calculations of asteroid disruptions: The role of pressure dependent failure models
• Creep stability of the proposed AIDA mission target 65803 Didymos: I. Discrete cohesionless granular physics model
• Identification of meteorite source regions in the Solar System
• Internal Structure of Asteroids Having Surface Shedding due to Rotational Instability
• Long-term Stable Equilibria for Synchronous Binary Asteroids
• On the Secular Behavior of Irregular Satellites
• The Excited Spin State of Dimorphos Resulting from the DART Impact
• Ejecta Cloud from a Kinetic Impact on the Secondary of a Binary Asteroid: I. Mechanical Environment and Dynamic Model
• Near-Earth Binaries and Triples: Origin and Evolution of Spin-Orbital Properties
• DART Mission Determination of Momentum Transfer: Model of Ejecta Plume Observations
• Ejecta cloud from the AIDA space project kinetic impact on the secondary of a binary asteroid: II. fates and evolutionary dependencies
• Doubly Synchronous Binary Asteroid Mass Parameter Observability
• A six-part collisional model of the main asteroid belt
• An experimental study of low-velocity impacts into granular material in reduced gravity
• The role of fragment shapes in the simulations of asteroids as gravitational aggregates
• Micro-meteoroid seismic uplift and regolith concentration on kilometric scale asteroids
• A parallel-GPU code for asteroid aggregation problems with angular particles
• Constraints on the perturbed mutual motion in Didymos due to impact-induced deformation of its primary after the DART impact
• Dynamical Evolution of the Didymos-Dimorphos Binary Asteroid as Rubble Piles following the DART Impact
• Non-principal axis rotation in binary asteroid systems and how it weakens the BYORP effect
• New multi-part collisional model of the main belt: The contribution to near-Earth asteroids
• Small-body deflection techniques using spacecraft: techniques in simulating the fate of ejecta
• The VIMOS Public Extragalactic Redshift Survey (VIPERS) -- Environment-size relation of massive passive galaxies at 0.5 < z < 0.8

Cited by in corpus (14)

• Momentum Transfer from the DART Mission Kinetic Impact on Asteroid Dimorphos
• Physical properties of asteroid Dimorphos as derived from the DART impact
• Light Curves and Colors of the Ejecta from Dimorphos after the DART Impact
• Direct $N$-body simulations of satellite formation around small asteroids: insights from DART's encounter with the Didymos system
• The Dynamical State of the Didymos System Before and After the DART Impact
• Energy Dissipation in Synchronous Binary Asteroids
• Dynamical Evolution of the Didymos-Dimorphos Binary Asteroid as Rubble Piles following the DART Impact
• Lessons learned from NASA's DART impact about disrupting rubble-pile asteroids
• The Hera Radio Science Experiment at Didymos
• Rotation-induced granular motion on the secondary component of binary asteroids: Application to the DART impact on Dimorphos
• High-Speed Boulders and the Debris Field in DART Ejecta
• The accuracy of mutual potential approximations in simulations of binary asteroids
• Analytical theory of the spin-orbit state of a binary asteroid deflected by a kinetic impactor
• A change of the rotation period of asteroid (65803) Didymos caused by the DART impact