Showing 1–20 of 68 results
/ Date/ Name
Feb 13, 2015Collisional Formation and Modeling of Asteroid FamiliesSep 23, 2022After DART: Using the first full-scale test of a kinetic impactor to inform a future planetary defense missionJun 11, 2013Numerical simulations of granular dynamics. I. Hard-sphere discrete element method and testsAug 1, 2014Numerical predictions of surface effects during the 2029 close approach of asteroid 99942 ApophisOct 28, 2021High-Resolution Observations of Bright Boulders on Asteroid Ryugu: 1. Size Frequency Distribution and MorphologyAug 6, 2017Constraints on the perturbed mutual motion in Didymos due to impact-induced deformation of its primary after the DART impactDec 2, 2016ASIME 2016 White Paper: In-Space Utilisation of Asteroids: "Answers to Questions from the Asteroid Miners"May 26, 2024The Yarkovsky effect on the long-term evolution of binary asteroidsJan 16, 2024The cumulation of debris clouds around a fast-rotating asteroidJul 14, 2022Predictions for the Dynamical States of the Didymos System before and after the Planned DART ImpactFeb 25, 2026Tidal disruptions of rubble piles: The case of PhobosJun 23, 2009Collisional and Rotational Disruption of AsteroidsMar 6, 2023Momentum Transfer from the DART Mission Kinetic Impact on Asteroid DimorphosNov 8, 2022Planetary Exploration Horizon 2061 Report, Chapter 3: From science questions to Solar System explorationJul 31, 2023The Perturbed Full Two-Body Problem: Application to Post-DART DidymosAug 10, 2018Fragment properties from large-scale asteroid collisions: I: Results from SPH/N-body simulations using porous parent bodies and improved material modelsJul 16, 2021The Excited Spin State of Dimorphos Resulting from the DART ImpactOct 28, 2021High-Resolution Observations of Bright Boulders on Asteroid Ryugu: 2. Spectral PropertiesAug 2, 2017Ejecta cloud from the AIDA space project kinetic impact on the secondary of a binary asteroid: II. fates and evolutionary dependenciesAug 2, 2017Structural analysis of rubble-pile asteroids applied to collisional evolution