20 results on '"Jutzi, Martin"'
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2. Combined impact and interior evolution models in three dimensions indicate a southern impact origin of the Martian Dichotomy
3. Investigating the feasibility of an impact-induced Martian Dichotomy
4. Dispersion and shattering strength of rocky and frozen planetesimals studied by laboratory experiments and numerical simulations
5. Modification of icy planetesimals by early thermal evolution and collisions: Constraints for formation time and initial size of comets and small KBOs
6. Collisional heating and compaction of small bodies: Constraints for their origin and evolution
7. The shape and structure of small asteroids as a result of sub-catastrophic collisions
8. Assessing possible mutual orbit period change by shape deformation of Didymos after a kinetic impact in the NASA-led Double Asteroid Redirection Test
9. Fragment properties from large-scale asteroid collisions: I: Results from SPH/N-body simulations using porous parent bodies and improved material models
10. Relevance of tidal heating on large TNOs
11. SPH calculations of Mars-scale collisions: The role of the equation of state, material rheologies, and numerical effects
12. Small-body deflection techniques using spacecraft: Techniques in simulating the fate of ejecta
13. SPH calculations of asteroid disruptions: The role of pressure dependent failure models
14. Selective sampling during catastrophic disruption: Mapping the location of reaccumulated fragments in the original parent body
15. Hypervelocity impacts on asteroids and momentum transfer I. Numerical simulations using porous targets
16. The Asteroid Veritas: An intruder in a family named after it?
17. Fragment properties at the catastrophic disruption threshold: The effect of the parent body’s internal structure
18. Numerical simulations of impacts involving porous bodies: II. Comparison with laboratory experiments
19. Numerical simulations of impacts involving porous bodies: I. Implementing sub-resolution porosity in a 3D SPH hydrocode
20. Chondrule formation during planetesimal accretion
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