189 citations · 470 across the 9 of their papers we have counts for
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Growth of Aggregates with Liquid-Like Ice-Shells in Protoplanetary Discs
Grzegorz Musiolik
During the first stages of planet formation, the collision growth of dust aggregates in protoplanetary discs (PPDs) is interrupted at the bouncing barrier. Dust aggregates coated b…
Wind erosion on Mars and other small terrestrial planets
Maximilian Kruss, Grzegorz Musiolik, Tunahan Demirci +2
We carried out wind tunnel experiments on parabolic flights with 100 m Mojave Mars simulant sand. The experiments result in shear stress thresholds and erosion rates for varying…
Contacts of Water Ice in Protoplanetary Disks - Laboratory Experiments
Grzegorz Musiolik, Gerhard Wurm
Water ice is abundant in protoplanetary disks. Its sticking properties are therefore important during phases of collisional growth. In this work, we study the sticking and rolling…
Saltation under Martian Gravity and its Influence on the Global Dust Distribution
Grzegorz Musiolik, Maximilian Kruss, Tunahan Demirci +6
Dust and sand motion are a common sight on Mars. Understanding the interaction of atmosphere and Martian soil is fundamental to describe the planet's weather, climate and surface m…
Analog Experiments on Tensile Strength of Dusty and Cometary Matter
Grzegorz Musiolik, Caroline de Beule, Gerhard Wurm
The tensile strength of small dusty bodies in the solar system is determined by the interaction between the composing grains. In the transition regime between small and sticky dust…
Ice Grain Collisions in Comparison: CO, HO and their Mixtures
Grzegorz Musiolik, Jens Teiser, Tim Jankowski +1
Collisions of ice particles play an important role in the formation of planetesimals and comets. In recent work we showed, that CO ice behaves like silicates in collisions. The…
Collisions of CO Ice Grains in Planet Formation
Grzegorz Musiolik, Jens Teiser, Tim Jankowski +1
In protoplanetary disks, CO is solid ice beyond its snow line at . Due to its high abundance, it contributes heavily to the collisional evolution in this region…