We conducted micro-gravity experiments to study the outcome of collisions between sub-mm-sized dust agglomerates consisting of µm-sized SiO2 monomer grains at velocities of several cm s −1. Prior to the experiments, we used X-ray computer tomography (nano-CT) imaging to study the internal structure of these dust agglomerates and found no rim compaction so that their collision behavior is not governed by preparation-caused artefacts. We found that collisions between these dust aggregates can lead either to sticking or to bouncing, depending mostly on the impact velocity. While previ-ous collision models derived the transition between both regimes from contact physics, we used the available empirical data from these and earlier experiments to...
To study the evolution of protoplanetary dust aggregates, we performed experiments with up to 2600 c...
Context. Collisions between dust particles may lead to agglomerate growth or fragmentation, dependin...
The coagulation of dust aggregates occurs in various astrophysical environments. Each one is charact...
Over the past years the processes involved in the growth of planetesimals have extensively been stud...
We performed laboratory experiments colliding 0.8-1.0 mm and 1.0-1.6 mm SiO2 dust aggregates with lo...
Context. The experiment results presented apply to the very first stages of planet formation, when s...
Collisions between centimeter- to decimeter-sized dusty bodies are important to understand the mecha...
Context. The experiment results presented apply to the very first stages of planet formation, when s...
Context. The experiment results presented apply to the very first stages of planet formation, when s...
Context. In the very first steps of the formation of a new planetary system, dust agglomer...
Context. Bouncing collisions of dust aggregates within the protoplanetary disk may have a significan...
Context. In the very first steps of the formation of a new planetary system, dust agglomer...
Context. Bouncing collisions of dust aggregates within the protoplanetary disk may have a significan...
In the last years, a number of new experiments have advanced our knowledge on the early growth phase...
Collisions of mm-size dust aggregates play a crucial role in the early phases of planet formation. I...
To study the evolution of protoplanetary dust aggregates, we performed experiments with up to 2600 c...
Context. Collisions between dust particles may lead to agglomerate growth or fragmentation, dependin...
The coagulation of dust aggregates occurs in various astrophysical environments. Each one is charact...
Over the past years the processes involved in the growth of planetesimals have extensively been stud...
We performed laboratory experiments colliding 0.8-1.0 mm and 1.0-1.6 mm SiO2 dust aggregates with lo...
Context. The experiment results presented apply to the very first stages of planet formation, when s...
Collisions between centimeter- to decimeter-sized dusty bodies are important to understand the mecha...
Context. The experiment results presented apply to the very first stages of planet formation, when s...
Context. The experiment results presented apply to the very first stages of planet formation, when s...
Context. In the very first steps of the formation of a new planetary system, dust agglomer...
Context. Bouncing collisions of dust aggregates within the protoplanetary disk may have a significan...
Context. In the very first steps of the formation of a new planetary system, dust agglomer...
Context. Bouncing collisions of dust aggregates within the protoplanetary disk may have a significan...
In the last years, a number of new experiments have advanced our knowledge on the early growth phase...
Collisions of mm-size dust aggregates play a crucial role in the early phases of planet formation. I...
To study the evolution of protoplanetary dust aggregates, we performed experiments with up to 2600 c...
Context. Collisions between dust particles may lead to agglomerate growth or fragmentation, dependin...
The coagulation of dust aggregates occurs in various astrophysical environments. Each one is charact...