activity
20112018
most citedThe Physics of Protoplanetesimal Dust Agglomerates. Vi. Erosion of Large Aggregates as a Source of Micrometer-Sized Particles

64 citations · 234 across the 5 of their papers we have counts for

collaborators

5 papers

astro-ph.EP2018★ 27 cited

The physics of protoplanetesimal dust agglomerates. X. High-velocity collisions between small and large dust agglomerates as growth barrier

Rainer Schräpler, Jürgen Blum, Sebastiaan Krijt +1

In a protoplanetary disk, dust aggregates in the m to mm size range possess mean collision velocities of 10 to 60 ms with respect to dm- to m-size bodies. We performed la…

astro-ph.EP2015★ 41 cited

The stratification of regolith on celestial objects

Rainer Schräpler, Jürgen Blum, Ingo von Borstel +1

All atmosphere-less planetary bodies are covered with a dust layer, the so-called regolith, which determines the optical, mechanical and thermal properties of their surface. These…

cond-mat.soft2013★ 45 cited

Granular convection and the Brazil nut effect in reduced gravity

Carsten Güttler, Ingo von Borstel, Rainer Schräpler +1

We present laboratory experiments of a vertically vibrated granular medium consisting of 1 mm diameter glass beads with embedded 8 mm diameter intruder glass beads. The experiments…

astro-ph.EP2012★ 57 cited

The physics of protoplanetesimal dust agglomerates. VII The low-velocity collision behavior of large dust agglomerates

Rainer Schräpler, Jürgen Blum, Alexander Seizinger +1

We performed micro-gravity collision experiments in our laboratory drop-tower using 5-cm-sized dust agglomerates with volume filling factors of 0.3 and 0.4, respectively. This work…

astro-ph.EP2011★ 64 cited

The Physics of Protoplanetesimal Dust Agglomerates. Vi. Erosion of Large Aggregates as a Source of Micrometer-Sized Particles

Rainer Schräpler, Jürgen Blum

Observed protoplanetary disks consist of a large amount of micrometer-sized particles. Dullemond and Dominik (2005) pointed out for the first time the difficulty in explaining the…