𝔖 Bobbio Scriptorium
✦   LIBER   ✦

Growth and sedimentation of dust grains in the primordial solar nebula

✍ Scribed by Yoshitsugu Nakagawa; Kiyoshi Nakazawa; Chushiro Hayashi

Publisher
Elsevier Science
Year
1981
Tongue
English
Weight
879 KB
Volume
45
Category
Article
ISSN
0019-1035

No coin nor oath required. For personal study only.

πŸ“œ SIMILAR VOLUMES

Accretional Remanence of Magnetized Dust
Accretional Remanence of Magnetized Dust in the Solar Nebula
✍ Henrik NΓΌbold; Karl-Heinz Glassmeier πŸ“‚ Article πŸ“… 2000 πŸ› Elsevier Science 🌐 English βš– 242 KB

Anticipating the results from the Rosetta magnetometer experiment, we present a theoretical study concerning the possible origin of a cometary magnetic field. Assuming the existence of a permanently magnetized iron dust fraction in the primordial solar nebula, we use a numerical model to investigate

Resonance Trapping in the Primordial Sol
Resonance Trapping in the Primordial Solar Nebula: The Case of a Stokes Drag Dissipation
✍ C. BeaugΓ©; S. Ferraz-Mello πŸ“‚ Article πŸ“… 1993 πŸ› Elsevier Science 🌐 English βš– 788 KB

We consider the problem of the orbital evolution of solid particles in a gas-rich planetary nebula where one planetary embryo already exists (Weidenschilling and Davis model). The case of a Stokes drag is studied both analytically and numerically. We present the equations of the averaged model for t

The Brownian Motion of Dust Particles in
The Brownian Motion of Dust Particles in the Solar Nebula: An Experimental Approach to the Problem of Pre-planetary Dust Aggregation
✍ JΓΌrgen Blum; Gerhard Wurm; Sascha Kempf; Thomas Henning πŸ“‚ Article πŸ“… 1996 πŸ› Elsevier Science 🌐 English βš– 321 KB

are subjected to drag-induced frictional forces. These drag forces are in many cases responsible for the occurrence of Laboratory experiments were performed to study the Brownian motion of m-sized dust grains and small aggregates mutual collisions among the dust particles. If the impact under pre-pl