𝔖 Bobbio Scriptorium
✦   LIBER   ✦

Distribution of Planetesimals around a Protoplanet in the Nebula Gas

✍ Scribed by Hidekazu Tanaka; Shigeru Ida

Publisher
Elsevier Science
Year
1997
Tongue
English
Weight
652 KB
Volume
125
Category
Article
ISSN
0019-1035

No coin nor oath required. For personal study only.

πŸ“œ SIMILAR VOLUMES

Formation of Protoplanets from Planetesi
Formation of Protoplanets from Planetesimals in the Solar Nebula
✍ Eiichiro Kokubo; Shigeru Ida πŸ“‚ Article πŸ“… 2000 πŸ› Elsevier Science 🌐 English βš– 311 KB

Planetary accretion from planetesimals to protoplanets is investigated using three-dimensional N-body simulations. The effect of gas drag due to solar nebula is included and realistic-sized planetesimals with a standard material density are used, with which the growth time scale of planetesimals is

A New Mechanism Relevant to the Formatio
A New Mechanism Relevant to the Formation of Planetesimals in the Solar Nebula
✍ Gerhard Wurm; JΓΌrgen Blum; Joshua E. Colwell πŸ“‚ Article πŸ“… 2001 πŸ› Elsevier Science 🌐 English βš– 137 KB

Current models of the formation of km-sized planetary building blocks, or planetesimals, by collisional accretion require unrealistically low collision velocities or ad hoc assumptions about sticking in order for growth to occur. Collision velocities in the protoplanetary nebula increase with increa

Distribution of counterions in the doubl
Distribution of counterions in the double layer around a cylindrical polyion
✍ D. Bratko; V. Vlachy πŸ“‚ Article πŸ“… 1982 πŸ› Elsevier Science 🌐 English βš– 238 KB

The modltied Posron-Beltzmann (LIPB) cqu~~t~on, and the Monte Carlo (MC) msthod, were apphed to the cell model oi a pol)clcctrolytc solutwn III order to ulculxe the dutrlbutlon oi counterlons mound a cylmdwxl polylon. Both mcthoils juggcjt stronger bmdmg oi munterlons to the polygon than predlctcd b