Formation of a star and planets around it through a gravitational instability in a disk of gas and dust

Keyphrases

• Dust 100%
• Jeans Instability 100%
• Gravitational Instability 100%
• Gasses 100%
• Turbulence 66%
• Non-axisymmetric 66%
• Jeans 66%
• Protostellar Disks 66%
• Order of Magnitude 33%
• Kinetic Energy 33%
• Cooling Method 33%
• Unstable Modes 33%
• Small Amplitude 33%
• Angular Momentum 33%
• Spontaneous Generation 33%
• Potential Energy 33%
• N-body 33%
• Solar System 33%
• Self-sustaining 33%
• Mass Flow 33%
• Amplitude Perturbation 33%
• Nonlinear Regime 33%
• Angular Momentum Transfer 33%
• Density Wave 33%
• WKB Approximation 33%
• Nonlinear Development 33%
• Hydrodynamic Turbulence 33%
• Characteristic Scale 33%
• Satellite Systems 33%
• Protoplanetary Disks 33%
• Spiral Pattern 33%
• Turbulent Heating 33%
• Thin Disk 33%
• Stochastic Motion 33%
• Generating Mechanism 33%
• Mass Redistribution 33%
• Cooling Mechanism 33%
• Giant Planets 33%
• Gravitational Torque 33%
• Vertical Scale Height 33%
• Collective Oscillation 33%
• Self-gravitating 33%
• Protostellar 33%

Physics

• Gravitational Instability 100%
• Angular Momentum 66%
• Kinetic Energy 33%
• Wentzel-Kramer-Brillouin Method 33%
• Potential Energy 33%
• Scale Height 33%
• Extrasolar Gas Giants 33%
• Hydrodynamics 33%
• Chilling 33%
• Protoplanetary Disk 33%
• Transportation 33%