SUMMARY
Radiation from a star effectively clears dust from a proto-planetary disc by exerting radiation pressure that pushes smaller dust particles outward, transitioning the area from opaqueness to transparency. The force of radiation pressure is proportional to the radius squared, while gravitational force is proportional to the radius cubed, which explains why smaller particles are more affected by radiation than larger, more massive objects. This differential scaling illustrates fundamental principles in astrophysics regarding the interaction between radiation and matter.
PREREQUISITES
- Understanding of radiation pressure and its effects on small particles
- Basic knowledge of gravitational forces and mass distribution
- Familiarity with the concepts of proto-planetary discs in astrophysics
- Awareness of scaling laws in physics
NEXT STEPS
- Research the role of radiation pressure in astrophysical processes
- Explore the dynamics of proto-planetary disc formation and evolution
- Study the mathematical relationships between force, mass, and radius in astrophysics
- Investigate the implications of differential scaling in various physical systems
USEFUL FOR
Astronomers, astrophysicists, and students of cosmology interested in the mechanisms of dust clearing in proto-planetary discs and the effects of stellar radiation on small particles.