Linked from

The 10 pages that link to Poynting–Robertson effect, each with the reason it gives.

• Radiation pressureRelated: Radiation pressure’s relativistic tangential component makes orbiting dust spiral inward.

• Orbital perturbationBroader topic: It slowly removes orbital energy from small particles around the Sun.

• Zodiacal lightRelated: It draws dust inward, helping shape the cloud that produces the light.

• Solar radiation pressureCompared with: It is a radiation-related drag, not the outward pressure from direct illumination.

• Debris diskRelated: It can draw small grains inward faster than collisions replenish them.

• Meteor showerRelated: This force gradually shifts small particles within streams and affects their long-term distribution.

• Rings of JupiterRelated: It removes ring dust over time, requiring continued replenishment.

• FomalhautRelated: It helps determine how quickly small grains in Fomalhaut’s disk migrate toward the star.

• GegenscheinRelated: It helps determine how dust is transported through the inner Solar System.

• Interplanetary dust cloudRelated: It draws many grains inward toward the Sun.