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- W1615527758 abstract "Our zodiacal cloud consists of small (~10-100 μm) dust grains, likely created by collisions between asteroids or Kuiper belt objects, and by comets. The smallest grains are ejected from the system while larger particles remain in orbit and slowly spiral inwards toward the host star due to Poynting-Robertson (PR) drag. As the particles spiral inwards, they can become trapped in mean motion resonances (MMRs) with planets, significantly extending their lifetimes. This prolonged trapping can produce a density structure in the dust disk." @default.
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- W1615527758 date "2007-06-01" @default.
- W1615527758 modified "2023-09-23" @default.
- W1615527758 title "Debris Disk Structures Induced by Terrestrial-Mass Planets" @default.
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