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Showing 1 to 4 of 4 for “"debris disc"”.

  1. Secular Dynamics of Self-gravitating Debris Discs

    Debris discs are the leftovers from the epoch of planetary formation, akin to the Solar System's asteroid and Kuiper belts. They preserve a record of the physical processes at work throughout the system's age, not least planet--disc interactions. Deciphering this record has become a central focus …

    cambridge Repository record for Secular Dynamics of Self-gravitating Debris Discs (opens in a new tab)

  2. High-resolution studies of exoplanetesimal belt formation and evolution

    Stars are born with gas-rich protoplanetary discs that typically survive for a few Myr before dispersing, after which they are left with the planetary bodies that formed within the protoplanetary system: planets, and belts of planetesimals (km-sized rocky and icy bodies). Planetesimals within belts …

    cambridge Repository record for High-resolution studies of exoplanetesimal belt formation and evolution (opens in a new tab)

  3. The origin and evolution of warm exozodiacal dust

    … of P-R drag and catastrophic collisions in a debris disc which predicts the levels of exozodiacal dust dragged into the habitable zone of a star from a cold outer belt. I show that detectable outer belts should produce exozodi levels tens of times higher than our zodiacal cloud via P-R drag, …

    cambridge Repository record for The origin and evolution of warm exozodiacal dust (opens in a new tab)

  4. EXOCOMETS AT LARGE ORBITAL RADII AND THEIR INWARD TRANSPORT IN DEBRIS DISCS

    … down solids producing dust and giving rise to debris discs. Primitive asteroids and comets likely played a major role in the emergence of life on Earth through their delivery of volatiles early in the lifetime of our planet. Cometary impacts, therefore, could be a necessary condition for the …

    cambridge Repository record for EXOCOMETS AT LARGE ORBITAL RADII AND THEIR INWARD TRANSPORT IN DEBRIS DISCS (opens in a new tab)