Formation of dust-rich planetesimals from sublimated pebbles inside of the snow line

2016/10/31 by Shigeru Ida, Tristan Guillot, T. Guillot · 4 citations
Mathematics · Physics and Astronomy · #Astro and Planetary Science #Astrobiology #Astrophysics #Astrophysics and Star Formation Studies #Context (archaeology) #Geology #Geometry #Inflow #Line (geometry) #Mathematics #Mechanics #Meteorology #Physics #Planet #Planetesimal #Snow #Snow cover #Snow line #Stellar, planetary, and galactic studies #astro-ph.EP

paper · pdf · doi:10.1051/0004-6361/201629680

5 pages, 3 figures; accepted for publication in Astronomy and Astrophysics

arxiv created 2016/11/05 · openalex publication_date 2016/11/08 · openalex created_date 2016/11/11 · arxiv updated 2016/12/07 · openalex updated_date 2026/08/06

Abstract

Context. For up to a few millions of years, pebbles must provide a quasi-steady inflow of solids from the outer parts of protoplanetary disks to their inner regions.

Citations

• Streaming Instabilities in Protoplanetary Disks
• The Formation of Planetesimals
• Can dust coagulation trigger streaming instability?
• HALL EFFECT CONTROLLED GAS DYNAMICS IN PROTOPLANETARY DISKS. II. FULL 3D SIMULATIONS TOWARD THE OUTER DISK
• Survival of the mm-cm size grain population observed in protoplanetary disks
• Solar System Abundances and Condensation Temperatures of the Elements
• The radial dependence of pebble accretion rates: A source of diversity in planetary systems

Cited by

• The Effect of Jupiter's Formation on the Distribution of Refractory Elements and Inclusions in Meteorites
• Formation of Terrestrial Planets
• Dust Evolution and Satellitesimal Formation in Circumplanetary Disks
• Rocky Planetesimal Formation Aided by Organics