How to form planetesimals from mm-sized chondrules and chondrule aggregates

· by · in , , , ,

Daniel Carrera, Anders Johansen, Melvyn B. Davies

PDF LINK (full text)

LINK

Related posts (automatically generated):

  1. Growth of asteroids, planetary embryos and Kuiper belt objects by chondrule accretion
  2. Growth of asteroids, planetary embryos, and Kuiper belt objects by chondrule accretion
  3. The Macroporosity of Rubble Pile Asteroid Ryugu and Implications for the Origin of ChondrulesOPEN ACCESS 
  4. Constraints on planetesimal accretion inferred from particle-size distribution in CO chondritesOPEN ACCESS 
  5. Petrological evidence for the existence and disruption of a 500 km-sized differentiated planetesimal of enstatite-chondritic parentage
  6. Fragmentation of colliding planetesimals with water content
  7. Meteorite evidence for partial differentiation and protracted accretion of planetesimalsOPEN ACCESS 
  8. Structure of differentiated planetesimals: A chondritic fridge on top of a magma ocean
  9. Early accretion of planetesimals unraveled by the thermal evolution of the parent bodies of magmatic iron meteorites
  10. Time and Duration of Chondrule Formation: Constraints from 26Al-26Mg Ages of Individual Chondrules
Tags: , , , ,