Core Formation and Internal Structure of Planetesimals: The Role of Formation Time, Accretion Duration, and Terminal Size

· by · in , , , , ,

T. Suwa, H. Nagahara

48th Lunar and Planetary Science Conference (2017), Abstract #2130

LINK

Related posts (automatically generated):

  1. Structure of differentiated planetesimals: A chondritic fridge on top of a magma ocean
  2. Effects of pebble accretion on the growth and composition of planetesimals in the inner Solar SystemOPEN ACCESS 
  3. Early accretion of planetesimals unraveled by the thermal evolution of the parent bodies of magmatic iron meteorites
  4. Rocky Planetesimal Formation Aided by Organics
  5. The Effect of a Strong Pressure Bump in the Sun’s Natal Disk: Terrestrial Planet Formation via Planetesimal Accretion Rather than Pebble Accretion
  6. Meteorite evidence for partial differentiation and protracted accretion of planetesimalsOPEN ACCESS 
  7. Origin of water in the inner Solar System: planetesimals scattered inward during Jupiter and Saturn’s rapid gas accretionOPEN ACCESS 
  8. Dynamical orbital evolution of asteroids and planetesimals across distinct chemical reservoirs due to accretion growth of planets in the early solar systemOPEN ACCESS 
  9. Contemporary formation of early Solar System planetesimals at two distinct radial locationsOPEN ACCESS 
  10. A pebble accretion model for the formation of the terrestrial planets in the Solar SystemOPEN ACCESS 
Tags: ,