Forming the cores of giant planets from the radial pebble flux in protoplanetary discs

Physics & Astronomy

• protoplanetary disks 100%
• planets 74%
• protoplanets 62%
• planetary cores 52%
• dust 40%
• gases 24%
• gas giant planets 24%
• stars 21%
• Neptune (planet) 21%
• embryos 19%
• coagulation 18%
• extrasolar planets 17%
• solar system 16%
• solid surfaces 16%
• metallicity 15%
• seeds 14%
• fragmentation 14%
• envelopes 13%
• fragments 13%
• dissipation 12%
• trapping 12%
• orbits 11%
• orbitals 11%
• life (durability) 10%

Earth & Environmental Sciences

• pebble 89%
• planetesimal 82%
• planet 72%
• core (planetary) 68%
• dust 44%
• gas 41%
• accretion 37%
• Neptune 27%
• solar system 21%
• temporal evolution 21%
• embryo 20%
• trapping 19%
• coagulation 19%
• dissipation 18%
• fragmentation 17%
• particle size 14%
• particle 10%