Super-Earth masses inferred from Kepler match the pebble isolation mass in viscously heated discs only if planets form within the first million years, while passive discs require mergers.
Title resolution pending
1 Pith paper cite this work. Polarity classification is still indexing.
1
Pith paper citing it
fields
astro-ph.EP 1years
2019 1verdicts
CONDITIONAL 1representative citing papers
citing papers explorer
-
Inner rocky super-Earth formation: distinguishing the formation pathways in viscously heated and passive discs
Super-Earth masses inferred from Kepler match the pebble isolation mass in viscously heated discs only if planets form within the first million years, while passive discs require mergers.