The influence of cold Jupiters in the formation of close-in planets. I. planetesimal transport

The influence of cold Jupiters in the formation of close-in planets. I. planetesimal transport

The formation of a cold Jupiter (CJ) is expected to quench the influx of pebbles and the migration of cores interior to its orbit, thus limiting the efficiency of rocky planet formation either by pebble accretion and/or orbital migration. Observations, however, show that the presence of outer CJs (...

Ausführliche Beschreibung

Gespeichert in:
Bibliographische Detailangaben
Veröffentlicht in:arXiv.org 2023-09
Hauptverfasser: Best, Marcy, Sefilian, Antranik A, Petrovich, Cristobal
Format: Artikel
Sprache:eng
Schlagworte:
Decay rate
Deposition
Drag
Extrasolar planets
Gas giant planets
Jupiter
Nebulae
Orbit decay
Planet formation
Planetary systems
Radial velocity
Resonance
Terrestrial planets
Online-Zugang:Volltext
Tags: Tag hinzufügen
Keine Tags, Fügen Sie den ersten Tag hinzu!
Beschreibung
Zusammenfassung:The formation of a cold Jupiter (CJ) is expected to quench the influx of pebbles and the migration of cores interior to its orbit, thus limiting the efficiency of rocky planet formation either by pebble accretion and/or orbital migration. Observations, however, show that the presence of outer CJs ( >1 au and >0.3 Jupiter masses) correlates with the presence of inner Super Earths (at
ISSN:2331-8422