Formation of Super-Earths and Mini-Neptunes from Rings of Planetesimals
The solar system's planetary architecture has been proposed to be consistent with the terrestrial and giant planets forming from material rings at ∼1 au and ∼5 au, respectively. Here, we show that super-Earths and mini-Neptunes may share a similar formation pathway. In our simulations conducted...
Saved in:
Main Authors: | Sho Shibata, Andre Izidoro |
---|---|
Format: | Article |
Language: | English |
Published: |
IOP Publishing
2025-01-01
|
Series: | The Astrophysical Journal Letters |
Subjects: | |
Online Access: | https://doi.org/10.3847/2041-8213/ada3d1 |
Tags: |
Add Tag
No Tags, Be the first to tag this record!
|
Similar Items
-
Most Super-Earths Have Less Than 3% Water
by: James G. Rogers, et al.
Published: (2025-01-01) -
Interior Convection Regime, Host Star Luminosity, and Predicted Atmospheric CO2 Abundance in Terrestrial Exoplanets
by: Antonin Affholder, et al.
Published: (2025-01-01) -
Secular Perturbations from Exterior Giants Strongly Influence Gap Complexity in Peas-in-a-pod Exoplanetary Systems
by: Joseph R. Livesey, et al.
Published: (2025-01-01) -
Tracing the Winds: A Uniform Interpretation of Helium Escape in Exoplanets from Archival Spectroscopic Observations
by: Patrick McCreery, et al.
Published: (2025-01-01) -
An HST Transmission Spectrum of the Closest M Dwarf Transiting Rocky Planet LTT 1445Ab
by: Katherine A. Bennett, et al.
Published: (2025-01-01)