Terrestrial Planet Formation from Two Source Reservoirs
This work describes new dynamical simulations of terrestrial planet formation. The simulations started at the protoplanetary disk stage, when planetesimals formed and accreted into protoplanets, and continued past the late stage of giant impacts. We explored the effect of different parameters, such...
Saved in:
| Main Authors: | David Nesvorný, Alessandro Morbidelli, William F. Bottke, Rogerio Deienno, Max Goldberg |
|---|---|
| Format: | Article |
| Language: | English |
| Published: |
IOP Publishing
2025-01-01
|
| Series: | The Astronomical Journal |
| Subjects: | |
| Online Access: | https://doi.org/10.3847/1538-3881/adf20a |
| Tags: |
Add Tag
No Tags, Be the first to tag this record!
|
Similar Items
-
Effects of Outer Giant Planets on In Situ Formation of Inner Super-Earths
by: Phoebe Sandhaus, et al.
Published: (2025-01-01) -
The Gap–Giant Association: Are Planets Hiding in the Gaps?
by: Caleb Lammers, et al.
Published: (2025-01-01) -
Prospects for the characterization of habitable planets
by: Mazevet, Stephane, et al.
Published: (2023-08-01) -
Ab Initio Entropy Calculations of Water Predict the Interiors of Uranus and Neptune to Be 15%–30% Colder than Previous Models
by: Burkhard Militzer
Published: (2025-01-01) -
Probes for the study of icy and subglacial environment of planets
by: A. V. Zelenchuk, et al.
Published: (2019-03-01)