On the Origin of Jupiter’s Fuzzy Core: Constraints from N-body, Impact, and Evolution Simulations
It has been suggested that Jupiter’s fuzzy core could be a result of a giant impact. Here, we investigate the expected impact conditions from N -body simulations. We then use state-of-the-art smoothed particle hydrodynamics simulations to investigate the results of impacts with different conditions...
Saved in:
Main Authors: | Thomas Meier, Christian Reinhardt, Sho Shibata, Simon Müller, Joachim Stadel, Ravit Helled |
---|---|
Format: | Article |
Language: | English |
Published: |
IOP Publishing
2025-01-01
|
Series: | The Astrophysical Journal |
Subjects: | |
Online Access: | https://doi.org/10.3847/1538-4357/addbe6 |
Tags: |
Add Tag
No Tags, Be the first to tag this record!
|
Similar Items
-
An Energy Perspective of Core Erosion in Gas Giant Planets
by: J. R. Fuentes, et al.
Published: (2025-01-01) -
A Resonant Beginning for the Solar System’s Terrestrial Planets
by: Shuo Huang, et al.
Published: (2025-01-01) -
Absence of a Runaway Greenhouse Limit on Lava Planets
by: Iris D. Boer, et al.
Published: (2025-01-01) -
Atmospheres /
by: Goody, Richard M.
Published: (1972) -
Hydrogen Loss on Venus Driven by Photochemistry
by: Hao Gu, et al.
Published: (2025-01-01)