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Simulations Undercut Giant-Impact Origin of Jupiter’s Fuzzy Core

A peer-reviewed MNRAS study using DiRAC COSMA models finds a gradual accretion process better matches Juno’s observations.

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Jupiter in true colour by Hubble's "Outer Planet Atmospheres Legacy" - January 5 2024 (Credit : NASA/STSCI)

Overview

  • High-resolution collision simulations failed to reproduce the stable dilute core structure inferred from NASA’s Juno data.
  • The models showed that impact-disrupted core material would re-settle into distinct layers rather than form a smooth transition.
  • The authors conclude Jupiter’s interior likely emerged through slow incorporation of heavy and light elements over time.
  • Evidence that Saturn also hosts a dilute core strengthens the case for gradual formation over rare, extreme impacts.
  • Research by Durham University with NASA, the SETI Institute, and the University of Oslo ran on DiRAC COSMA using the open-source SWIFT code, informing interpretations of giant-planet and exoplanet interiors.