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New Supercomputer Simulations Undercut Giant-Impact Theory for Jupiter’s Dilute Core

Improved modeling shows displaced heavy material re-settles quickly, pointing to a slow-growth origin for the planet’s interior.

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Overview

  • A Durham-led team used the SWIFT code on the DiRAC COSMA supercomputer with the REMIX SPH approach to test extreme collision scenarios and produced no stable dilute core.
  • In the runs, rock-and-ice core material mixed only briefly before re-forming a sharp boundary with the surrounding hydrogen-helium envelope.
  • The peer-reviewed study, published in Monthly Notices of the Royal Astronomical Society, revisits ideas proposed after Juno’s measurements revealed Jupiter’s gradual core.
  • Authors conclude gradual accretion and internal mixing during formation are the more likely origin, noting recent evidence for a similar dilute core in Saturn.
  • The findings inform how scientists interpret the interiors of Jupiter- and Saturn-sized exoplanets and advance methods for simulating giant planetary impacts.