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Early Jupiter Shaped Earth's Formation Zone, Study Finds

High-resolution simulations link the gas giant’s rapid birth to disk rings that delayed a second generation of solids.

Overview

  • Rice University researchers used hydrodynamic and dust-evolution simulations, publishing their results in Science Advances.
  • The model indicates Jupiter formed within about 2 million years, opening a wide gap that split the protoplanetary disk into inner and outer zones.
  • Higher-pressure ridges created dust traps that account for the 2–3 million-year age gap recorded in meteorites.
  • By blocking inward flows of gas and dust, Jupiter likely kept terrestrial material from spiraling into the Sun and prevented super-Earth outcomes near 1 AU.
  • The authors contend their framework may be the first to unite Jupiter’s growth, dust transport, and asteroid formation into a single explanation consistent with meteoritic evidence.