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Volume 643 Issue 8072, 17 July 2025
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Volume 643 Issue 8072, 17 July 2025

Forged in fire

The terrestrial planets in our Solar System are thought to have formed from a mixture of interstellar solids and rocky material that precipitated out from the cooling hot gas around the young Sun. The moment minerals start to condense from hot gas is the moment the clock starts for planet formation. In this week’s issue, Melissa McClure and colleagues present astronomical observations of this planet-forming zero hour for the protostar HOPS-315 in the Orion B molecular cloud. Captured by the James Webb Space Telescope (JWST) and the Atacama Large Millimeter/submillimeter Array (ALMA), the observations suggest that interstellar solids near the protostar burn up and recondense as crystalline minerals at the base of a narrow jet of silicon monoxide and carbon monoxide. The cover image shows an artist’s impression of this moment based on the ALMA map of carbon monoxide at HOPS-315. The similarities between the environment of HOP-315 and the Solar System suggest that this protostar could make a good proxy for studying how planetary bodies formed closer to home.

Cover image: Luis Calçada/ESO for Nature.

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