Solar System Chemical Composition Super-Earths Rocky Planets Earth-Moon System Particle Aggregation Red Dwarf Stars Planetary Characteristics Differentiation Processes Debris Disks Chemical Signatures Interstellar Objects Solar System History Volatiles Delivery Origins of Water Icy Comets Chemical Processes Inner Core Formation Formation Processes Stellar Influence Planetesimals Trans-Neptunian Objects Chemical Evolution Gravitational Influence Cosmic Origins Building Blocks of Planets Meteorite Impacts Moon Formation Theory Protoplanetary Disks Lunar Formation Planetary Destruction Lunar Formation Theories Exoplanets Magma Oceans Isotopes Planetary Systems Magnetosphere Studies Terrestrial Planets Early Earth Differentiation Natural Satellite Origins
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Computer models indicate the first stars’ supernovae could have quickly enriched nearby gas to make water-bearing disks capable of seeding early rocky planets.
