Supernovae Star Formation Supermassive Black Holes X-ray Astronomy Black Holes Interstellar Objects Solar Activity Charged Particles Magnetars Fast Radio Bursts Neutron Stars Comet Composition Radio Waves Magnetic Fields Supernova Remnants Cometary Studies Radiation Solar Wind Transient Events Cometary Behavior X-ray Emissions Accretion Disks Celestial Bodies Gamma-Ray Bursts Comets Stellar Evolution Flares Interstellar Travel Cosmic Rays Radio Signals Shock Waves Gas and Dust Clouds Pulsars Cometary Activity Neutrino Astronomy High-Energy Emissions Gravitational Waves Dark Matter Trajectory Analysis Stellar Winds Object Trajectories Asteroids Planetary Systems Energy Emission Galaxies Natural vs Artificial Objects Celestial Mechanics Electromagnetic Radiation Explosions Cosmic Dark Ages X-ray Emission Radio Emissions Interstellar Visitors Interstellar Medium Cosmic Accelerators Celestial Jewelry Dimming Stars Energy Jets Black Hole Growth Cosmic Microwave Background Radiation Orbital Mechanics Gravitational Effects Cosmic Radiation Light Observation Magnetized Stars Mass Transfer Space Weather Energy Transfer Hydrogen Clouds Protostars Radio Jets Energy Release Light Years Early Universe Studies Solar Eruptions Cosmic Web Eclipses Planetary Atmospheres Micrometeoroids Cosmic Flares Particle Collisions Disintegration Events Gas Dynamics Luminosity Variations Dark Energy and Dark Matter Active Galactic Nuclei Star Interactions Meteoroids Dark Energy Blazars Pulsars and Cosmic Objects Cosmic Events Electrostatic Discharge Energy Discharges Comet Origins Auroras Energy Outbursts Space Travel Comets and Asteroids Stellar Dynamics
Scientists describe the rare interstellar visitor as a natural, volatile‑driven comet posing no risk.