Comets Interstellar Objects Stars Asteroids Nebulae Planets Brown Dwarfs Galaxies Near-Earth Objects Star Clusters Constellations Black Holes Neutron Stars Moons Moon Rogue Planets Dwarf Planets Meteors Interestelar Objects Pulsars Sun Mini-Moons Kometen Globular Clusters White Dwarfs Binary Stars Oort Cloud Kuiper Belt Icy Bodies Interstellar Comets Interestellar Objects Deep-Sky Objects Planetary Nebulae Exoplanets Trans-Neptunian Objects Observation Techniques Hypervelocity Objects Supernovae Brightness Binary Systems Star Systems Substellar Objects Nebulas Supernova Remnants Sednoids Long-Period Transients Stellar Evolution Quasi-Moons Gas Giants Quasars Orbits Solar System Comets and Asteroids Star Formation Co-orbital Asteroids Orbital Mechanics Telescopes Outer Planets Molecular Clouds Stellar Remnants Debris Disks Telescope Asteroids and Comets Trajectory Analysis Gas Clouds Bright Stars Comparative Analysis Sonnensystem Detection Techniques Star Naming Planetary Formation Interestellar Comets Other Comets Supergiant Stars Outer Solar System Transneptunian Objects Nomenclature Cometary Studies Meteoroiden Discovery of Interstellar Objects Kuiper Belt Objects Failed Galaxies Dying Stars Arrokoth New Discoveries Meteoroids Reflection Nebulae Young Stars Pillars of Creation Position Prediction Great Globular Cluster Dark Comets Protostars Galaxy Cataloging Uranus Asteroiden Citizen Science Red Dwarf Stars Fast-moving Objects Rogue Worlds
Multiwavelength data show visible dimming with an infrared spike, signaling hot debris from an impact.
