Dark Energy Gamma Rays Research Findings Gravitational Lensing WIMPs Galaxy Formation Primordial Black Holes Galaxies Research Dark Dwarfs Galactic Dynamics Fast Radio Bursts Black Hole Research High-Redshift Stars Research Discoveries Vera C. Rubin Observatory Supermassive Black Holes Dark Matter Theories Euclid Telescope Dark Matter Distribution New Cosmological Model Challenges to Prevailing Theories Gravitational Phenomena Quasars Mystery of Dark Matter Galaxy Formation Theory Missing Matter Baryonic Matter Intergalactic Space Dark Matter Halos Evolving Dark Matter Galactic Interactions Vera C. Rubin's Contributions Cosmic Evolution Molecular Clouds Planet Nine Vera Rubin Observatory Cosmic Structures Gravitational Waves Reionization-Limited H I Cloud Filaments Theoretical Physics Reionization-Limited H I Clouds Dark Matter Annihilation Cosmic Entities Lambda-CDM Model Dwarf Galaxies Research Applications Dark Matter Halo Cosmic Dark Ages Self-Interacting Dark Matter Dark Stars Euclid Mission Subhalos Detection Weakly Interacting Massive Particles (WIMPs) Detection of Dark Matter Weakly Interacting Massive Particles Gamma-ray Observations Detection Methods Halo Shapes Nature of Dark Matter Halo Properties Observational Evidence Dark Matter Entities Dark Matter Particles Dark Matter Detection Characteristics Galactic Ecosystems Self-Interaction Cosmic Expansion Influence on Galaxy Motion
Deep Hubble imaging ruled out even faint starlight, making the object a benchmark for testing dark matter physics.
