Dark Energy Research Composition Nature of Dark Matter Galaxies Primordial Black Holes Measurement Distribution Cosmic Web Galaxy Clusters Detection Models Detection Methods Nature Dark Matter Halo Properties Matter Distribution Euclid Mission Understanding Dark Matter Dark Side of the Universe Nonvisible Forces Characteristics Gravitational Lensing Galaxy Formation Dark Matter Haloes Gamma Rays Existence Cosmology Dark Energy Theories Distribution Patterns Dark Matter Filaments Dark Matter-Hunting Telescope Mapping Gravitational Effects Dark Matter Theories Dark Matter Models Observations Properties of Dark Matter Cold Dark Matter Theories Influence Gravitational Forces Coma Cluster Formation of Dark Matter Concentrations Quasar Studies Light Bending Galactic Stability LSST Survey Computer Simulations Observable Universe Cosmological Simulations Galactic Interactions Origin of Intracluster Stars Dwarf Galaxies Halo Structures Cosmic Discoveries Observational Astronomy Astrophysics Celestial Objects Vera C. Rubin's Contributions Telescopes Brown Dwarfs Euclid Mission Capabilities Infrared Detection Self-Interacting Dark Matter Cold Dark Matter Unknown Particles Hypotheses Missing Satellites Problem Galactic Dark Matter Distribution Galaxy Dynamics Dark Matter Detection Techniques Theories Milky Way Distribution Theoretical Physics
Deep Hubble imaging ruled out even faint starlight, making the object a benchmark for testing dark matter physics.
