Dark Energy Research Primordial Black Holes Galaxies Composition Nature of Dark Matter Characteristics Detection Cosmic Web Properties Detection Methods Models Theories Measurement Distribution Galaxy Clusters Dark Matter Halo Nature Understanding Dark Matter Dark Matter Candidates Existence Theoretical Physics Hypotheses Halo Structures Nonvisible Forces Galactic Dark Matter Distribution Cold Dark Matter Theories Self-Interacting Dark Matter Light Bending Dark Matter-Hunting Telescope Origin of Intracluster Stars Properties of Dark Matter Galactic Stability Milky Way Distribution Vera C. Rubin's Contributions Cosmological Simulations Euclid Mission Galaxy Formation Computer Simulations LSST Survey Galactic Interactions Astrophysics Observable Universe Cosmic Discoveries Cosmology Gravitational Effects Quasar Studies Cosmic Structures Observations Distribution Patterns Dark Matter Filaments Dark Matter Detection Techniques Mapping Gravitational Lensing Influence Cold Dark Matter Missing Satellites Problem Observational Astronomy Fermionic Dark Matter Gamma Rays Formation of Dark Matter Concentrations Unknown Particles Brown Dwarfs Coma Cluster Infrared Detection Euclid Mission Capabilities Gravitational Forces Dark Matter Haloes Matter Distribution Dark Side of the Universe Telescopes Galaxy Dynamics Dark Matter Models Dwarf Galaxies Celestial Objects Dark Matter Theories Dark Energy Theories
Stacked images around four tightly grouped globular clusters expose CDG-2’s diffuse starlight, making it the strongest dark‑galaxy candidate reported.
