Dark Energy Cosmic Structures Galaxy Formation Dark Matter Halos Research Galaxy Evolution Hypothetical Particles Galactic Structure Cosmology Gravitational Lensing Exotic Particles Vera Rubin Cosmic Structure Properties Primordial Black Holes Dark Matter Detection Theoretical Physics Exoplanets Detection Methods Mini-halo Formation Cosmic Phenomena Fundamental Physics Normal Matter Theories of Dark Matter Axion Clouds ΛCDM Model Axion Dark Matter Light Dark Matter Gravitational Effects Hernquist Halo Galaxy Mass Galaxies Evidence of Existence Observational Techniques Asteroids Halo Models Black Holes Galaxy Dynamics Properties of Dark Matter Cosmic Mapping Dark Star Clusters Halos Theories Fermions Cosmic Dust Dark Electrons Characteristics Neutrino Theories Dark Energy Surveys Neutron Stars Galactic Dynamics Galactic Structures Self-Interacting Dark Matter Cosmological Models Halo Mass Function Ultralight Dark Matter Galaxy Composition Interstellar Medium Sterile Neutrinos Research Questions Historical Theories Experimental Searches Halo Formation Gravitational Influence Dwarf Galaxies
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The coronagraph is powered on for months of calibration and the mission will deliver large, open data streams that aim to transform studies of dark matter, dark energy and exoplanets.
