Science ❯ Astronomy ❯ Astrophysics
Active Galactic Nuclei Milky Way Supermassive Black Holes Early Universe Galaxy Formation High-Redshift Galaxies Black Holes Quasars Quiescent Galaxies Galaxy Mergers Gravitational Lensing Dwarf Galaxies Seyfert Galaxies Star Formation M87 Galaxy Evolution Large-Scale Structure Compact Galaxies Interstellar Medium Narrow Line Seyfert 1 Emission-line Galaxies Photometric Redshift Compact Objects Galaxy Collisions Sextans A Hidden Galaxies Radio-loud Galaxies Distant Galaxies Galactic Interactions NGC 5253 Sombrero Galaxy Anomalous Galaxies Hydrogen Gas Halos Cosmology HELM Galaxies Anomalous Objects Lyman-Alpha Emission NGC 4141 Starburst Galaxies Circumgalactic Medium Stellar Dynamics Supernovae Galaxy M87 Markarian 501 Starless Dark Matter Halos Lyman Continuum Escape Lyman-alpha Nebulae Jellyfish Galaxies Early Galaxies Gas Outflows Anomalies NGC 1052 Dark Matter Star-Forming Galaxies Spectral Energy Distribution High-redshift Galaxies Black Hole Stars Atomic Hydrogen Bullet Cluster Survey Techniques
The 2.4‑meter primary mirror passed final inspection, allowing barge transport to Kennedy Space Center for launch processing before final reviews.