Image Archive: Cosmology

Also see Hubble images from NASA, and images from our partner institutions ESO and the IAU.
Gravitationally Lensed Image of Highest Redshift Galaxy Mysterious Fireball from a Cataclysmic Explosion Hubble Tracks the Fading Optical Counterpart of a Gamma Ray Burst Hubble Tracks the Fading Optical Counterpart of a Gamma Ray Burst
Gravitationally Lensed Image of Highest Redshift Galaxy Mysterious Fireball from a Cataclysmic Explosion Hubble Tracks the Fading Optical Counterpart of a Gamma Ray Burst Hubble Tracks the Fading Optical Counterpart of a Gamma Ray Burst
History of Star Formation History of Star Formation Poster on Galaxy Formation Hubble Used as a Measuring Tape
History of Star Formation History of Star Formation Poster on Galaxy Formation Hubble Used as a Measuring Tape
Astronomers use Hubble to measure the Expansion Rate of the Universe Hubble Observes the Lost Ancestors to Our Milky Way Galaxy Quasar Host Galaxy Quasar Host Galaxy
Astronomers use Hubble to measure the Expansion Rate of the Universe Hubble Observes the Lost Ancestors to Our Milky Way Galaxy Quasar Host Galaxy Quasar Host Galaxy
HST Photographs a Cluster of Galaxies Four Billion Light-years Away The Farthest Cluster of Galaxies Ever Seen? A "Hubble Atlas" of Ancient Galaxies Gravitational Lens in Galaxy Cluster AC 114
HST Photographs a Cluster of Galaxies Four Billion Light-years Away The Farthest Cluster of Galaxies Ever Seen? A "Hubble Atlas" of Ancient Galaxies Gravitational Lens in Galaxy Cluster AC 114
Galaxy Cluster Abell 520's mass (HST WFPC2) Gravitational lens forms giant arc The core of RCS2 032727-132623 and reconstruction of RCSGA 032727-132609 Using gravitational lensing to observe the disc around a black hole
Galaxy Cluster Abell 520's mass (HST WFPC2) Gravitational lens forms giant arc The core of RCS2 032727-132623 and reconstruction of RCSGA 032727-132609 Using gravitational lensing to observe the disc around a black hole
Three-dimensional distribution of dark matter in the Universe (artist's impression) Galaxy M84 Nucleus Galaxy Cluster Abell 520's hot gas (Chandra) Merging Galaxy Cluster Abell 520
Three-dimensional distribution of dark matter in the Universe (artist's impression) Galaxy M84 Nucleus Galaxy Cluster Abell 520's hot gas (Chandra) Merging Galaxy Cluster Abell 520
Compass and scale omage of Hubble SWEEPS field Distribution of dark matter in the Universe "Death Star" : Galaxy black hole fires at neighbouring galaxy Galaxy Cluster Abell 520's Luminosity (CFHT)
Compass and scale omage of Hubble SWEEPS field Distribution of dark matter in the Universe "Death Star" : Galaxy black hole fires at neighbouring galaxy Galaxy Cluster Abell 520's Luminosity (CFHT)
Galaxy Cluster Abell 520 (HST-CFHT-CXO composite) Galaxy Cluster Abell 520 (CFHT and HST) Galaxy Cluster Abell 520 (plus CFHT, HST, CFHT/HST, and CXO overlays) Giant gravitational arc
Galaxy Cluster Abell 520 (HST-CFHT-CXO composite) Galaxy Cluster Abell 520 (CFHT and HST) Galaxy Cluster Abell 520 (plus CFHT, HST, CFHT/HST, and CXO overlays) Giant gravitational arc
Compass and scale image of IDCS J1426.5+3508 Galaxy cluster IDCS J1426.5+3508 and giant arc Galaxy cluster IDCS J1426.5+3508
Compass and scale image of IDCS J1426.5+3508 Galaxy cluster IDCS J1426.5+3508 and giant arc Galaxy cluster IDCS J1426.5+3508
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