The entire wiki reimagined as a visual magazine with video discovery · Watch your interests come alive
The entire wiki reimagined as a visual magazine with video discovery · Watch your interests come alive
The Holmdel Horn Antenna on which Penzias and Wilson discovered the cosmic microwave background.
The Holmdel Horn Antenna on which Penzias and Wilson discovered the cosmic microwave background.
Comparison of CMB results from COBE, WMAP and Planck (March 21, 2013)
Comparison of CMB results from COBE, WMAP and Planck (March 21, 2013)
Artist impression of the gravitational lensing effect of massive cosmic structures
Artist impression of the gravitational lensing effect of massive cosmic structures
Temperature power spectrum and E-mode and B-mode polarization power spectra of the cosmic microwave background
Temperature power spectrum and E-mode and B-mode polarization power spectra of the cosmic microwave background
Hubble Ultra-Deep Field image of a region of the observable universe (equivalent sky area size shown in bottom left corner), near the constellation Fo
Hubble Ultra-Deep Field image of a region of the observable universe (equivalent sky area size shown in bottom left corner), near the constellation Fornax. Each spot is a galaxy, consisting of billions of stars. The light from the smallest, most redshifted galaxies originated around 12.6 billion years ago, close to the age of the universe.
Computer simulated image of an area of space more than 50 million light-years across, presenting a possible large-scale distribution of light sources
Computer simulated image of an area of space more than 50 million light-years across, presenting a possible large-scale distribution of light sources in the universe—precise relative contributions of galaxies and quasars are unclear.