Cosmology
Investigating the origin, evolution, fundamental structure, and ultimate fate of the entire universe.
Explore by Cosmology

July 31, 2026
How Old Is the Universe? 155,600 Ancient Stars, a 13.73 Gyr Floor, and the Hubble Tension

July 30, 2026
South Pole Telescope Finds 7,190 Galaxy Clusters: Inside the SPT-3G 5-Year Sunyaev-Zel'dovich Catalog

July 29, 2026
Does Dark Energy Exist? Tilted Observers, the >7σ q₀ Dipole, and Pantheon+ Deceleration

July 28, 2026
Is Early Dark Energy Dead? Axion EDE and the 3.3σ Hubble Tension

July 27, 2026
Was the Electron Heavier in the Early Universe? Varying mₑ and the Hubble Tension

July 26, 2026
Did AGN Feedback Solve the S8 Tension? SPT-3G Compton-y Maps & 21σ Cross-Correlation

July 25, 2026
Is the Universe Flat or Closed? The Ω_k Curvature Tension After ACT DR6 and DESI DR2

July 24, 2026
Is the Universe a Donut? Cosmic Topology, Matched Circles, and the E1–E18 Manifold Search

July 23, 2026
Are Primordial Black Holes Dark Matter? CMB μ-Distortion Limits & QCD-Epoch Formation
FAQs about Cosmology
Cosmology is the scientific study of the entire universe. It asks questions about how the universe began, how it has evolved, and what its ultimate fate will be.
The Big Bang Theory is our best explanation for how the universe started. It states that the universe began as an extremely hot, dense point about 13.8 billion years ago and has been expanding and cooling ever since.
These are the two biggest mysteries in cosmology. Dark matter is an invisible substance that provides extra gravity to hold galaxies together. Dark energy is a mysterious force that is causing the expansion of the universe to accelerate.
Because light takes time to travel, looking at distant galaxies is like looking back in time. Telescopes like Hubble and James Webb allow us to see galaxies as they were billions of years ago, giving us clues about the early universe.