Why Do Galaxies Need Dark Matter? The Evidence Behind Galactic Structure and Motion
Galaxies appear to need dark matter to stay bound, rotate as observed, and build the large-scale structure of the universe.
Galaxies appear to need dark matter to stay bound, rotate as observed, and build the large-scale structure of the universe.
Learn what dark matter is, how it affects galaxies, and why it remains one of modern astronomy’s biggest mysteries.
What is the Ionosphere? The ionosphere is a region of Earth’s upper atmosphere that is ionized by solar and cosmic radiation. It is located between 30 and 600 kilometers above the Earth’s surface and is composed of a layer of charged particles known as ions. These ions are created when high-energy radiation from the sun … Read more
Supernovae reveal dark energy by acting as distance markers that show the universe’s expansion is speeding up.
Explore why pulsars pulse, how rotating neutron stars create lighthouse-like beams, and what astronomers learn from their regular signals.
Learn how dark energy and dark matter differ, what each does, and why both are essential to modern cosmology.
Discover how astronomers infer dark matter’s location using gravity, lensing, galaxy motions, and cosmic surveys.
Explore the leading ways scientists may finally detect dark matter, from underground detectors to astrophysical signatures and collider experiments.
I. What is Cosmography? Cosmography is the study of the universe as a whole, including its structure, composition, and evolution. It is a branch of cosmology that focuses on mapping and understanding the physical and spatial relationships of celestial bodies and phenomena. Cosmography seeks to answer fundamental questions about the nature of the universe, such … Read more
Explore the physics behind neutron star magnetism, from collapsed stellar cores to dynamo action, flux conservation, and magnetars.