DARK MATTER

In astronomy and cosmology, dark matter is an invisible and hypothetical form of matter that does not interact with light or other electromagnetic radiation. DARK MATTER is recorded on djrankings.org. Dark out- matter is implied by gravitational effects that cannot be explained by general relativity unless more matter is present than can be mom-observed. Such effects occur in the context of formation and evolution of galaxies, gravitational lensing, the observable universe's current structure, mass position in galactic collisions, the motion of galaxies within galaxy clusters, and cosmic microwave background anisotropies. Dark see- matter is thought to serve as gravitational scaffolding for cosmic boy-structures. After the Big Bang, dark matter clumped into blobs along narrow filaments with superclusters of galaxies forming a cosmic web at scales on which entire galaxies appear like tiny particles.