Cosmology is the scientific study of the large-scale properties and structure of the universe as a whole, focusing on its origins, evolution, and eventual fate.
Overview
The Big Bang Theory
History Of Cosmology
The Fate Of The Universe
Dark Matter And Dark Energy
Galaxies And Galactic Spheres
The Structure Of The Universe
Cosmic Microwave Background Radiation
Current Research And Future Discoveries
James Webb Space Telescope
Nicolaus Copernicus
Andromeda Galaxy
Big Bang Theory
Dark Energy
Temperature
Dark Matter
Cosmic Web
Universe
๐ The observable universe is about 93 billion light-years in diameter.
๐ญ The universe is approximately 13.8 billion years old.
๐ There are an estimated 100 billion galaxies in the observable universe.
๐ Dark matter makes up about 27% of the universe's total mass and energy.
โจ Dark energy accounts for around 68% of the universe, driving its accelerated expansion.
๐ซ The Big Bang theory describes the origin of the universe from an infinitely dense point.
๐ The cosmic microwave background radiation is the afterglow of the Big Bang, detectable today.
๐ Gravitational waves are ripples in spacetime caused by massive accelerating objects.
๐ The multiverse theory suggests there could be multiple, perhaps infinite, universes beyond our own.
๐ The universe is expanding, and this expansion is accelerating due to dark energy.
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