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Universe

Physical cosmology Universe · Big Bang Age of the universe Timeline of the Big Bang Ultimate fate of the universe Inflation · Nucleosynthesis GWB · Neutrino background Cosmic microwave background Redshift · Hubble's law Metric expansion of space Friedmann equations FLRW metric Shape of the universe Structure formation Reionization Galaxy formation Large-scale structure Galaxy filament Lambda-CDM model Dark energy · Dark matter Dark fluid · Dark flow Timeline of cosmological theories Future of an expanding universe Observational cosmology 2dF · SDSS COBE · BOOMERanG · WMAP · Planck v d e The Universe is commonly defined as the totality of everything that exists, including all matter and energy, the planets, stars, galaxies, and the contents of intergalactic space. Definitions and usage vary and similar terms include the cosmos, the world and nature. Scientific observation of earlier stages in the development of the Universe, which can be seen at great distances, suggests that the Universe has been governed by the same physical laws and constants throughout most of its extent and history. There are various multiverse theories, in which physicists have suggested that our universe is one among many universes that likewise exist. Cite error: There are tags on this page, but the references will not show without a {{Reflist}} template or a tag; see the help page.
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