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According to the prevailing scientific model of the Universe, known as the [[Big bang|Big Bang]], the Universe expanded from an extremely hot, dense phase called the [[Planck epoch]], in which all the matter and energy of the [[observable universe]] was concentrated. Since the Planck epoch, the Universe has been [[Cosmic expansion|expanding]] to its present form, possibly with a brief period (less than 10<sup>−32</sup> seconds) of [[cosmic inflation]]. Several independent experimental measurements support this theoretical [[Metric expansion of space|expansion]] and, more generally, the Big Bang theory. Recent observations indicate that this expansion is accelerating because of [[dark energy]], and that most of the matter in the Universe may be in a form which cannot be detected by present instruments, and so is not accounted for in the present models of the universe; this has been named [[dark matter]]. The imprecision of current observations has hindered predictions of the [[ultimate fate of the Universe]].
Current interpretations of [[observable universe|astronomical observations]] indicate that the [[age of the Universe]] is 13.75 ±0.17 [[1000000000 (number)|billion]] years,<ref name="marshallaugerhilbertblandford">S. H. Suyu, P. J. Marshall, M. W. Auger, S. Hilbert, R. D. Blandford, L. V. E. Koopmans, C. D. Fassnacht and T. Treu. [http://www.iop.org/EJ/abstract/0004-637X/711/1/201/ Dissecting the Gravitational Lens B1608+656. II. Precision Measurements of the Hubble Constant, Spatial Curvature, and the Dark Energy Equation of State.] The Astrophysical Journal, 2010; 711 (1): 201 DOI: 10.1088/0004-637X/711/1/201</ref> and that the diameter of the [[observable universe]] is at least 93 billion [[light year]]s, or [[Scientific Notation|8.80
==Etymology, synonyms and definitions==
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