redshift law
1Redshift (theory) — Redshift is a techno economic theory suggesting hypersegmentation of Information Technology (IT) markets based on whether individual computing needs are over or under served by Moore s Law, which predicts the doubling of computing transistors… …
2Redshift quantization — is the hypothesis that the redshifts of cosmologically distant objects (in particular galaxies) tend to cluster around multiples of some particular value. Since there is a correlation of distance and redshift as expressed in Hubble s Law,… …
3Redshift (disambiguation) — Redshift or red shift can refer to:cience* Redshift, the increase of wavelength of detected electromagnetic radiation with respect to the original wavelength of the emission. * Red shift, an informal term for a bathochromic shift * RedShift… …
4Redshift — This article is about the astronomical phenomenon. For other uses, see Redshift (disambiguation). Physical cosmology …
5Redshift survey — In astronomy, a redshift survey, or galaxy survey, is a survey of a section of the sky to measure the redshift of astronomical objects. Using Hubble s law, the redshift can be used to calculate the distance of an object from Earth. By combining… …
6Hubble's law — Physical cosmology Universe · Big Bang …
7Intrinsic redshift — is the hypothesis from various non standard cosmologies that a significant portion of the observed redshift of extragalactic objects (e.g. quasars and galaxies) may be caused by a phenomenon other than the traditionally accepted redshift… …
8Photometric redshift — A photometric redshift is an estimate for the distance of an astronomical object, such as a galaxy or quasar. The technique uses photometry (that is, the brightness of the object viewed through various standard filters, each of which lets through …
9Hubble's law — n. the law, formulated by Edwin Hubble, that the velocities of distant galaxies moving away from the earth are directly proportional to their distance from the earth: cf. REDSHIFT …
10Hubble law — noun states that the velocity at which a distant object is receding from the Earth (as measured by its redshift) is proportional to its distance; observational evidence for an expanding universe See Also: Hubble constant …
