Redshift Surveys: the
Universe in 3 Dimensions

The Universe has 3 spatial dimensions and in order to understand its geometry we need distance information to supplement the angular information obtained from locating galaxies on the celestial sphere.
Las Campanas redshift survey (Source). The right ascension is given around the partial circles, and the figure corresponds to a superposition of 3 slices in declination (39-45 degrees). We are in the center, and the distance from the center is the recessional velocity, which is related to distance from us.

Redshifts and the Third Dimension

The standard way to obtain distances on larger scales is to use the Hubble law and the redshift measured from the Doppler effect on spectral lines. This is difficult, however, because to accumulate sufficient light to measure the redshift of distant objects accurately requires long observations.

Thus, deep space redshift surveys (that is, those out to very large distances) to date have been confined to limited regions, either by examining narrow slices of the celestial sphere, or by concentrating on a very small region of the celestial sphere but trying to observe objects as far away as possible in that region (pencil surveys).

Although such surveys are difficult and time-consuming, they have over the last decade or so begun to be available for limited portions of the sky and have begun to allow a full 3-dimensional picture of large-scale structure to be constructed. This information suggests structure on even larger scales than that of superclusters. The adjacent image shows one such redshift survey.

The 3D Structure of the Universe

From detailed studies of this sort the following picture begins to emerge from redshift surveys out to approximately 200 Mpc. Such observations place strong constraints on our later discussions of the origin of structure in the Universe, since any viable theory of such structure must explain why the Universe has this appearance.

Scientific American article: Mapping the Universe


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