Shape of The Universe

The shape of the universe is a matter of debate in physical cosmology over the local and global geometry of the universe which considers both curvature and topology, though, strictly speaking, it goes beyond both. In practice, more formally, the debate seeks a 3-manifold that corresponds to the spatial section (in comoving coordinates) of the 4-dimensional space-time of the universe.

The recent Wilkinson Microwave Anisotropy Probe (WMAP) measurements have led NASA to state, "We now know that the universe is flat with only a 0.5% margin of error." Within the Friedmann–Lemaître–Robertson–Walker (FLRW) model, the presently most popular shape of the Universe found to fit observational data according to cosmologists is the infinite flat model, while other FLRW models that fit the data include the Poincaré dodecahedral space and the Picard horn.

Read more about Shape Of The Universe:  Introduction, Local Geometry (spatial Curvature), Global Geometry

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    his fear of the word “veil”;
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    —Joáo Cabral De Melo Neto (b. 1920)

    In the multitude of middle-aged men who go about their vocations in a daily course determined for them much in the same way as the tie of their cravats, there is always a good number who once meant to shape their own deeds and alter the world a little.
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    To the virtuous man, the universe is the only sanctum sanctorum, and the penetralia of the temple are the broad noon of his existence.
    Henry David Thoreau (1817–1862)