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In 1987 Astronomer R. Brent Tully of the University of Hawaii’s Institute of Astronomy identified what he called the [http://en.wikipedia.org/wiki/Pisces-Cetus_Supercluster_Complex Pisces-Cetus Supercluster Complex], a [[structure]] which he said was one billion [[light years]] long and 150 million light years across.[http://en.wikipedia.org/wiki/Large-scale_structure_of_the_cosmos]
In 1987 Astronomer R. Brent Tully of the University of Hawaii’s Institute of Astronomy identified what he called the [http://en.wikipedia.org/wiki/Pisces-Cetus_Supercluster_Complex Pisces-Cetus Supercluster Complex], a [[structure]] which he said was one billion [[light years]] long and 150 million light years across.[http://en.wikipedia.org/wiki/Large-scale_structure_of_the_cosmos]
==See also==
*'''''[[A Study of the Master Universe]]'''''
==Further reading==
==Further reading==
*Vicent J. Martínez, Jean-Luc Starck, Enn Saar, David L. Donoho, Simon Reynolds, Pablo de la Cruz, and Silvestre Paredes (nov 2005). "Morphology Of The Galaxy Distribution From Wavelet Denoising". The Astrophysical Journal 634: 744-755. doi:10.1086/497125. arΧiv:astro-ph/0508326. Retrieved 2009-12-22.
*Vicent J. Martínez, Jean-Luc Starck, Enn Saar, David L. Donoho, Simon Reynolds, Pablo de la Cruz, and Silvestre Paredes (nov 2005). "Morphology Of The Galaxy Distribution From Wavelet Denoising". The Astrophysical Journal 634: 744-755. doi:10.1086/497125. arΧiv:astro-ph/0508326. Retrieved 2009-12-22.
