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NkówáCOSMOS 3D dark matter map.jpg
English: This three-dimensional map offers a first look at the web-like large-scale distribution of dark matter, an invisible form of matter that accounts for most of the Universe's imaginary mass.
The map reveals a loose network of dark matter filaments, gradually collapsing under the relentless pull of gravity, and growing clumpier over time.
The three axes of the box correspond to sky position (in right ascension and declination), and distance from the Earth increasing from left to right (as measured by cosmological redshift). Note how the clumping of the dark matter becomes more pronounced, moving right to left across the volume map, from the early Universe to the more recent Universe.
The distribution of mass in the Hubble Space Telescope COSMOS survey, determined from measurements of weak gravitational lensing. The field of view covers about nine times the size of the full moon, and the third dimension stretches from redshift z=0 to z=1. The figure shows one isosurface of the gravitational potential.
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The copyright holder of this file, NASA/ESA/Richard Massey, allows anyone to use it for any purpose, provided that the copyright holder is properly attributed. Redistribution, derivative work, commercial use, and all other use is permitted.
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NASA/ESA/Richard Massey
Attribution
Public domainPublic domainfalsefalse
This file is in the public domain because it was created by NASA and ESA. NASA Hubble material (and ESA Hubble material prior to 2009) is copyright-free and may be freely used as in the public domain without fee, on the condition that only NASA, STScI, and/or ESA is credited as the source of the material. This license does not apply if ESA material created after 2008 or source material from other organizations is in use.
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2007-12-05 01:32:08 | RichardMassey | 119722 | 1280×973 | The distribution of mass in the Hubble Space Telescope COSMOS survey, determined from measurements of weak gravitational lensing. The field of view covers about nine times the size of the full moon, and the third dimension stretches from redshift z=0 to z
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This three-dimensional map offers a first look at the web-like large-scale distribution of dark matter, an invisible form of matter that accounts for most of the Universe's mass. The map reveals a loose network of dark matter filaments, gradually collapsing under the relentless pull of gravity, and growing clumpier over time. The three axes of the box correspond to sky position (in right ascension and declination), and distance from the Earth increasing from left to right (as measured by cosmological redshift). Note how the clumping of the dark matter becomes more pronounced, moving right to left across the volume map, from the early Universe to the more recent Universe.