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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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Originally uploaded at en.wikipedia as File:COSMOS 3D dark matter map.jpg by User:RichardMassey. (Transfered by User:Quibik.)
Also available at http://spacetelescope.org/images/heic0701b/

Isosuface data can be found at http://www.roe.ac.uk/~rm/cosmos/
Odé ákwụ́kwọ́ NASA/ESA/Richard Massey (California Institute of Technology)
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This file has been superseded by COSMOS 3D dark matter map.png. It is recommended to use the other file. Please note that deleting superseded images requires consent.

Reason to use the other file: "A PNG version of this file is now available."
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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

Public domain
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.

The material was created for NASA by Space Telescope Science Institute under Contract NAS5-26555, or for ESA by the Hubble European Space Agency Information Centre. Copyright statement at hubblesite.org or 2008 copyright statement at spacetelescope.org.

For material created by the European Space Agency on the spacetelescope.org site since 2009, use the {{ESA-Hubble}} tag.


Original upload log

The original description page was here. All following user names refer to en.wikipedia.

Upload date | User | Bytes | Dimensions | Comment

  • 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

Nkowapụta

Tinye nkọwa otu ahịrị ihe faịlụ a na-anochi anya ya.
Dark Matter

Ihe ndị egosiri na faịlụ a

depicts Bekee

image/jpeg

checksum Bekee

67e2328f591efa3351ddfa7924cf9475fb329321

data size Bekee

951,649 byte

2,146 pixel

width Bekee

2,823 pixel

Ịta nke usòrò

Bìri èhì/ogè k'ị hụ òtù ụ̀fa dị̀ m̀gbè ahụ̀.

Èhì/OgèMbọ-akaÓgólógó na asaáÒjìèmeNkwute
dị ùgbu â22:22, 30 Novemba 2011NvóÁká màkà otù ȯ dị nà 22:22, 30 Novemba 20112,823 × 2,146 (929 KB)QuibikFull-size image from http://spacetelescope.org/images/heic0701b/. Converted to 95% quality JPEG from TIFF.
22:12, 30 Novemba 2011NvóÁká màkà otù ȯ dị nà 22:12, 30 Novemba 20111,280 × 973 (117 KB)CommonsHelper2 Bot

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