Image:Age.png

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Description
English: A plot of the age of the universe as a function of some important cosmological parameters. The product of the age and the current Hubble parameter is a function of other cosmological parameters, describing the matter density, cosmological constant density, etc. Contours of this function are plotted as a function of the two most important parameters. The WMAP best-fit value (as of 2006) for these parameters is denoted by a box in the upper left, and the matter-only universe is denoted by an asterix in the lower right. This image was generated by user Wesino, and the relevant code can be found on Wesino's user page.
Source

Transferred from en.wikipedia; transfered to Commons by User:Jalo using CommonsHelper.

Date

2006-11-12 (original upload date)

Author

Original uploader was Wesino at en.wikipedia

Permission
( Reusing this image)

Released into the public domain (by the author).


License information

Public domain This image has been (or is hereby) released into the public domain by its author, Wesino at the wikipedia project. This applies worldwide.

In case this is not legally possible:
Wesino grants anyone the right to use this work for any purpose, without any conditions, unless such conditions are required by law.

Original upload log

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

  • 2006-11-12 12:45 Wesino 930×858×8 (64279 bytes) A plot of the age of the universe as a function of some important cosmological parameters. The product of the age and the current Hubble parameter is a function of other cosmological parameters, describing the matter density, cosmological constant densit

File history

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Date/Time Dimensions User Comment
current 12:49, 24 June 2008 930×858 (63 KB) File Upload Bot (Magnus Manske) ( {{BotMoveToCommons|en.wikipedia}} {{Information |Description={{en|A plot of the age of the universe as a function of some important cosmological parameters. The product of the age and the current Hubble parameter is a function of other cosmological para)

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