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2,565 bytes added ,  03:12, May 4, 2007
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No credible, unbiased scientist would claim that "proves" billions of years old, and no citation was given for it.  That's a liberal opinion and should be stated as such, if stated at all.  There are many reasons why that falls short of a "proof".--[[User:Aschlafly|Aschlafly]] 22:58, 3 May 2007 (EDT)
 
No credible, unbiased scientist would claim that "proves" billions of years old, and no citation was given for it.  That's a liberal opinion and should be stated as such, if stated at all.  There are many reasons why that falls short of a "proof".--[[User:Aschlafly|Aschlafly]] 22:58, 3 May 2007 (EDT)
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The line about 'proving' the universe to be billions of years old can be left out without omitting the section on recent research, which is well supported by evidence. To remove this while only leaving in the Young Earth Creationist stuff and then locking the article to prevent editing is risible. Here is the excised material, from which I have removed the disputed last sentence. Please unlock the article so that this can be reinserted. It does your project no favors at all to ignore scientific research in favor of YEC theories. At least you can present both and let the reader decide.--[[User:Britinme|Britinme]] 23:12, 3 May 2007 (EDT)
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==Recent research
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Astronomers have searched for ways to find out accurately how old a [[star]] is. A new technique called gyrochronology, which works this out based on the star’s rate of rotation, has just been announced and will be published in the Astrophysical Journal. <ref> http://www.astronomy.com/asy/default.aspx?c=a&id=5479</ref> Knowing the age of the host star of a [[planetary system]] helps astronomers understand how planetary systems change over time.
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The research shows that the rotation period of a star changes steadily and predictably in line with its age and color. Thus, by measuring two of these attributes you can determine the third. The star’s color is a visible sign of its [[mass]] or surface temperature. The age of the [[[Sun]] is believed by astronomers to be 4.6 billion years <ref> http://cosmos.phy.tufts.edu/~zirbel/ast21/handouts/Energy-of-Sun-better.PDF </ref> and can be used to calibrate the gyrochronology of most other stars.
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There are other methods of working out a star’s age, but they have much larger uncertainties than gyrochronology. Unlike some other methods, gyrochronology also works well for stars not found in star clusters (‘field’ stars). It is used to calculate the age of stars that burn their hydrogen fuel at a predictable and steady rate; it does not work so well for younger stars, although the researchers hope to do future work to extend the method to these.
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The forthcoming [[NASA]] Kepler Mission will yield more information about the rotation period of other stars, as this is information gleaned while searching for the transit of new planets orbiting across their disks. Once researchers have more precise ages for stars, other problems of chronometry can be solved and a better study made of the way astronomical phenomena change through time, using the stars themselves as clocks. --[[User:Britinme|Britinme]] 23:12, 3 May 2007 (EDT)
    
==Facts==
 
==Facts==
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