crazyeddie- see my post of 10/08/04 07:49 PM. Clearly you want me to post more evidence, and I will do so.<br /><br />Meanwhile, you would do well to review the line of reasoning I already posted. <br /><br />For example, how far do the internal solar magnetic fields penetrate the sun? Do they extend through and beyond the solar core?<br /><br />Solar seismic activity also penetrates the core.<br /><br />Would you like me to post links and references as to the evidence, or would you prefer researching independently first?<br /><br />Hint: compare the stirring time of earth's ocean: 1,000 years.<br /><br />Then compare the mass of the solar gaseous 'ocean' layers. <br /><br />Also compare the speed of transmission of energy from core to surface - if I remember correctly it is about one million years.<br /><br />While there is much more energy available in the sun's layers than in earth's oceans, there is also a much larger mass. <br /><br />The temperature difference between core and outer layers is also similarly involved.<br /><br />I was simply giving a ballpark estimate on solar stirring time.<br /><br />To me it seems likely it is at least 1,000 times slower than the time it takes energy to travel from core to surface.<br /><br />Hence, the mixing time may be at least one billion years, likely 10 billion years, perhaps one trillion years.<br /><br />The standard model cannot be easily checked at this very slow mixing rate.<br /><br />By way of comparison, consider how difficult it was for astronomers to detect variations in the CMBR- so much so it was assumed by some to be smooth.<br />Astronomers are noting more and more how different stellar radiation and other properties can be.<br /><br />Therefore, it would be difficult to extrapolate a life span for our sun from an average from the so many different types of main sequence stars out there.