Conceptually, most cosmological distances are measured from here on Earth to the centre of distant galaxies.<br /><br />We use a combination of factors to determine these huge distances, including the brightness and redshift of a galaxy. These are measurements of that galaxys light, which would be an average of all the light emitted from it. Seeing as the mass that emitted that light was mostly concentrated in the centre of those galaxies (the middle is brighter than the edges), we can consider our measurements to be from here on Earth to the centre of those galaxies.<br /><br />Consider that the Earth is around 8 light minutes from the Sun and around 30,000 light years from the centre of our galaxy. If we are looking at a galaxy similar to our own that is 10,000,000,000 light years away the difference between the centre and the edge of that galaxy is a small fraction of the overall figure, and it is a lot harder to determine where a galaxy ends than it is to determine where its centre is. <div class="Discussion_UserSignature"> <p><font color="#ff0000">_______________________________________________<br /></font><font size="2"><em>SpeedFreek</em></font> </p> </div>