10. But leaving the stars, as well erring as fixed, see what Aristarchus proves and demonstrates in his treatise of magnitudes and distances; that the distance of the sun is above eighteen times and under twenty times greater than that of the moon from us. And yet they who place the moon lowest say that her distance from us contains six and fifty of the earth’s semidiameters, that is, that she is six and fifty times as far from us as we are from the centre of the earth; which is forty thousand stadia, according to those that make their computation moderately. Therefore the sun is above forty millions and three hundred thousand stadia distant from the moon; so far is she from the sun by reason of her gravity, and so near does she approach to the earth. So that if substances are to be distinguished by places, the portion and region of the earth challenges to itself the moon, which, by reason of neighborhood and proximity, has a right to be reputed and reckoned amongst the terrestrial natures and bodies. Nor shall we, in my opinion, do amiss if, having given so vast an interval and distance to these bodies which are said to be above, we leave also to those which are below some space and room to turn them in, such as is that between the earth and the moon. For neither is he who calls only the utmost superficies of the heaven _above_ and all the rest _beneath_ moderate or tolerable; nor is he to be endured who confines _beneath_ only to the earth, or rather to its centre; seeing the vast greatness of the world may afford means for the assigning farther to this lower part some such space as is necessary for motion. Now against him who holds that whatever is above the earth is immediately high and sublime, there is presently another opposition to encounter and contradict it, that whatever is beneath the sphere of the fixed stars ought to be called low and inferior.