41:4.1

The mass of your sun is slightly greater than the estimate of your physicists, who have reckoned it as about two octillion (2 x 1027) tons. It now exists about halfway between the most dense and the most diffuse stars, having about one and one-half times the density of water. But your sun is neither a liquid nor a solid—it is gaseous—and this is true notwithstanding the difficulty of explaining how gaseous matter can attain this and even much greater densities.