40/48 It is about nine-tenths of a second. Hence this star is almost two hundred and thirty thousand times as far from us as the sun. With its companion, it revolves round their common centre of gravity in eighty-one years, and hence it would seem that their conjoint mass is less than that of the sun. Its parallax was first found by Bessel in 1838, and is about one-third of a second. The distance from us is, therefore, much more than five hundred thousand times that of the sun. |