hundred and fifty millions of years, supposing that our rate of travelling was about three times that of our earth in its orbit. Now, as the velocity is assumed to be the same in both cases, the ratio between the distance (already so tremendous) of Bessel's 61 _Cygni_, and that of Lord Rosse's farthest frontier, is as forty- one thousand to two hundred and fifty millions. This is a simple rule- of-three problem for a child. And the answer to it will, perhaps, convey the simplest expression of the superhuman power lodged in the new telescope:--as is the ratio of forty-one thousand to two hundred and fifty million, so is the ratio of our own distance from the sun multiplied by six hundred and seventy thousand, to the outermost limit of Lord Rosse's sidereal vision.] Another class, and a frequent one, of equivocal phenomena, phenomena that are reconcilable indifferently with either of two assumptions, though less plausibly reconciled with the one than with the other, concerns the position of stars that seem connected with each other by systematic relations, and which yet _may_ lie in very different depths of space, being brought into seeming connection only by the human eye. There have been, and there are, cases where two stars dissemble an interconnection which they really _have_, and other cases where they simulate an interconnection which they have not. All these cases of simulation and dissimulation torment the astronomer by multiplying his perplexities, and deepening the difficulty of escaping them. He cannot get at the truth: in many cases, magnitude and distance are in collusion with each other to deceive him: motion subjective is in collusion with motion objective; duplex systems are in collusion with fraudulent stars, having no real partnership whatever, but mimicking such a partnership by means of the limitations or errors affecting the human eye, where it can apply no other sense to aid or to correct itself. So that the business of astronomy, in these days, is no sinecure, as the reader perceives. And by another evidence, it is continually becoming less of a sinecure. Formerly, one or two men,-- Tycho, suppose, or, in a later age, Cassini and Horrox, and Bradley, had observatories: one man, suppose, observed the stars for all Christendom; and the rest of Europe observed _him_. But now, up and down Europe, from the deep blue of Italian skies to the cold frosty atmospheres of St. Petersburg and Glasgow, the stars are conscious of being watched everywhere; and if all astronomers do not publish their observations, all use them in their speculations. New and brilliantly appointed observatories are rising in every latitude, or risen; and none, by the way, of these new-born observatories, is more interesting from the circumstances of its position, or more _picturesque_ to a higher organ than the eye--viz., to the human heart--than the New Observatory raised by the university of Glasgow.[Footnote: It has been