in giving the same result. Principles on which the investigation of the solar motion depends. Absolute velocity of the Sun's motion. Supposed revolution of the whole sidereal system round a common centre. Systematic parallax and aberration. Effect of the motion of Of clustering groups of stars. Globular clusters. Their stability dyna- mically possible. List of the most remarkable. Classification of nebulæ and clusters. Their distribution over the heavens. Irregular clusters. Resolvability of nebulæ. Theory of the formation of clus- ters by nebulous subsidence. Of elliptic nebulæ. That of Andro- meda. Annular and planetary nebulæ. Double nebulæ. Nebulous stars. Connection of nebula with double stars. Insulated nebulæ of forms not wholly irregular. Of amorphous nebula. Their law of distribution marks them as outliers of the galaxy. Nebula and nebulous group of Orion — of Argo—of Sagittarius-of Cygnus. The Magellanic clouds. Singular nebula in the greater of them. Variable nebulæ. The zodiacal light. Shooting stars. Speculations on the Natural units of time. Relation of the sidereal to the solar day affected by precession. Incommensurability of the day and year. Its incon- venience. How obviated. The Julian Calendar. Irregularities at its first introduction. Reformed by Augustus. Gregorian reformation. Solar and lunar cycles. Indiction. Julian period. Table of Chrono- logical eras. Rules for calculating the days elapsed between given Dates. Equinoctial time. Fixation of ancient dates by eclipses. Notes II. Synoptic Table of the Elements of the Planetary System III. Synoptic Table of the Elements of the Orbits of the Satellites, analogies, and the general prevalence of vulgar errors. first preparation, therefore, for the course he is about to commence, he must loosen his hold on all crude and hastily adopted notions, and must strengthen himself, by something of an effort and a resolve, for the unprejudiced admission of any conclusion which shall appear to be supported by careful observation and logical argument, even should it prove of a B in giving the same result. Principles on which the investigation of the solar motion depends. Absolute velocity of the Sun's motion. Supposed revolution of the whole sidereal system round a comme centre. Systematic parallax and aberration. Effect of the motion of Of clustering groups of stars. Globular clusters. Their stability dyna- mically possible. List of the most remarkable. Classification of nebulæ and clusters. Their distribution over the heavens. Irregular clusters. Resolvability of nebulæ. Theory of the formation of clus- ters by nebulous subsidence. Of elliptic nebulæ. That of Andro- I. Lists of Northern and Southern Stars, with their approximate OUTLINES OF ASTRONOM Y. (1.) INTRODUCTION. EVERY student who enters upon a scientific pursuit, especially if at a somewhat advanced period of life, will find not only that he has much to learn, but much also to unlearn. Familiar objects and events are far from presenting themselves to our senses in that aspect and with those connections under which science requires them to be viewed, and which constitute their rational explanation. There is, therefore, every reason to expect that those objects and relations which, taken together, constitute the subject he is about to enter upon will have been previously apprehended by him, at least imperfectly, because much has hitherto escaped his notice which is essential to its right understanding: and not only so, but too often also erroneously, owing to mistaken analogies, and the general prevalence of vulgar errors. first preparation, therefore, for the course he is about to commence, he must loosen his hold on all crude and hastily adopted notions, and must strengthen himself, by something of an effort and a resolve, for the unprejudiced admission of any conclusion which shall appear to be supported by careful observation and logical argument, even should it prove of a nature adverse to notions he may have previously formed for himself, or taken up, without examination, on the credit of B As a others. Such an effort is, in fact, a commencement of that intellectual discipline which forms one of the most important ends of all science. It is the first movement of approach towards that state of mental purity which alone can fit us for a full and steady perception of moral beauty as well as physical adaptation. It is the "euphrasy and rue" with which we must "purge our sight" before we can receive and contemplate as they are the lineaments of truth and nature. (2.) There is no science which, more than astronomy, stands in need of such a preparation, or draws more largely on that intellectual liberality which is ready to adopt whatever is demonstrated, or concede whatever is rendered highly probable, however new and uncommon the points of view may be in which objects the most familiar may thereby become placed. Almost all its conclusions stand in open and striking contradiction with those of superficial and vulgar observation, and with what appears to every one, until he has understood and weighed the proofs to the contrary, the most positive evidence of his senses. Thus, the earth on which he stands, and which has served for ages as the unshaken foundation of the firmest structures, either of art or nature, is divested by the astronomer of its attribute of fixity, and conceived by him as turning swiftly on its centre, and at the same time moving onwards through space with great rapidity. The sun and the moon, which appear to untaught eyes round bodies of no very considerable size, become enlarged in his imagination into vast globes, the one approaching in magnitude to the earth itself, the other immensely surpassing it. The planets, which appear only as stars somewhat brighter than the rest, are to him spacious, elaborate, and habitable worlds; several of them much greater and far more curiously furnished than the earth he inhabits, as there are also others less so; and the stars themselves, properly so called, which to ordinary apprehension present only lucid sparks or brilliant atoms, are to him suns of various and transcendent glory-effulgent centres of life and light to myriads of unseen worlds. So that when, after dilating his thoughts to comprehend the grandeur of those |