(For the Mirror.)
It has been computed, that all the celestial orbs perceived by the unassisted eye (which on a clear night never exceed 1,000,) do not form the 80,000 part of those which may be descried by the help of a telescope, through which they appear prodigiously increased in number; seventy stars have been counted in the constellation of the pleiades, and no fewer than 2,000 in that of Orion.
The galaxy, or via lactea, (milky way,) is a remarkable appearance in the heavens, being a broad ray of whitish colour surrounding the whole celestial concave, whose light proceeds from vast clusters of stars, discoverable only by the telescope. Mr. Brydone, in his journey to the top of Mount Etna, found the phenomenon make a most glorious appearance, "like a pure flame that shot across the heavens."
Dr. Herschel made many observations on this portion of the heavens, using a Newtonian reflector of twenty feet focal length, and an aperture of eighteen inches. With this powerful telescope he completely resolved the whitish appearance into stars, which the telescopes he had formerly used had not light enough to do. In the most vacant place to be met with in that neighbourhood, he found sixty-three stars; other six fields, or apparent spaces in the heavens, which he could see at once through his telescope, averaged seventy-nine stars in each field: thus he found that by allowing 15 min. of a deg. for the diameter of his field of view, a belt of 15 deg. long, and 2 deg. broad, which he had often seen pass before his telescope in an hour's time could not contain less than 50,000 stars, large enough to be distinctly numbered, besides which he suspected twice as many more, which could be seen only now and then by faint glimpses, for want of sufficient light. In the most crowded part of that region he informs us, he has had fields of view which contained no less than 588 stars, and these were continued for many minutes, so that in one quarter of an hour's time there passed no less than 116,000 stars. He also intimates the probability of the sun being placed in this great stratum, though perhaps not in the very centre of its thickness.
From the appearance of the galaxy it seems to encompass the whole heavens, as it certainly must if the sun be within the same. From succeeding observations made by Dr. Herschel, he gathers that the milky way is a most extensive stratum of stars of various sizes, and our sun evidently one of the heavenly bodies belonging to it. In viewing and gauging this shining zone in almost every direction, he found the number of stars composing it, by the account of those gauges constantly increase and decrease in proportion to its apparent brightness to the naked eye.
The nebulæ, or small whitish specks, discoverable by telescopes in various parts of the heavens are owing to the same cause. Former astronomers could only reckon 103, but Herschel counts upwards of 1,250. He has also discovered a species of them, which he calls planetary nebulæ, on account of their brightness, and shining with a well defined disk.
The sun enters Virgo on the 23rd at 11h. 42m. evening.
Mercury comes to his inferior conjunction on the 13th at 1-1/4h. morning, becomes stationary on the 22nd, and is at his greatest elongation on the 31st, when he passes his ascending node; he may be seen early on that morning rising at 3-1/2h.
Venus is in conjunction with Mars on the 21st at 3h. afternoon; she rises on the 1st at 2h. 38m., and on the 31st at 4h. 10m. morning.
Jupiter still continues a conspicuous object in the western part of the heavens, setting on the 1st at 9h. 43m., and on the 31st at 8h. None of the eclipses of his satellites are visible during the month in consequence of his being so near the sun.