CHAP. IX. Of the true Systeme of the Ʋniverse.
I. The C ••er∣nico▪Carte∣sian Hypo∣thesis ex∣plained. DES Cartes supposeth that Matter indefinitely extended, and by motion imprest upon it, di∣vided into various Particles, did run together into several Vortexes or Whirl-Pools, whirling about some certain Points with a most swift motion; that the more subtil matter gathered together about the * 1.1Center of these Vortices, constitutes the fixt Star; that the matter which is a degree bigger, makes the Heavens; and that the more solid Bodies (such as is the Earth and the rest of the Planets) hanging poisd in this fluid matter, comply with the motion of the Vortex about the fixt Star, and may over and above this, be whirld about their own Axis; as we often see that Bodies, carried in a fluid Stream, are turn'd round by a motion of their own, that is, proper to themselves, and not derived from the Stream wherein they are carried.
II. The first Heaven. Moreover Des Cartes divides all the Vortexes, that comp••se this World into two Heavens. In the first, he supposeth all the Matter of Heaven in which the Planets move, to run round continual∣ly in manner of a great Vortex, or mass of fluid Matter whirling round, in the Center whereof is the Sun, S, and that those Parts that are nearer to the Sun, move more swiftly, than those that are more remote, and that all the Planets (of whose number also the Earth T is,) have their course continually amidst the Parts of that Caelestial Matter.
III. The second Heaven. The second Heaven comprehends an immense number of other Vortexes, which surround this Vor∣tex or first Heaven A, B, C, which in their Cen∣ters have the several fixt Stars. And because we are uncertain at how great a distance the fixt Stars are from us, and cannot conceive them so remote as to contradict the Phaenomena, we will not con∣tent our selves with placing them above Saturn, but will take the liberty to conceive them much higher; seeing that it is apparent from the Coele∣stial motions, that they are so far distant from us, that Saturn compar'd to them, seems to be very near us. Des Cartes to illustrate the Truth the more about the motion of the Planets, and espe∣cially of the Comets, made no difficulty to assign an immense distance between Saturn and the fixt Stars.
IV. The di∣stance of the fixt Star•• from the Sun. Neither is this in the least contrary to Reason, forasmuch as we know that Mercury is above two hundred Diameters of the Earth distant from the Sun; Venus above Four hundred; Mars Nine hundred or a Thousand; Jupiter above Three thousand, and Saturn Five or Six thousand. And proportionably we may extend the Space between Saturn and the fixt Stars, to any distance how vast soever. For tho the Region of the fixt Stars, be commonly reputed the utmost Bounds of the World, yet its Figure cannot be certainly deter∣mined by us, seeing we can perceive nothing of its Internal nor External Superficies.
V. Saturn is the First of the Planets. The first of the Planets and nearest to the fix'd Stars is Saturn, who sometimes appears as if he had three Bodies, sometimes Long or Tall, some∣times Sphaerical, sometimes Oval, with Ears and Ear-rings. For tho' Saturn like the other Stars, be of a Round Figure, yet is he surrounded with a broad Circle or Ring; standing at an equal di∣stance from him; the proportion of the Semidia∣meter of the Planet, being to the distance of the Ring, as 3 to 5: but the entire Diameter of the Ring, to that of Saturn is about the proportion of 11 to 5. The Ring is thin, but broad, and if continued, would pass through the Center of Sa∣turn. This Planet being most remote from the Sun, the Center of this our World, and being moved in a large Vortex, is almost 30 years in finishing his Circuit in our Heaven ABC.
VI. Saturns three Satel∣lites. Three Satellites or Guards, are observed to move about him, the First whereof is distant from the Center of Saturn, one Diameter of the fore∣said Ring, and performs his Circuit about Saturn in the Space of 4 days, 12 hours and 27 minutes. He is seen through a Telescope of 35 Foot, in his furthest digression from Saturn, but is impercep∣tible when nearer to him. The Second is much more illustrious, and may be descried by any mo∣derate Telescope, and is distant from Saturn four Diameters of the said Ring, and whirls round him in the time of 16 days and 23 hours. The Third is distant from him 10 Diameters of the Ring, and performs his Circumvolution in the Space of about 80 days.
VII. The Second is Jupiter. The next to Saturn is Jupiter, who absolves his Course in almost 12 years. He hath four less Planets, as so many little Moons to be his Com∣panions, to which GALILAEUS gave the name of the Medicaean Stars, because he first discovered them in the Dominions of the Duke of Florence. Their special names are, the Jovial Saturn, Eu∣ropa, Ganymedes, Calisto; whereof the First or remotest wheels about Jupiter in 16 days; the Second in 7 Days; the Third in 85 hours, and the Fourth in 42 hours.
VIII. T•••• 〈◊〉〈◊〉 is Ma••••. The Third Planet Mars is carried about a in greater Vortex than the Earth, and in a less than Jupiter; and finisheth his Revolution in near two years. In the midst of this Planet CAMPA∣NELLA by the help of Prospectives discovered a Black Mountain, higher than the Mountains of the Moon: From whence, as likewise from the Spots, wherewith his Face is sprinkled, CASSINUS gathered, that Mars was whirld about his own Center in the Space of 24 hours and 49 minutes. There is also a round Ring somewhat resembling a Rainbow, but of a Redder Colour, which surrounds the Foot of that Mountain.