But that, which he judgeth most remarkable, is, that he found by his Calculation, that the said least distance should be on the 29. of December, when the Comet was opposite to the Sun; which he does not know whether it may not serve to decide the grand Question concerning the Motion of the Earth.

He taketh further notice, that the Tayl of the Comet was to turn Westward, with a point to the North, until the 29. of December, at which time it was to be opposite to the Sun, and that then the said Tayl was to look directly North; but that, after that time, the Tayl was to turn Eastward, and continue to do so, until it disappear; and that it shall draw a little towards the North, until the 8. or 10. of February, at which time the Tayl is to be parallel to the Æquator, as if the Comet be yet seen for some time after, the Tayl shall go a little lower towards the South, but grow smaller.

He finds by his Hypothesis, that on the 2. of December, which is the first observation, that he hath heard of, this Star was to be about 7. times more remote from the Earth, than when it was in its Perigeum; and that it will be again in an equall remoteness from the Earth, on the 27. of January, so that he is of opinion, that in case this Comet have not been seen before the 2. of December, it will not be seen any more after the 27. of January.

He wishes above all things, that it might be very exactly observed, at what Angle the way of the Comet cuts the Æquator, and, most of all, the Ecliptick, that so it may be seen, whether

there hath not been some Parallaxe in the Circle of his Motion; as also, that some observations could be had of its greatest descent beneath the Tropick of Capricorn in the more Southern parts, where he saith it would have been without Refractions; Moreover of the Time, when it hath been in Quadrat with the Sun about the 20 of December; and that also very exact Observation might be made of the time of its being again in Quadrat with the Sun, which, according to him, was to be January 16.

He wishes also, that some in Madagascar may have observed this Star; Seeing that it began to appear over the middle of that Island, and passed twice over their heads; he judgeth, that they have seen it before us. And he wisheth lastly, that there were some intelligent person in Guiana to observe it there, seeing that within a few daies, according to his reckoning, it will pass over their Heads, and will not remove from thence but 8 or 10 degrees Northward, where he saith, it will disappear; thinking it improbable, that it can still appear, after the Sun shall have passed it.

This Account beareth date of the 2. January, new stile, 1665. and the Author thereof addeth this Note, That, seeing it could not be printed nor distributed so soon as he desired, he hath had the opportunity to verifie it by some Observations, from which he affirms he hath found no sensible difference; or, if there be, that it proceeds only from thence, that the Stars have advanced, since his Globe was made. He concludeth, that if this continue, and the first Observations do likewise agree, or that the differences do arrive within the Times ghessed by him, that he hopes, he shall determine both the Distance and the Magnitude of this Comet; and that perhaps one may be enabled to decide the Question of the Motion of the Earth. In the interim, he assureth, that he hath not changed the least number in his Calculations, and that Monsieur Huygens, and several French Gentlemen, to whom he saith, he hath given them long since, can bear him witness that he hath done so; as also many other friends of his, who saw upon his Globe, several daies before, the way of the Comet from day to day.

Thus for the Parisian Account of the Comet, which is here inserted at large, that the intelligent and curious in England may

compare their Observations therewith, either to verifie these Prædictions, or to shew wherein they differ; which is (as was also hinted above) the design of this Philosophical Prophet in dispersing his Conceptions, who declareth himself ready, in case he be mistaken in his reckoning, to learn another Hypothesis, to explicate these admirable appearances by.