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CHAP. V.
Of the Comet that appeared in the year 1652.
ANno 1652. December the 9. by most (the 6, 7, and 8 by some) was the first appearance of a great Comet, or blazing Star, having a large Tail, which at some times and in some pla∣ces appeared bigger than at other times it seemed.
It continued visible about 23 days, therefore the effects must continue so many years from the time of its appearance, viz. till the year 1675. so that the influence thereof must be manifested, and also co-operate with the effects of our present Conjunction, according to the determination of the times thereof; and be∣cause it was of great Magnitude, even (in the simile of Mr. Boo∣ker) as the full Moon in her Apogaeon, or farthest distance from the Earth, or as Mr. Lilly and Mr. Wharton have it, about 14 or 15 inches diameter, and the Tail extended to 3 or 4 degrees North-east-ward, or opposite to the Sun; Hence the effects are of the greater concernment; For, Quo magis Stella eo efficacior est; By how much greater a Star is, the more powerful and efficacious: The times of its Appearance, its Longitude, Latitude, Diurnal motion, as it was observed by Mr. Rook sometime Reader of Astronomy at Gresham Colledge; and the declination by Mr. Wharton, is as by the following Table appears.
Where we must observe, that the 9th day was the first time of the observation thereof by Instrument, though it did appear two or three days before, nor could it be every night seen, so as to observe it, therefore there is no more set down than the observa∣tions were.
The nature of the Effects we come to know from the colour of the Comet, and the ruling Planets, &c.