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since 'Jupiter was last in Opposition to the Sun, is what he calls Num. II.in which the Inequality of the Earttis Motion is allowed sor in the Months,and that of Jupiters Orb by a Table of the Equatim of Num. II. amount-ing in all to z, Revolutions of the Satellite to Jupiter. This in the Tablesfollowing I have thought fit to leave out, Ihewing how to find it by the helpof the former Equation of N um. I. The Numbers are in effect the läme withM.Caffims, only Reduced to our Stile and Meridian, and the Form of themAbridged, and ’tis hoped Amended. -

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