COS SOME ACCOUNT OF THE 



Multiply into one another, the correction of the 

 node and the adjuttment of the latitude, and add the 

 producl: to the latitude of the moon, as taken out of 

 the table, to give the latitude correct ; which is 

 northern if the argument of latitude be in the firft 

 half of the zodiac, and vtcj? I'erfa. 



III. Tables of Saturn. 



1 — 6. Contain the mean longitudes and motions of 

 Saturn, of his apogee and node, for the fame periods 

 as the correfpondlng tables of the Sun and Moon. 



7 . Fir It. equation. Argument SaturrCs mean ano- 

 maly ; if in the fint fix iigns, fubtraction, and vict 

 I'crja. 



8. Equation of the node. Argument, the argu- 

 ment of latitude, found by fubtracting the longitude 

 of the node, from that of Saturn once equated ; addi- 

 tive in the ririt and fourth quarters, iubtractive in the 

 iecond and third. 



(). Saturn s iecond equation, or reduction of his 

 orbit to the ecliptic. Argument, the corrected argu- 

 ment of latitude or difference between Saturn s longi- 

 tude once equated and the equated longitude of the 

 rtode. This equation to be added to, or fubtracled 

 from, the planet's longitude once equated, (or his 

 place in his orbit,) in the fame cafes as indicated in 

 the correiponding table of the moon. 



10. Table of Saturn. i inclination. Argument, the 

 argument of latitude. 



11. Table of Saturn s diftance. Argument, his 

 mean anomaly correcTed by the iecond equation. 



IV. Tabues of J it it kr, correspond with thofe of 

 'Saturn, excepting that there is no equation of the 

 node, lb that they are only ten in number. 



V. 



