570 



European Scientific Intelligence. 



[Dec. 



f To the nearest minute, 



Planets, 

 viz, 



Vesta, 

 Juno, 

 Pallas, 

 C eres. 



f Heliocentric Longitude, 



Latitude 



Geocentric AR. in time, to the tenth of a minute, 



declination to the nearest minute, 



| Radius vector, to four places, 

 "j Long, distance from the earth, to four places, 

 j Mean time of transit, to the tenth of a minute, 



Geocentric AR. in time, to two places, 



Declination, to one place, 



For evert/ fourth 

 yday at noon. 



For one month before 

 >and after opposition at 

 midnight. 



Jupiter's 

 Satellites^ 



rFor every day. 



Radius vector, to five places, 



{-Long, distance from the Earth, to five places, - 



The co-efficients ABCD, for every day, at midnight. 



" .Jin mea'n and siderial time, to one place 



Eclipses on a- c i 



I diagrams for shewing the place at that time. 



Contact with the planet, in siderial time, n 



j Contact of shadows with the planet, in do. J T ° tke near€st minute ' 



(_ Configurations. 



f From the Sun and the nine principal 



Lunar Fixed Stars, and from Venus, Mars, 



Distances | Jupiter and Saturn, for every third hour. 



. With the proportional logarithm of the differences, annexed. 



Apparent obliquity of the ecliptic, to two places, 



Parallax of the Sun, to two places, 



Aberration of the Sun, to two places, 



Equation of equinoctial points, in Longitude, to two places, 



. ■ ■ ' in R A to two places, 



Mean longitude of the moon's node, to the tenth of a minute, _ 



r Solar, with the line of the moon's umbra, diagrams, &fc. 

 Eclipses | Lunai . t 



Predicted occultations (visible at Greenwich) of planets and fixed stars to the sixth 

 magnitude inclusive, in mean and siderial time, to the nearest minute; with the an- 

 gle from the vertex, and also from tke most northern point of the m 0.0 it's disc. 



Elements for predicting such occultations of the planets and fixed stars to the 

 fifth magnitude inclusive, as may be visible in any habitable part of the globe, with 

 the limits of latitude annexed. 



The apparent places of the stars on the days of occultation to be given in both 

 cases. 



Apparent places of the fixed stars (100 in number) for their time of transit : a 

 and 8 Ursae minoris for every day, the remainder for every tenth day, with differ- 

 ences annexed: 



Mean places of the same at the beginning of the year in a separate list. 

 A list of moon-culminating stars, continued within four days of new moon : the 

 apparent AR. of the stars to two places, and the mean declination to the nearest 

 minute ; also the 



f AR. in time, of her bright limb, to two places, 

 J Variation in ditto for one hour of longitude, 

 •\ Siderial time of semidiameter passing meridian, 

 j to two places, 

 ^-Declination, to nearest minute, for upper culmination 



Moon's 



For upper and 

 * lower culmination. 



