3^^ Longitude of Tale-Collegei 



Hourly mo. fr. ^un 27' 06.15"= 1626.15" Log. A.C.6.r888S94 

 One hour, . - ^ 3600 Log. 3.556302^ 



Lon. of moon from sun, - 2195.26 Log. 3.3414860 



Time from beginn. ") h. m. s. 



to conjunction, J 1 20 59.9=4859.9 Log. 3.6866279 



Time of begining, 44 12.7 



Time of conj. at Y.C. 2 05 12.6 



For the Parallaxes, '^c. at the enJ^ 



h. m. s. 

 Apparent time of end, 5 51 56.5 



Assumed differ, of Ion. 4 51 50 



Apparent time at Greenwich, 8 43 46.8 

 Sun's Right-ascen. in time, 11 38 02 

 Sun past meridian, 3 51 56.8 



*Cor. for the sun's advance, 4- 3.4 



R. Ascen. of mid heaven 15 30 02.2 

 Do. in degrees, 232o 30- 33" 



Dist, of merid. from cap. 37 29 27 



h. m. s, 

 Appa. time of end, 8 43 4G'8 



* Note. This correction, "vC^hich depends on the' 

 difference in the equation of time, on two fucceflive 

 days, is generally omitted, in the rules which are giv- 

 en, for finding the right afcenfion of midheaven ; prob- 

 ably becaufe it is of fmall account. But, in ftrid pro- 

 priety, it ©ught to be includedv In the prefent inftailc^, 

 it will make a difference, of more than a minute, in 

 the longitude of the nonagefimal. The equation of 

 time is 21 feconds greater, on the 1 8th of Sept, than- 

 on the 1 7thi The fun therefore, in twenty four hours, 

 not only makes a complete revolution ;- but, in addi-^ 

 tion to this, falls to the weft of the meridian, fuch a 

 diflance, as correfponds to 21 feconds of time. A pro- 

 portional part of this, fhould be allowed, for the time 

 between 12 o'clock, and the end of the eclipfe. 



