ShtSA uPpA slftc coast 0i 0aiiiOTnld, III lat. 27 degrees 30 minutes x. Ihcnce cugsillg northwarel!sy, minutes isioT-e It wlli enter the United States near the j. si- coFiief oif hioufsiatis,, and III. SIX minutes vi eeffess tic Mississippi. near st. francisville. Passing through the State of Mississippi, Alabama, and Georgia, in v minutes more it will ar- rive at point in Pendleton county, $. Carolina, in lat. 34 degrees 37 minutes \. longitude S2 degrees 2Sminutes ". where the sun will be centrally eclipsed on the meridian. Thence passing over North Carolina into Virginia, in I4 min utes it will cross James River, near Richmond; and continuing in nearly a direct line, in 5 minutes will leave the Jersey shore at Little Egg Harbour, passing q few miles east of Montauk Point; in 5 minutes 1t will leaYe tic eastern shore of Cape God at wellaeet, and in Q minutes will enter upon the southwestern extremity of Nova Scotia. Thence passing over the island of Newfoundland, and increasing in velo- city as 1t approaches the verge etf the earth, in l9 minutes more it will leave its disk in lat. 57 degrees N, long. 2S deg. 40 minutes ". at which point the sun will set centrally eclipsed at 4h. 30m. or 6h. 25m. Greenwich time.

 The eclipse will have been 2h. s3Ina. in crossing the earth's disk, and about one hour from its entrance to the time of it's leaving the United States.-A line drawn through the above points on map of North America, will pass through all those places where the eclipse is central. Two other lines on. each side of the first at the distance. of 58 miles, will include all places in the United State where 1t will be annuIar. lis Penanlbra will proceed and follow the centre, at the mean interval of one hour and thirty minutes, making on the central track the beginning and end of the eclipse. Lines drawn on a map of the United States, parallel to the cen trai track, at intervals on tho $. side of 200, IS5 and l75 miles, and on the north at intervals, of 225, 250, and 300 miles, will exhibit, nearly, the respect iFe points where the sun wifi be I. iD, and 3 digits eclipsed. By making proportions along the central path of the eclipse, of the intervals of Green wich time, and Protraeting the hour fines at right angles. the lime and phase Of the eclipse may be found for very nearly any place in the United States observing to reduce the Greenwich time 10 that of the place of observation.

 This eclipse will be visible oyer eve " part of the North American conti- nent and the West Indies, and will be seen as far south as the city of Quito in South America.