( i76o^) 
duced to little or no breadth, in comparifon to what it 
had been towards the Suns Center, and fo clofe to the 
Limb of the Diskc, that 1 could only perceive a fmall 
ftreak of the Suns Light between it and the Limb of the 
SunsBody^ at o a Clocfe I could juft perceive it, but 
grown extremely. flenden 
The firft Pvcvolution T faw the Spot half \v\ the Circum- 
ference of the Sun's Limb at 2 a Clock iOn Sunday^ May 
thesgd: And the fecond Revolution I Juft perceived it 
with the 18 foot GUfs, at half an hour after two a Clock 
on SaUirday the 19th day of ]J?/>;e. ' / 
Obfcrvations of the Solar Spots fccn in June 
and July J 1703. 
Jvut.uhe2)th Sipidaj/y Jmte the 27th, about fix a Clock in the 
\_,/ Evening I 'obferved feveral Spots in the £un's 
Diske^) but had not the Conveniency to ufe my longefl: 
Tellefcope, becaufe of fome Trees that were in my way 
to Weftward, fo that I made no Obfervation till the 
Tuefday following, 
Jumthei<)th. Tnefday, Jme iVit 29th, About 7 in the Morning I count- 
ed 16 Remarkable Spots in the Suns Body, and near his 
Center they appeared as in the Figure, through the 18 
foot Glafs 5 then I took my ftven Foot Tellefcope and 
Frame, and obferved that>the foremoft Center of fix 
that looke4 op t tie Paper as one fpot, wasdifkafnt from 
the Sun s A nteriour Limb S i feconds of Tiaie, aad the laft 
Clufter 87. . . ' - r : 
This day the foremoft Spot was diftant from the fol- 
lowing Lirab^ according to the Path of the Spot, juft 5-5- 
feconds of Time. The Suns Diameter was always 156 
feconds ia the Tranfit, and the Spot was 12^ : So that 
that the Spots path was ip feconds fhorter than the 
Sun s Diameter. 
Wed^ef' . 
