The Beginning was deduced froni many Obfervations made soon aster it. TheMoon’s Diameter appear’d then not to be morethan aboutao / ; though bytheObservations of her Diameter made tarne days betöre and after, it was judged tobc 31 / . 30". But the Extremities of the Horns, on which depended the Ex-actnels of that Determination, appear’d a little Blunted.

Phases

Time.

Phases.

Time.

Lefs that)

* Digiti. Digitz Digits

3 Digits

4 Digitsy Digits

6 Digits

7 Digits7i Digits

h. ' "z 2.9 30

2. 37 42z 40 zyz. 48 34z y4 30

3 3 00

3 iz 40

3 zz 18

3 ;8 -+-

7 Digits

6 Digitsy Digits

3 Digitsz Digitsof fere'

h. ' "

3 yi zo

4 2. zy

4 10 yo4 2.4 3 1

4 29 544 41 00

5 -

*At the Collegeof Lewis theGreat ; bj R'.P. Fontenay.lb.f. 7 i 7 -

6. The Beginning was at z h . 54/. 30". The End at 5 h . 9'. 9The Great- Aix;6yM.nesi of the Eclipsi; 8^ Digits. Gautier. ih.

j. 718.

Phases.

Time.

By FixtStars.

By theSun.

i Digit

8 »Digits

1 Digits

h. ' "

2. 45 3

3 53 52

4 59 20

h. ' "

2 50 3

3 y8 yz

5 4 20

7 -

<At Lyons;K. P. PaulHoste, lb.

b

At 3K zö'. 14s 1 . (bythe Stars ) The Diameter of the Sun and Motm 30h58". but at 4ii.zo^. 34". The Diameter of the Sun 30'. 58". of the M00»,3 c/.y' 7 .

Phases.

Times.

h. ' "z 40 00

3 zy 00

3 40 00

4 iy 00

523°

8 .

utt the Buy deRoses; bj M.Chassclles. lb,t- 7 l 9<

The Greatnefs of the Eclipse about 4 of the Sun’s Diameter, at which timeVenus might be scen without Pain. 9. The