[ 23 ] 
Times 
Longitudes 
Latitudes 
h 
/ 
a 
0 
1 
n 
0 
/ 
a 
2 I 
4 6 
if 
3 ° 
21 
0 E 
6 2 
3 ° 
34 N 
21 
*8 
39 
42 
53 
30 
60 
53 
O 
22 
l 3 
39 
5 * 
3 2 
40 
*8 
8 
20 
22 
28 
39 
68 
58 
0 
54 
41 
40 
This eclipfe, therefore, at Sardes, or any-where 
elfe that we can well fuppofe this battle to have been 
fought, could not have been great enough to turn 
day into night ; and therefore doth not anfwer Hero- 
dotus’s defcription. 
Archbifhop Ufher rejects both thefe eclipfes, as 
inconfift ent with his chronology ; and fuppofes that 
intended to have been A. M. 41 13. An. Nab. 147. 
before Chrift 601. Olymp. xliv . 4. Sunday July 20. 
3 h 2 f'. before noon, digits eclipfed 9. But this like- 
wife is greatly defective as to quantity. 
But tho’ this is infufficient for the purpofe, yet 
there was one two years before this, or the year 
before Chrift 603, that will be found by good ta- 
bles intirely fatisfadtory. Petavius, indeed, makes the 
digits eclipfed only 7.2 o'; but, according to Dr. 
Halley’s tables, the apparent time of the true con- 
junction was at Greenwich, May 17^ 20 h 42' 19". 
The place of the luminaries i f . 19 0 12k and the 
moon’s latitude north 25' 17", 
J ft! 
Semidiameter of the fun I f 49 
Semidiameter of the moon 16 4> 
Semidiameter of the penumbra 34 
Semidiameter of the earth's difk 60 yo 
Beginning 
