of a new Variable Star . \ 
06 L 6. At 6% h. and 7I h. lefs than J'and x, and a little lefs 
than $ Lyras ; between the fifth and fourth magnitude. 
Oft. 7. At 6| h. between the fourth and third magnitude; 
a little brighter . than 0, and nearly equal to J Herculis ; much 
brighter than J", k, and £ Lyras ; I obferved it till 12% h, when 
it was certainly increafed. 
At 7I h. Mr. E. Pigott thought it brighter than J and 9 
Herculis. 
Ode. 8. At 8 h. nearly equal to 7 Lyras ; on account of the 
intervening clouds, I could not perceive which was larged: ; 
third magnitude. 
06 L 9. At 7 h, rather lefs than y Lyras. 
Oft. 10. At 7 h. ii| h. and 12L nearly equal to 7, if 
not rather lefs. 
Oft. 11. At 8 h. 10 h. and 12 b. rather lefs than y; at 
12 h. if any difference, lefs than it was lad night. 
061 . 15. At 8 h.— nearly equal to, 9 though rather lefs 
than, y Lyras. 
061 16. At 6 1 h. and 9I h. little lefs than 7, if not equal 
to it. 
At 1 1 h. rather larger than 7, but the weather was foggy. 
Mr. E. Pigott agrees with me in both obfervations. 
061 . 17. At 6 1 h. and 7 h. fo me what lefs than 7 Lyras. 
061 . 1 8. At 6| h. between the fourth and fifth magnitude;, 
brighter than x and and rather brighter than f Lyras ; good 
obfervation. 
At 9 1 h. I thought it was decreafed, being equal to f and 
rather brighter than k Lyras. Mr. E, Pigott alfo thought it 
was decreafing. 
06 L 19. At 6| h. it was rather lefs than £ and x, and 
brighter than § Ly rse. 
' f 
At 
