B 5 06 58.06 58.16 +0.10 5 16 20.49 20.28 -0.21 5 23 57.67 57.71 +0.04 5 28 13.25 13.44 + 0.19 2 54 48.27 4 26 52.96 53.00+ 0.04 5 05 03.64 03.47-0.17 5 06 58.18 58.140.04 5 16 20.71 20.26-0.45 5 23 57.65 57.69 +0.04 5 25 46.89 47.11 +0.22 5 28 13.67 13.42 - 0.25 4 26 52.90 52.96 +0.06 4 51 56.67 5 05 03.53 03.43 -0.10 5 06 57.84 58.10+ 0.26 5 16 20.38 20.23 -0.15 5 23 57.59 57.66 +0.07 5 28 13.40 13.38 -0.02 5 46 38.87 38.84-0.03 5 54 20.25 6 13 26.13 26.05 -0.08 6 34 14.69 14.74 + 0.05 6 38 12.41 12.81+ 0.40 7 24 33.77 33.32 -0.45 7 31 04.01 03.82 7 00 51.16 51.15 -0.19 66 7 35 41.06 40.99 6 57 39.65 7 10 42.27 43.32 +0.95 7 24 33.32 33.29-0.03 8 38 26.81 26.87 +0.06 -0.22 66 - 0.22 - 0.64 12 25 41.04 40.61-0.43 12 46 11.69 11.71+0.02 11 45 34.09 33.45 7 31 03.14 03.24+0.10| 7 35 40.30 40.38+0.08 11 42 30.71 30.98 +0.27 11 45 33.12 33.44 +0.32 12 46 11.46 11.71 +0.25 12 48 41.14 41.20 +0.06 13 15 59.36 13 16 55.78 55.72 -0.06 17 07 29.29 29.43 +0.14 17 15 58.00 17 21 50.22 50.03 -0.19 17 50 12.06 11.94-0.12 18 04 22.03 21.92 -0.11 19 10 36.92 19 12 33.48 33.19 0.29 66 * B2 indicates the observation to have been made by G. P. Bond. B2 Mr. Bond communicated a third series of moon culminations, made at Dorchester. Mr. Bond remarked, that, although these observations had been made at Dorchester, yet the results might safely be reduced to the new Observatory in Cambridge, by means of the differences of latitude and longitude given with each series, without risk of sensible error; the points of observation |