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hich had already fully entered upon the Sun's disc on the left, so that the limbs of the Sun and Venus precisely coincided, forming an angle of contact. Not doubting that this was really the shadow of the planet, I immediately applied myself sedulously to observe it. 'In the first place, with respect to the inclination, the line of the diameter of the circle being perpendicular to the horizon, although its plane was somewhat inclined on account of the Sun's altitude, I found that the shadow of Venus at the aforesaid hour--namely, fifteen minutes past three--had entered the Sun's disc about 62 deg. 30', certainly between 60 deg. and 65 deg., from the top towards the right. This was the appearance in the dark apartment; therefore, out of doors, beneath the open sky, according to the laws of optics, the contrary would be the case, and Venus would be below the centre of the Sun, distant 62 deg. 30' from the lower limbs or the nadir, as the Arabians term it. The inclination remained to all appearances the same until sunset, when the observation was concluded. 'In the second place, the distance between the centres of Venus and the Sun I found by three observations to be as follows:-- The Hour. | Distance of the Centres. | At 3.15 by the clock | 14' 24'' " 3.35 " | 13' 30'' " 3.45 " | 13' 0'' " 3.50 the apparent sunset. | The true setting being 3.45, and the apparent about 5 minutes later, the difference being caused by refraction. The clock therefore was sufficiently correct. 'In the third place I found after careful and repeated observation that the diameter of Venus, as her shadow was depicted on the paper, was larger indeed than the thirtieth part of the solar diameter, though not more so than the sixth, or at the utmost the fifth of such a part. Therefore let the diameter of the Sun be to the diameter of Venus as 30' to 1' 12''. Certainly her diameter never equalled 1' 30'', scarcely perhaps 1' 20'', and this was evident as well when the planet was near the Sun's limb as when far distant from it. [Illustration: VENUS ON THE SUN'S DISC.] 'This observation was made in an obscure village where I have long been in the habit of observing, about fifteen miles to the north of Liverpool, the latitude of which I believe to be 53 deg. 20', although by common maps it is stated at 54 deg. 12', theref
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