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Page 2
Sir Edmond Halley of cometary fame was mapping the southern skies in St. Helena when he happened to observe a much more frequent Mercury transit. It dawned on him this kind of events could be put to good use to determine a long sought value, the Earth - Sun distance. Venus should be more useful than Mercury being farther out from the Sun, thus affording a more favorable geometry for the sake of accuracy. Tragically, he was well aware the upcoming 1761 and 1769 events were beyond his life span, yet laid the foundations for the experiment further perfected by Joseph-Nicolas Delisle.
Transits gone, German astronomer Johann Encke determined in 1824 after careful analysis of 1761 and 1769 timing data, the Earth - Sun distance to be 153,34 million km (95.28 million miles), 2.5% higher than the correct 149,59 million km. A movie shot before the invention of cinema The 17th Century observations unveiled problems that marred the otherwise excellent precision the method could provide for the Astronomical Unit determination. For one, precision rested on the accuracy of timing contacts between the Sun's limb and Venus limb - a fact that was found to be subject to individual response times (remember, it was then clockwork era) - and then there was atmospheric disturbances, Venus' atmospheric bright halo, and the so called "black drop" effect masking the contact point at the most critical instant.
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