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However, transits of Venus are very rare. Before 1761, the previous transit had been in 1639; after 1769, the next transit would be in 1874. The importance of the measurement led to an unprecedented international effort to obtain as many observations as possible from different points in the world – points as far apart from one another as ...
A transit of Venus takes place when Venus passes directly between the Sun and the Earth (or any other superior planet), becoming visible against (and hence obscuring a small portion of) the solar disk. During a transit, Venus is visible as a small black circle moving across the face of the Sun. Transits of Venus reoccur periodically.
Print/export Download as PDF; Printable version; In other projects ... Pages in category "Transit of Venus" The following 28 pages are in this category, out of 28 ...
Venus was 0.7205 au from the Sun on the day of transit, decidedly less than average. [9] Moving far backwards in time, more than 200,000 years ago Venus sometimes passed by at a distance from Earth of barely less than 38 million km, and will next do that after more than 400,000 years.
A Transit of Venus occurs when the planet Venus passes between the Sun and the Earth, as it happened in: Transit of Venus, 1639; Transit of Venus, 1761; Transit of Venus, 1769; Transit of Venus, 1874; Transit of Venus, 1882; Transit of Venus, 2004; Transit of Venus, 2012; Transit of Venus may also refer to:
The numbers and the Greek word appear immediately above the English translation instead of side by side, as is common in many interlinears. The Apostolic Bible Polyglot also contains The Lexical Concordance of the ABP, [ 2 ] The English Greek Index of the ABP, [ 3 ] and The Analytical Lexicon of the ABP. [ 4 ]
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Transits of Venus directly between the Earth and the Sun's visible disc are rare astronomical events. The first such transit to be predicted and observed was the 1639 transit of Venus, seen and recorded by English astronomers Jeremiah Horrocks and William Crabtree. [18]