Astronomical transit
A transit is the astronomical event that occurs when a non-luminous body subtending a smaller angular diameter passes between an observer and another body which, though more distant, subtends a larger angular diameter.
The term is most frequently used to describe the motion of a planet beween a terrestrial observer and the Sun. This can happen only with inferior planets. To a pedant, an annular eclipse is a transit of the Moon.
In recent years the discovery of extra solar planets has excited interest in the possibility of detecting their transits across their own stellar primaries. HD 209458b is the first such transiting planet to be discovered.
Transits of Venus with respect to Earth are rare, they currently happen in pairs 8 years apart which repeat only after more than a century. The last transit of Venus was in 1882; the next three will occur on June 8, 2004, followed by June 6, 2012 and December 11, 2117. In the 18th century, the transit pair of 1761 and 1769 was used to determine the value of the astronomical unit.
Transits of Mercury with respect to Earth, being closer to the Sun, are more frequent, about thirteen per century. The last ones were on November 15, 1999, and May 7, 2003, the next ones will be on November 8, 2006, May 9, 2016 and November 11, 2019.
Referenced By
1769 in science | 2004 | 2004 AD | As of 2004 | As of January 2004 | HD 209458b | Mercury/Planet | Mercury (Planet) | Osiris (planet | Osiris (planet) | Planet Mercury | Vulcan (planet)
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