Definition
In astronomy, a transit is the occurrence, as seen by an external observer, of a partial eclipse of a body (star, planet) by another body (star, planet) orbiting the first one. The transit refers to the entire duration of the phenomenon. Historically, the observations of the transit of Venus in front of the Sun as seen from Earth, and especially the ones in 1761 and 1769, have been the occasion to measure the Sun–Earth distance with a fair accuracy. The last transit of Venus across the Sun was in 2012.
The transit phenomenon presents a powerful method for detecting extrasolar planets. Thanks to the Kepler space telescope, this method has been able to detect close to 1,000 extrasolar planets. The transits of an extrasolar planet in front of its host star is also used to determine several of the planet’s parameters such as its radius, period, and eccentricity. It is also the most promising technique for characterizing exoplanets atmosphere.
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© 2014 Springer-Verlag Berlin Heidelberg
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Latham, D.W., Haghighipour, N. (2014). Transit. In: Amils, R., et al. Encyclopedia of Astrobiology. Springer, Berlin, Heidelberg. https://doi.org/10.1007/978-3-642-27833-4_1603-4
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DOI: https://doi.org/10.1007/978-3-642-27833-4_1603-4
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Publisher Name: Springer, Berlin, Heidelberg
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