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Lunar occultation of Venus

Astronomical phenomenon of Lunar Occultation of Venus From Wikipedia, the free encyclopedia

Lunar occultation of Venus
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The lunar occultation of Venus refers to a natural phenomenon in which the Moon passes in front of Venus, obstructing it from view on some regions of the Earth. Since the orbital planes of both the moon and Venus are tilted relative to the ecliptic, occultations only happen about twice a year rather than once a month. A computer search predicts that 101 lunar occultations occur in the date range of 1995–2045.[1]

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Probable lunar occultations of Venus, 2020 to 2060. These are calculated by a simple method that may include some near occultations. The blue points represent occultations closer to the moon's ascending node while the red are closer to the descending node. Note the series of five in 2054, which have been checked.

Occultations can occur at any value of the moon's argument of latitude, not just near its nodes, because Venus goes further north and south of the ecliptic than the moon does. In 2054 for example there are five occultations at intervals of just one month (January through May), and the first two are when Venus is more than 5.1° north of the ecliptic.[2]

Whether there is an occultation depends on whether the distance of the centre of the moon is greater or less than 8093 kilometres (the sum of the earth's polar radius and the moon's radius) away from the line connecting the centre of the earth to Venus. The angle between the lines from the centre of the earth to the centres of the moon and Venus will then be the arc sine of 8093 km divided by the distance to the moon. Since this distance can vary in the range of 356,400 to 406,700 kilometres, there will always be an occultation (of the centre of Venus) if the said angle is less than 1.14° and there will never be one if the angle is more than 1.30°. Venus itself can have an angular radius up to nearly 0.01°, which needs to be taken into account when determining whether all of Venus will be hidden. This is similar to considerations of gamma for solar eclipses.

For years up to 2025, a website giving easily observable occultations for the year is available.[3]

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