Neith (hypothetical moon)

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For the Egyptian goddess, see Neith.
Francesco Fontana’s drawing of the supposed satellite(s) of Venus. Woodcuts from Fontana’s work (1646). The fringes of light around Venus are produced by optical effects. Compare with later depictions of the Paramecium


Neith is a hypothetical natural satellite of Venus reportedly sighted by Giovanni Cassini in 1672 and by several other astronomers in following years. The first supposed sighting of this moon was in 1650. It was 'observed' up to 30 times by astronomers until 1770, when there were no new sightings and it was not found during the transit of Venus in 1761 and 1769.[1]

Discovery[edit]

In 1672, Giovanni Cassini found a small object close to Venus. He did not take great note of his observation, but when he saw it again in 1686, he made a formal announcement of a possible moon of Venus. The object was seen by many other astronomers over a large period of time: by James Short in 1740, by Andreas Mayer in 1759, by Joseph Louis Lagrange in 1761, another eighteen observations in 1761, including one in which a small spot was seen following Venus while the planet was in a transit across the Sun, eight observations in 1764, and by Christian Horrebow in 1768.

Summary of sightings[edit]

Year City Person Number of Sightings
1645 Naples Francesco Fontana 3
1646 Naples Francesco Fontana 1
1672 Paris Giovanni Domenico Cassini 1
1686 Paris Giovanni Domenico Cassini 1
1740 London John Short 1
1759 Greifswasld Andreas Mayer 1
1761 Marseilles Louis Lagrange 3
1761 Limoges Jacques Montaingne 4
1761 St. Neots unknown 1
1761 Greifswald Friedrich Artzt 1
1761 Krefeld Example 2
1761 Copenhagen Example 8
1764 Copenhagen Example 2
1764 Copenhagen Example 3
1764 Auxerre Montbarron 3
1768 Copenhagen Example 1


Observations[edit]

Many astronomers failed to find any moon during their observations of Venus, including William Herschel in 1768. Cassini originally observed Neith to be one-fourth the diameter of Venus. In 1761, Lagrange announced that Neith's orbital plane was perpendicular to the ecliptic. In 1766, the director of the Vienna Observatory speculated that the observations of the moon were optical illusions. He said: "the bright image of Venus was reflected in the eye and back into the telescope, creating a smaller secondary image." In 1777, J.H. Lambert estimated its orbital period as eleven days and three hours.

In 1884, Jean-Charles Houzeau, the former director of the Royal Observatory of Brussels suggested that the "moon" was actually a planet which orbited the Sun every 283 days. Such a planet would be in conjunction with Venus every 1080 days, which fit with the recorded observations. Houzeau was also the first to give the object the name Neith, after an Egyptian goddess.

The Belgian Academy of Sciences published a paper in 1887 which studied each reported sighting of Neith. Ultimately, they determined that most of the sightings could be explained by stars which had been in the vicinity of Venus, including Chi Orionis, M Tauri, 71 Orionis, Nu Geminorum and Theta Librae.

See also[edit]

References[edit]

  1. ^ Kragh, Helge (2008). "The Moon that Was not: The Saga of Venus' Spurious Satellite". Birkhäuser. ISBN 978-3-7643-8908-6. 

External links[edit]