(See description below)
Neptune is the eighth planet from the Sun and the
fourth largest (by diameter). Neptune is smaller in diameter but
larger in mass than Uranus. After the discovery of Uranus, it was
noticed that its orbit was not as it should be in accordance with
Newton's laws. It was therefore predicted that another more
distant planet must be perturbing Uranus' orbit. Neptune was
first observed by Galle and d'Arrest on 1846 Sept 23 very near to
the locations independently predicted by Adams and Le Verrier
from calculations based on the observed positions of Jupiter,
Saturn and Uranus. An international dispute arose between the
English and French (though not, apparently between Adams and Le
Verrier personally) over priority and the right to name the new
planet; they are now jointly credited with Neptune's discovery.
Subsequent observations have shown that the orbits calculated by
Adams and Le Verrier diverge from Neptune's actual orbit fairly
quickly. Had the search for the planet taken place a few years
earlier or later it would not have been found anywhere near the
Neptune has been visited by only one spacecraft, Voyager 2 on Aug 25 1989. Almost everything we know about Neptune comes from this encounter.
Because Pluto's orbit is so eccentric, it sometimes crosses the orbit of Neptune. Since 1979 Neptune has actually been the most distant planet from the Sun; Pluto will again be the most distant in 1999.
Neptune's composition is probably similar to Uranus': various "ices" and rock with about 15% hydrogen and a little helium. Like Uranus, but unlike Jupiter and Saturn, it may not have a distinct internal layering but rather to be more or less uniform in composition. But there is most likely a small core (about the mass of the Earth) of rocky material. Its atmosphere is mostly hydrogen and helium with a small amount of methane.
Neptune's blue colour is the result of absorption of red light by methane in the atmosphere. Like a typical gas planet, Neptune has rapid winds confined to bands of latitude and large storms or vortices. Neptune's winds are the fastest in the solar system, reaching 2000 km/hour. Like Jupiter and Saturn, Neptune has an internal heat source -- it radiates more than twice as much energy as it receives from the Sun.
At the time of the Voyager encounter, Neptune's most prominent feature was the Great Dark Spot (left) in the southern hemisphere. It was about half the size as Jupiter's Great Red Spot (about the same diameter as Earth). Neptune's winds blew the Great Dark Spot westward at 300 metres/second (700 mph). Voyager 2 also saw a smaller dark spot in the southern hemisphere and a small irregular white cloud that zips around Neptune every 16 hours or so now known as "The Scooter" (right). It may be a plume rising from lower in the atmosphere but its true nature remains a mystery. However, HST observations of Neptune in 1994 show that the Great Dark Spot has disappeared! It has either simply dissipated or is currently being masked by other aspects of the atmosphere. A few months later HST discovered a new dark spot in Neptune's northern hemisphere. This indicates that Neptune's atmosphere changes rapidly, perhaps due to slight changes in the temperature differences between the tops and bottoms of the clouds.
|Neptune also has rings. Earth-based observations showed only faint arcs instead of complete rings, but Voyager 2's images showed them to be complete rings with bright clumps. One of the rings appears to have a curious twisted structure (right). Like Uranus and Jupiter, Neptune's rings are very dark but their composition is unknown. Neptune's rings have been given names: the outermost is Adams (which contains three prominent arcs now named Liberty, Equality and Fraternity), next is an unnamed ring co-orbital with Galatea, then Leverrier (whose outer extensions are called Lassell and Arago), and finally the faint but broad Galle.|
Neptune's magnetic field is, like Uranus', oddly
oriented and probably generated by motions of conductive material
(probably water) in its middle layers.