Earth - Neptune Size Comparison

• Neptune is the eighth planet from the sun and the fourth largest (by diameter). It is smaller in diameter but larger in mass than Uranus. In Roman mythology, Neptune (Greek: Poseidon) was the god of the sea.


• 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. Galle and d'Arrest first observed Neptune on Sept. 23, 1846, 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. Adams and Le Verrier 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 predicted location.


• 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 percent hydrogen and a little helium. Like Uranus, but unlike Jupiter and Saturn, it may not have a distinct internal layering but have a more or less uniform 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 color 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 2,000 km/hour (1,250 miles/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 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 meters/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". 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.


• 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 coorbital 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.


• Neptune can be seen with binoculars (if you know exactly where to look), but a large telescope is needed to see anything other than a tiny disk.

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