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{{#invoke:Hatnote|hatnote}}{{#invoke:Pp-move-indef|main}}{{#invoke:Protection banner|main}} {{ safesubst:#invoke:Unsubst||$N=Use British English |date=__DATE__ |$B= }} {{ safesubst:#invoke:Unsubst||$N=Use dmy dates |date=__DATE__ |$B= }} {{#invoke:Infobox|infobox}}

Neptune is the eighth and farthest planet from the Sun in the Solar System. It is the fourth-largest planet by diameter and the third-largest by mass. Among the giant planets in the Solar System, Neptune is the most dense. Neptune is 17 times the mass of Earth and is slightly more massive than its near-twin Uranus, which is 15 times the mass of Earth, and not as dense as Neptune.<ref group=lower-alpha name="mass2">Neptune is denser and physically smaller than Uranus because Neptune's greater mass gravitationally compresses the atmosphere more.</ref> Neptune orbits the Sun at an average distance of {{safesubst:#invoke:convert|convert}}. Named after the Roman god of the sea, its astronomical symbol is ♆, a stylised version of the god Neptune's trident.

Neptune is not visible to the unaided eye and is the only planet found by mathematical prediction rather than by empirical observation. Unexpected changes in the orbit of Uranus led Alexis Bouvard to deduce that its orbit was subject to gravitational perturbation by an unknown planet. Neptune was subsequently observed with a telescope on 23 September 1846<ref name="Hamilton"/> by Johann Galle within a degree of the position predicted by Urbain Le Verrier. Its largest moon, Triton, was discovered shortly thereafter, though none of the planet's remaining 14 moons were located telescopically until the 20th century. The planet's distance from Earth gives it a very small apparent size, making it challenging to study with Earth-based telescopes. Neptune was visited by Voyager 2, when it flew by the planet on 25 August 1989.<ref name="NYT-20141018-KC">{{#invoke:citation/CS1|citation |CitationClass=news }}</ref> The advent of Hubble Space Telescope and large ground-based telescopes with adaptive optics has allowed for more-detailed observations.

Neptune is similar in composition to Uranus, and both have compositions that differ from those of the larger gas giants, Jupiter and Saturn. Neptune's atmosphere, like Jupiter's and Saturn's, is composed primarily of hydrogen and helium, along with traces of hydrocarbons and possibly nitrogen; it contains a higher proportion of "ices" such as water, ammonia, and methane. Scientists sometimes categorise Uranus and Neptune as "ice giants" to emphasise this distinction.<ref name="Lunine 1993"/> The interior of Neptune, like that of Uranus, is primarily composed of ices and rock.<ref name="Podolak Weizman et al. 1995"/> Traces of methane in the outermost regions in part account for the planet's blue appearance.<ref name=bluecolour> {{#invoke:citation/CS1|citation |CitationClass=web }}</ref>

In contrast to the hazy, relatively featureless atmosphere of Uranus, Neptune's atmosphere has active and visible weather patterns. For example, at the time of the 1989 Voyager 2 flyby, the planet's southern hemisphere had a Great Dark Spot comparable to the Great Red Spot on Jupiter. These weather patterns are driven by the strongest sustained winds of any planet in the Solar System, with recorded wind speeds as high as {{safesubst:#invoke:convert|convert}}.<ref name="Suomi1991"> {{#invoke:Citation/CS1|citation |CitationClass=journal }}</ref> Because of its great distance from the Sun, Neptune's outer atmosphere is one of the coldest places in the Solar System, with temperatures at its cloud tops approaching {{safesubst:#invoke:convert|convert}}. Temperatures at the planet's centre are approximately {{safesubst:#invoke:convert|convert}}.<ref name=hubbard/><ref name="nettelmann"/> Neptune has a faint and fragmented ring system (labelled "arcs"), which may have been detected during the 1960s but was indisputably confirmed only in 1989 by Voyager 2.<ref name=ring1/>


Neptune sections
Intro   History    Composition and structure    Planetary rings    Climate    Orbit and rotation    Formation and migration    Moons    Observation    Exploration    See also    Notes    References    Bibliography    Further reading    External links   

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