Neptune is the most remote of the distant group of large, hydrogenrich worlds collectively known as the ‘major planets’, the others being Jupiter (the nearest and largest), Saturn and Uranus. Neptune and Uranus together comprise a distinct subclass. While the planets Jupiter and Saturn are composed predominantly of hydrogen and helium, these elements account for less than 80% of the masses of Uranus and Neptune. The outer pair have significantly higher percentages of heavier elements such as carbon, nitrogen, oxygen and iron. These major differences between the inner and outer pairs of the giant planets indicate distinct differences in their formation and evolution, as well as in their present-day interiors, atmospheres and dynamics.
Despite its remoteness, Neptune exhibits some of the most active meteorology and global variability in the outer solar system (Plate 31). Numerous haze and cloud layers distributed throughout the visible atmosphere have been observed to vary on timescales...
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Baines, K.H. (1997). Neptune: Atmosphere . In: Encyclopedia of Planetary Science. Encyclopedia of Earth Science. Springer, Dordrecht. https://doi.org/10.1007/1-4020-4520-4_276
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