Jupiter completes one slightly eccentric orbit around the [[Sun]] in 11.86 years, and returns to the same position in [[Earth]]'s night sky in roughly 399 years.<ref name=nasa2/><ref name=nelson/> Its mean distance from the Sun is about 5.2 AU--almost exactly the distance predicted by the [[Titius-Bode Law]] of planetary distances. Though Jupiter is the fifth ''planet'' from the Sun, it is actually the ''sixth'' object of a size requiring the assumption of a spheroidal shape. Hence ''n=6'' is the proper number to use in the Bode's Law formula.
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Jupiter completes one slightly eccentric orbit around the [[Sun]] in 11.86 years, and returns to the same position in [[Earth]]'s night sky in roughly 399 years.<ref name=nasa2/><ref name=nelson/> Its mean distance from the Sun is about 5.2 AU--almost exactly the distance predicted by the [[Titius-Bode law]] of planetary distances. Though Jupiter is the fifth ''planet'' from the Sun, it is actually the ''sixth'' object of a size requiring the assumption of a spheroidal shape. Hence ''n=6'' is the proper number to use in the Bode's Law formula.