An Oblique Belt on Jupiter

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Scientific paper

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Scientific paper

OWING in the main part to the swift axial rotation of the planet Jupiter, it is usual to find the dark belts, which constitute the principal configuration of his visible surface, lying both parallel to one another and to the planet's equator. An instance of obliquity of one of the bands relatively to the others is rare, and a most definite and striking example of the kind was recorded in the northern hemisphere in 1860. A recent phenomenon akin to this was observed in the spring months of the present year. Although in this case the band was a faint one, yet the marked trend which it exhibited called: for special notice, and the more important facts relating to it might he briefly recorded here.

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