Celestial hemisphere:  Northern  ·  Constellation: Camelopardalis (Cam)  ·  Contains:  NGC 1502
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Kemble's Cascade, Charles Pevsner
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Kemble's Cascade

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Kemble's Cascade, Charles Pevsner
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Kemble's Cascade

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Description

Something unusual:  A prominent deep sky object discovered with binoculars, in 1980.  Well, not “object” in the traditional sense of a galaxy, nebula, or cluster, and not exactly "discovered" either.  In 1980, the Canadian observer Lucian Kemble noticed this very pretty apparent tumbling of prominent stars across the sky after observing them through 7x35 binoculars.  He sent remarks about the asterism to Walter Scott Houston, who published them in Sky and Telescope magazine in December 1980.  Since then this succession of stars has been informally known as Kemble’s Cascade.  Two other asterisms are also named for Kemble:  Kemble 2,  and Kemble’s Kite.  (I must say that "Kemble 2" does not take any prizes for imaginative naming.)

Although the definition of an asterism is a “prominent” pattern of stars, in fact the stars in Kemble’s cascade are quite faint; they’re just much brighter than the other stars around.  The Cascade lies in the northern constellation Camelopardalis (the Giraffe), and spans 2.5° degrees of the night sky, about five times the width of the full moon.  The bright star in the center is HIP 18505; but again, “bright” is a relative term, since its magnitude is only +4.9.  At the foot of the cascade is a beautiful open cluster NGC 1502, consisting of about 45 stars.

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Kemble's Cascade, Charles Pevsner