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Hubble probes the core of galaxy NGC 247

NGC 247 is a relatively small spiral galaxy in the southern constellation of Cetus (The Whale), part of the Sculptor Group around 11 million light-years from us. NGC 247 displays one particularly unusual and mysterious feature — an apparent void in the usual swarm of stars and H II regions in the northern part of its disc that spans almost a third of the galaxy’s total length.

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Cosmic recycling in the Prawn Nebula

Dominating this image is the so-called Prawn Nebula, part of the gigantic nebula Gum 56, some 6,000 light-years away in Scorpius. For millions of years stars have been born out of the nebula’s gas, material which is later returned to the stellar nursery when the aging stars either expel their material gently into space, or eject it more dramatically in supernova explosions.