Insight Astronomy Photographer of the Year 2015 Shortlist

Solar Prominence. Searing hot loops of plasma radiate from the edge of our local star – the sun – in a phenomenon known as a solar prominence. Emanating from the sun’s outer shell, from which light is emitted, prominences extend to the corona, which is the aura of the plasma surrounding it. A typical prominence covers over thousands of kilometres, with the largest ever recorded estimated to be over 800,000 kilometres, equalling roughly the radius of the sun itself. (Photo by Gary Palmer)
Insight Astronomy Photographer of the Year 2015 Shortlist
   
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