A close-up of the star RIK 113, seen here surrounded by a cloud of gas and dust called a protoplanetary disc. These discs are a common feature around young stars, containing all the building blocks needed to make a new planet. Over time, these dusty discs will fragment and condense under the influence of gravity, forming larger objects like protoplanets. These planetary embryos carve out gaps in the dust around them, forming the intricate, ring-like structures that we can see in this disc. Location of a possible new planet marked with the white circle.
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