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A wide-orbit giant planet in the high-mass b Centauri binary system - Nature

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A wide-orbit giant planet in the high-mass b Centauri binary system - Nature

Planet formation occurs around a wide range of stellar masses and stellar system architectures1. An improved understanding of the formation process can be achieved by studying it across the full parameter space, particularly towards the extremes. Earlier studies of planets in close-in orbits around high-mass stars have revealed an increase in giant planet frequency with increasing stellar mass2 until a turnover point at 1.9 solar masses (M⊙), above which the frequency rapidly decreases3.

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A wide-orbit giant planet in the high-mass b Centauri binary system - Nature

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A wide-orbit giant planet in the high-mass b Centauri binary system - Nature

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