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A resonant sextuplet of sub-Neptunes transiting the bright star HD 110067 - Nature

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A resonant sextuplet of sub-Neptunes transiting the bright star HD 110067 - Nature

Planets with radii between that of the Earth and Neptune (hereafter referred to as 'sub-Neptunes') are found in close-in orbits around more than half of all Sun-like stars1,2. However, their composition, formation and evolution remain poorly understood3. The study of multiplanetary systems offers an opportunity to investigate the outcomes of planet formation and evolution while controlling for initial conditions and environment.

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A resonant sextuplet of sub-Neptunes transiting the bright star HD 110067 - Nature

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A resonant sextuplet of sub-Neptunes transiting the bright star HD 110067 - Nature

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