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Slow Rotation for the Super-puff Planet Kepler-51d

  • Authors: Caleb Lammers, Joshua N. Winn

Caleb Lammers and Joshua N. Winn 2024 The Astrophysical Journal Letters 977 .

  • Provider: AAS Journals

Caption: Figure 1.

The projected oblateness parameters (top; to scale) and a comparison between spherical-planet and oblate-planet models for Kepler-51d (bottom). The models differ at ingress and egress (by ~200 ppm for f⊥  =  0.2 and θ⊥  =  45∘) from that of a spherical planet with the same cross-sectional area and orbital parameters.

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