Neptune-sized exoplanet found in retrograde orbit
AstronomyComments
To expand on that, the Rossiter-McLaughlin effect is likely how they measured the spin-orbit misalignment. It would be interesting to see the eccentricity data to confirm if the orbit is still circularizing.
We saw similar claims with WASP-17b years ago. Did the researchers account for the stellar obliquity of the host star in this case?
Why jump straight to a hidden giant? Could this just be a case of extreme tidal migration or a capture event from a passing star?
If the orbital inclination is near 180 degrees, wouldn't it be statistically improbable for simple tidal migration to flip the axis entirely? A massive perturber via the Kozai-Lidov mechanism seems more plausible here.
I wonder if this ties into the recent data on those salt clouds in the Pink Planet... could these orbital disruptions be more common in systems with specific chemical signatures?
The paper actually mentions the star's metallicity is unusually high. This often correlates with more massive disks, which increases the likelihood of the gravitational scattering they are proposing.