The HD 191939 Exoplanet System is Well-Aligned and Flat
Jack Lubin, Erik A. Petigura, Judah Van Zandt, Corey Beard, Fei Dai,, Samuel Halverson, Rae Holcomb, Andrew W. Howard, Howard Isaacson, Jacob Luhn,, Paul Robertson, Ryan A. Rubenzahl, Gudmundur Stefansson, Joshua N. Winn, Max, Brodheim, William Deich, Grant M. Hill

TL;DR
This study reveals that the HD 191939 exoplanet system is dynamically cold, flat, and well-aligned, with detailed measurements of the spin-orbit angle and orbital parameters of its planets, indicating a formation from a well-aligned protoplanetary disk.
Contribution
First measurement of the spin-orbit angle for HD 191939 b, and new constraints on the orbits of distant planets, demonstrating the system's overall coplanarity and flatness.
Findings
HD 191939 b's orbit is well-aligned with the star.
The distant super-Jupiter planet f has a mass of 2.88 M_J and a 2898-day orbit.
The inner planets are nearly coplanar with mutual inclinations less than 12 degrees.
Abstract
We report the sky-projected spin-orbit angle for HD 191939 b, the innermost planet in a 6 planet system, using Keck/KPF to detect the Rossiter-McLaughlin (RM) effect. Planet b is a sub-Neptune with radius 3.4 0.8 R and mass 10.0 0.7 M with an RM amplitude 1 ms. We find the planet is consistent with a well-aligned orbit, measuring 3.7 5.0 degrees. Additionally, we place new constraints on the mass and period of the distant super-Jupiter, planet f, finding it to be 2.88 0.26 on a 2898 152 day orbit. With these new orbital parameters, we perform a dynamical analysis of the system and constrain the mutual inclination of the non-transiting planet e to be smaller than 12 degrees relative to the plane shared by the inner three transiting planets. Additionally, the further planet f is inclined off this…
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Taxonomy
TopicsAstronomy and Astrophysical Research · Stellar, planetary, and galactic studies · Adaptive optics and wavefront sensing
