The KPF-SLOPE Survey - Small, Compact Multi-Planet Systems Appear Spin-Orbit Aligned
Luke B. Handley, Andrew W. Howard, Fei Dai, Ryan A. Rubenzahl, Steven Giacalone, Howard Isaacson, J. M. Joel Ong, Theron W. Carmichael, Yaguang Li, Jack Lubin, Pranav H. Premnath, Claire J. Rogers, Pranav Nagarajan, Gregory J. Gilbert, Benjamin Fulton, Steven R. Gibson

TL;DR
This paper introduces the SLOPE survey using the KPF spectrograph to measure stellar obliquities of small planets, finding that planets in compact multi-planet systems are generally spin-orbit aligned.
Contribution
The paper presents four new obliquity measurements of small planets and demonstrates their alignment in compact multi-planet systems, advancing understanding of planetary system dynamics.
Findings
All four measured planets are consistent with spin-orbit alignment.
Planets in compact multi-planet systems tend to be aligned with the stellar equator.
The statistical analysis shows a 6 sigma confidence in alignment for these systems.
Abstract
The angle between stellar spin axes and planetary orbits -- stellar obliquity -- probes the dynamics of planetary migration and evolution. The obliquities of giant planets have been extensively studied because they are the most easily measured. Smaller planets, while more difficult to measure, have the advantage of better reflecting the dynamics of planetary systems because they trigger negligible back-reactions onto the host star. This paper introduces a new observational campaign called the Small, Low-mass Oblique Planets Experiment (SLOPE) survey with the Keck Planet Finder (KPF) spectrograph, and presents four new obliquity measurements. The SLOPE survey focuses on planets smaller than Saturn across a variety of system architectures. The sky-projected obliquities of the four planets measured -- TOI-1386b, TOI-480b, TOI-4596b, and TOI-1823b -- are all consistent with spin-orbit…
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