The Warm Neptune GJ 3470b has a Polar Orbit
Gudmundur Stefansson, Suvrath Mahadevan, Cristobal Petrovich, Joshua, N. Winn, Shubham Kanodia, Sarah C. Millholland, Marissa Maney, Caleb I., Ca\~nas, John Wisniewski, Paul Robertson, Joe P. Ninan, Eric B. Ford, Chad F., Bender, Cullen H. Blake, Heather Cegla

TL;DR
This study reveals that the warm Neptune GJ 3470b orbits its star on a polar trajectory, with implications for its formation, potential outer companions, and atmospheric characteristics, based on spectroscopic and radial velocity data.
Contribution
First measurement of GJ 3470b's polar orbit using NEID spectrometer and analysis of possible outer companion influence.
Findings
GJ 3470b has a true obliquity of about 95°, indicating a polar orbit.
Data suggest a long-term RV slope compatible with an outer companion.
Tidal heating likely inflates GJ 3470b's radius by 1.5-1.7 times.
Abstract
The warm Neptune GJ 3470b transits a nearby (pc) bright slowly rotating M1.5-dwarf star. Using spectroscopic observations during two transits with the newly commissioned NEID spectrometer on the WIYN 3.5m Telescope at Kitt Peak Observatory, we model the classical Rossiter-Mclaughlin effect yielding a sky-projected obliquity of and a km/s. Leveraging information about the rotation period and size of the host star, our analysis yields a true obliquity of , revealing that GJ 3470b is on a polar orbit. Using radial velocities from HIRES, HARPS and the Habitable-zone Planet Finder, we show that the data are compatible with a long-term RV slope of m/s/day over a baseline of 12.9 years. If the RV slope is due to acceleration from another companion in the system,…
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