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Spin–Orbit Alignment of Two Neptune-size Planets Younger Than 500 Myr: TOI-560 b and TOI-5082 b

  • Authors: Elina Y. Zhang, Fei Dai, Andrew W. Howard, Samuel P. Halverson, Howard Isaacson, Ryan A. Rubenzahl, Huan-Yu Teng, Xian-Yu Wang, Songhu Wang, Daniel Hey, Daniel Huber, Benjamin J. Fulton, Jack Lubin, Luke B. Handley, Steven Giacalone, Erik A. Petigura, Lauren M. Weiss, Aaron Householder, Casey Y. Lam, Judah Van Zandt, Steve R. Gibson, Kodi Rider, Arpita Roy, Ashley Baker, Jerry Edelstein, Christopher L. Smith, Josh Walawender, Joshua N. Winn

Elina Y. Zhang et al 2026 The Astronomical Journal 172 .

  • Provider: AAS Journals

Caption: Figure 2.

Joint RM and transit fit for TOI-5082 b, following the plotting conventions of Figure 1. The KPF observations were obtained on UTC 2024 November 26, and the best-fitting RM model corresponds to a sky-projected obliquity of ﹩{\lambda }_{{\rm{b}}}=19{^\circ }_{-13^\circ }^{+17^\circ }﹩.

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