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TOI-4495: A Pair of Aligned, Near-resonant Sub-Neptunes That Likely Experienced Overstable Migration

  • Authors: Mu-Tian Wang, 王 牧天, Fei Dai, 戴 飞, Hui-Gen Liu, 刘 慧根, Kento Masuda, Andrew W. Howard, Samuel Halverson, Howard Isaacson, Elina Y. Zhang, Max Goldberg, Huan-Yu Teng, Ryan A. Rubenzahl, Benjamin Fulton, Erik A. Petigura, Steven Giacalone, Luke Handley, David W. Latham, Allyson Bieryla, Ashley Baker, Jerry Edelstein, Steven R. Gibson, Kodi Rider, Arpita Roy, Chris Smith, Josh Walawender, David Rapetti, Jon M. Jenkins, Joshua N. Winn

Mu-Tian Wang et al 2026 The Astronomical Journal 171 .

  • Provider: AAS Journals

Caption: Figure 8.

Eccentricities, ∣Z∣, as a function of the innermost period Pin of TOI-4495 (square) and 43 pairs of Kepler near-resonant planets (circles) from S. Hadden & Y. Lithwick (2017). Anticipating different tidal dissipation rates on terrestrial (Rp < 1.7 R⊕) and gaseous (Rp > 1.7 R⊕) planets, we mark them in red and blue, respectively. ∣Z∣ consistent with zero are shown as open circles.

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