A TESS Disappearing Act: The Vanishing Transits of TOI-2535 b

Abstract Planetary transits require a fortuitous alignment between a planet’s orbit and our line of sight, but dynamical interactions can render this geometric coincidence only temporary. We report the discovery of the hot Jupiter TOI-2535b, the first confirmed planet orbiting a single star whose transits have been directly observed to disappear. Over 7 yr of photometry from NASA’s Transiting Exoplanet Survey Satellite (TESS), the planet’s transit chord traversed and eventually moved off the stellar disk entirely, with an impact parameter changing at the rate of b ̇ = 0.16 yr − 1 . The transit midtimes also show significant departures of ±6 hr from a linear ephemeris. Joint modeling of the transit timing and duration variations (TTVs and TDVs) and NEID radial-velocity data indicates the presence of a nearby, mutually inclined ( i mut ≳ 5 ∘ ) planetary perturber, with the TDV being primarily due to precession of the planets’ orbital planes. Our dynamical modeling reveals that the perturber is likely of Saturn-mass or greater and in a mean-motion resonance with TOI-2535b, making this an unusual system that contains two short-period giant planets. The TDVs measured for TOI-2535b represent one of the most extreme examples of planet–planet interactions driving orbital evolution on human timescales.

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Journal
The Astrophysical Journal Letters
Published
2026-11-09
DOI
https://doi.org/10.3847/2041-8213/aeb4a4
Primary Topic
Stellar, planetary, and galactic studies
Type
article
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article

A TESS Disappearing Act: The Vanishing Transits of TOI-2535 b

Eric P Girardin, M. Gillon, F. Murgas, Ε. Πάλλη et al.
The Astrophysical Journal Letters
Stellar, planetary, and galactic studies
article

A TESS Disappearing Act: The Vanishing Transits of TOI-2535 b

Eric P Girardin, M. Gillon, F. Murgas, Ε. Πάλλη, David W. Latham, Emmanuël Jehin, Rafael Brahm, Phil Evans, Howard M. Relles, Abderahmane Soubkiou, Samuel W. Yee, Karen A. Collins, Adam Popowicz, Erik A. Petigura, Richard P. Schwarz, Khalid Barkaoui, Victoria DiTomasso, Andrés Jordán, Carl Ziegler, David Watanabe, Avi Shporer, Trifon Trifonov, Francis P. Wilkin, Don J. Radford, Thomas K. Henning, Mourad Ghachoui, Allyson Bieryla, Gregor Srdoč
article en

Abstract

Abstract Planetary transits require a fortuitous alignment between a planet’s orbit and our line of sight, but dynamical interactions can render this geometric coincidence only temporary. We report the discovery of the hot Jupiter TOI-2535b, the first confirmed planet orbiting a single star whose transits have been directly observed to disappear. Over 7 yr of photometry from NASA’s Transiting Exoplanet Survey Satellite (TESS), the planet’s transit chord traversed and eventually moved off the stellar disk entirely, with an impact parameter changing at the rate of b ̇ = 0.16 yr − 1 . The transit midtimes also show significant departures of ±6 hr from a linear ephemeris. Joint modeling of the transit timing and duration variations (TTVs and TDVs) and NEID radial-velocity data indicates the presence of a nearby, mutually inclined ( i mut ≳ 5 ∘ ) planetary perturber, with the TDV being primarily due to precession of the planets’ orbital planes. Our dynamical modeling reveals that the perturber is likely of Saturn-mass or greater and in a mean-motion resonance with TOI-2535b, making this an unusual system that contains two short-period giant planets. The TDVs measured for TOI-2535b represent one of the most extreme examples of planet–planet interactions driving orbital evolution on human timescales.

The Astrophysical Journal LettersVol. 1011(2)
Silesian University of Technology (PL), Cadi Ayyad University (MA), University of Liège (BE), Universidad de La Laguna (ES), University of California, Los Angeles (US), Union College (US), Stephen F. Austin State University (US), Adolfo Ibáñez University (CL), Heidelberg University (DE), Max Planck Institute for Astronomy (DE), Center for Astrophysics Harvard & Smithsonian (US), Instituto de Astrofísica de Canarias (ES), Sofia University "St. Kliment Ohridski" (BG), Massachusetts Institute of Technology (US), University of Chile (CL)
Stellar, planetary, and galactic studies
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