arXiv2026
Trans-Neptunian objects (TNOs) are among the most primitive remnants of the early Solar System, and constraining their sizes, shapes, albedos, and surface properties is essential for understanding their origin and evolution. Stellar occultations provide highly accurate size and shape measurements for TNOs, while photometry constrains their albedo and surface colours. (28978) Ixion is one of the largest TNOs and a prominent Plutino, making it a key target for comparative studies. We aim to constrain Ixion's projected size, shape, absolute magnitude, geometric albedo, and surface colours, and to search for evidence of an atmosphere or circum-object material. We analysed stellar occultation campaigns by Ixion conducted between 2020 and 2023 within the Lucky Star collaboration, comprising 51 observations from eight events, including 30 positive detections. Five multi-chord events enabled a global limb fit and an accurate reconstruction of Ixion's projected shape. The occultations reveal a slightly elongated limb well represented by a single projected ellipse, yielding an area-equivalent diameter of $D_{\mathrm{equiv}} = 696.78^{+10.75}_{-8.87}$ km and an apparent oblateness $ε' = 0.081^{+0.004}_{-0.010}$. Typical radial residuals of order $\sim$10 km indicate a largely stable shape across epochs, with modest epoch-dependent variations. Calibrated photometric data yield an absolute magnitude of $H_V = 3.845 \pm 0.006$, a phase-curve slope of $β= 0.1301 \pm 0.0078$ mag deg$^{-1}$, and a visible geometric albedo of $p_V = 0.106^{+0.003}_{-0.003}$, with colours consistent with moderately red TNO surfaces. No atmosphere or circum-object material is detected down to our sensitivity limits. The best-sampled event also allows a precise measurement of the angular diameter of the occulted star Gaia DR3 4056440205544338944, $θ_\star = 0.670 \pm 0.010$ mas.