Poster of the diversity of TNG-Cluster satellites in soft X-ray emission. We show the soft X-ray (0.5−2.0 keV) surface brightness for 16 example TNG-Cluster satellite galaxies at z = 0. Each image is 600 × 600 kpc² in size (scale bar in the upper left). These galaxies are necessarily within a projected distance of 1.5 R_200c of their host. We include information about the galaxy and its host in the upper right and lower left corners; the units of the cluster $M_{200\mathrm{c}}^{\mathrm{host}}$ and satellite $M_{\star }^{\mathrm{sat}}$ mass are [log₁₀ M_⊙], and the soft X-ray luminosity $L_{0.5-2.0\mathrm{keV}}^{<300\mathrm{kpc}}$ is the total X-ray luminosity within a projected aperture of 300 kpc in units of [log₁₀ erg s⁻¹]. Many of the maps display morphological signatures of SMBH feedback, with dome-like inflated bubbles and/or ram pressure, with gas tails extending in specific directions.