{"references": ["Beck, T. L., Schaefer, G. H., Guilloteau, S., et al. 2020, ApJ, 902, 132", "Duch\\^ene, G., Ghez, A. M., McCabe, C., & Ceccarelli, C. 2005, ApJ, 628, 832", "Foreman-Mackey, D., Hogg, D. W., Lang, D., & Goodman, J. 2013, PASP, 125, 306", "Hartmann, L., Hewett, R., Stahler, S., & Mathieu, R. D. 1986, ApJ, 309, 275", "K\u00f6hler, R., Kasper, M., Herbst, T. M., Ratzka, T., & Bertrang, G. H. M. 2016, A&A, 587, A35", "K\u00f6hler, R., and Kubiak, K. 2020, Research Notes of the AAS, 4, 73", "Schaefer, G. H., Beck, T. L., Prato, L., & Simon, M. 2020, AJ, 160, 35"]}

In this contribution I present my latest analysis of the orbits in the famous triple system T Tauri. I discuss what we can deduce about the 3D structure of the system and the long-standing question whether T Tau S is in front or in the back of T Tau N. I also describe how a circumbinary disk around T Tau Sa/Sb can explain the brightness fluctuations of T Tau Sb, because its orbital motion moved it behind the denser parts of the disk in 2016. In the coming years, the motion of T Tau Sb will allow us to probe the near side of the circumbinary disk.