Photodynamical model light curve of KIC 7955301 for the present century. The ∼19.2 yr-period precession cycle is clearly visible. Within a cycle the inner pair exhibits regular eclipses during a ∼7.3 yr-long interval. The last eclipsing session had finished by January 2, 2016 with a short (∼80 ppm) amplitude fading, while the next session is expected to begin on January 18, 2028. The gray vertical area represents the time of Kepler observations, and TESS Sector 14 observations are also denoted with a thin vertical line.