Planets that will be observed with MIRI in transit in JWST Cycles 1–5. As mentioned in Section 5, we see a wide variety of planet sizes and equilibrium temperatures. The currently published planets are shown in black dots and listed in Table 1 and Figure 1. We have omitted the white dwarf planet WD 1856 b (T_eq = 160 K, R_p = 10.2 R_⊕, Cycle 4), as well as the disintegrating planets K2-22 b (see Section 2.1) and BD +05 4868 A b (T_eq = 1820 K, unknown R_p, Cycle 4).