NGTS-30b/TOI-4862b: An ~1 Gyr old 98-day transiting warm Jupiter

Open Access

Fig. 12

Period vs. mass plot for all transiting giant exoplanets (0.2 R_J ≤ R_P ≤ 13 R_J) with well-constrained masses $(σ_{M_{P}} / M_{P} \leq 25 %)$ $\left( {{\sigma _{{M_{\rm{P}}}}}/{M_{\rm{P}}} \le 25\% } \right)$ and radii $(σ_{R_{P}} / R_{P} \leq 8 %)$ $\left( {{\sigma _{{R_{\rm{P}}}}}/{R_{\rm{P}}} \le 8{\rm{\% }}} \right)$ . Individual points are colour-coded by the planetary eccentricity, illustrating a general trend towards higher eccentricities at longer periods. TOI-4862 b is circled in black.

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