Bayesian analysis of interiors of HD 219134b, Kepler-10b, Kepler-93b, CoRoT-7b, 55 Cnc e, and HD 97658b using stellar abundance proxies

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Table 3

Data of selected exoplanets.

Name	M [M_⊕]	R [R_⊕]	Fe/Si_bulk	Mg/Si_bulk	Na₂O [wt%]	Al₂O₃ [wt%]

HD 219134 b (V0)	4.36 ± 0.44	1.606 ± 0.086	1.73 ± 1.55	1.44 ± 0.91	0.021	0.055
HD 219134 b V1	4.36 ± 0.44	1.606 ± 0.086	10.68 ± 1.55	1.02 ± 0.91	0.01	0.023
HD 219134 b V2	4.36 ± 0.44	1.606 ± 0.086	1.00 ± 1.55	1.14 ± 0.91	0.025	0.057
Kepler 10-b	3.7 ± 0.43	1.47 ± 0.02	2.18 ± 0.41	1.14 ± 0.28	0.02	0.05
Kepler 93-b	4.02 ± 0.68	1.478 ± 0.019	2.87 ± 0.98	1.02 ± 0.38	0.02	0.05
CoRoT 7-b	4.386 ± 0.985	1.614 ± 0.102	2.34 ± 0.68	0.87 ± 0.25	0.02	0.05
HD 97658b (V0)	7.866 ± 0.73	2.340 ± 0.165	2.03 ± 1.17	0.87 ± 0.33	0.018	0.046
HD 97658b V1	7.866 ± 0.73	2.340 ± 0.165	2.87 ± 1.17	0.93 ± 0.33	0.018	0.045
HD 97658b V2	7.866 ± 0.73	2.340 ± 0.165	1.41 ± 1.17	0.95 ± 0.33	0.019	0.05
55 Cnc e^L (V0)	8.37 ± 0.38	2.08 ± 0.16	1.86 ± 1.49	0.93 ± 0.77	0.024	0.062
55 Cnc e^S (V0)	8.37 ± 0.38	1.75 ± 0.13	1.86 ± 1.49	0.93 ± 0.77	0.024	0.062
55 Cnc e^S/LV1	8.37 ± 0.38	1.75 ± 0.13/2.08 ± 0.16	4.06 ± 1.49	1.02 ± 0.77	0.012	0.046
55 Cnc e^S/L V2	8.37 ± 0.38	1.75 ± 0.13/2.08 ± 0.16	0.89 ± 1.49	1.54 ± 0.77	0.024	0.048

Name	CaO [wt%]	R_star [R_sun]	T_star [T_sun]	Semi-major axis [AU]

HD 219134 b (V0)	0.021	0.778	0.815	0.038
HD 219134 b V1	0.01	0.778	0.815	0.038
HD 219134 b V2	0.021	0.778	0.815	0.038
Kepler 10-b	0.02	1.065	0.978	0.017
Kepler 93-b	0.02	0.919	0.983	0.054
CoRoT 7-b	0.02	0.870	0.921	0.017
HD 97658b (V0)	0.017	0.703	0.887	0.08
HD 97658b V1	0.017	0.703	0.887	0.08
HD 97658b V2	0.019	0.703	0.887	0.08
55 Cnc e^L (V0)	0.013	0.943	0.901	0.015
55 Cnc e^S (V0)	0.013	0.943	0.901	0.015
55 Cnc e^S/LV1	0.008	0.943	0.901	0.015
55 Cnc e^S/L V2	0.016	0.943	0.901	0.015

Notes. V0 represents median abundance estimates, whereas V1 and V2 refer to iron-rich and iron-poor cases as listed in Table 2; indices L and S of 55 Cnc e refer to different radius estimates (see Sect. 2).

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