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Table 9

Semi-major axes and minimum masses of exoplanets, and habitable zones of host stars derived from orbital parameters (found in the literature) and stellar parameters estimated in this work from isochrones (see Sect. 5.1).

Old solution Young solution
Star Planet a mpsin(i) a mpsin(i) HZ
[au] [MJup] [au] [MJup] [au]

HD 3651 b 0.2908 ± 0.0045 0.220 ± 0.021 0.2955 ± 0.0026 0.227 ± 0.021 0.62–1.23
HD 9826 b 0.0594 ± 0.0116 0.692 ± 0.027 0.06010 ± 0.00040 0.708 ± 0.010 1.56–3.14
c 2.521 ± 0.049 4.16 ± 0.16 2.551 ± 0.017 4.257 ± 0.064
d 0.830 ± 0.016 1.994 ± 0.079 0.8401 ± 0.0056 2.041 ± 0.033
e 5.26 ± 0.10 1.066 ± 0.050 5.324 ± 0.035 1.091 ± 0.033
HD 19994 b 1.415 ± 0.029 1.658 ± 0.111 1.4639 ± 0.0096 1.775 ± 0.098 1.64–3.29
HD 167042 b 1.281 ± 0.089 1.67 ± 0.24 3.24–6.42
HD 170693 b 1.148 ± 0.031 3.61 ±0.31 11.15–22.14
HD 173416 b 1.016 ± 0.066 2.08 ± 0.28 8.46–16.79
HD 190360 b 4.02 ± 0.11 1.573 ± 0.073 4.067 ± 0.098 1.61 ± 0.06 0.88–1.76
c 0.1314 ± 0.0025 18.97 ± 4.58* 0.1331 ± 0.0019 19.42 ± 4.69*
HD 217014 b 0.0532 ± 0.0010 0.480 ± 0.019 0.0534 ± 0.0011 0.485 ± 0.021 0.95–1.90
HD 221345 b 0.615 ± 0.015 2.61 ± 0.14 7.02–13.9

Notes. We took MJup = 1.8986 × 1027 kg.

(*)

Expressed in Earth mass, with M = 5.9736 × 1024 kg.

(†)

Lies in the HZ.

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