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Table 1
Physical properties of the GJ 3470 system.
Parameters | Symbol | Value | Reference | |||
---|---|---|---|---|---|---|
Distance from Earth | D* | 29.45 ± 0.07 pc | ||||
Star radius | R* | 0.547 ± 0.018 R⊙ | Awiphan et al. 2016 | |||
Star mass | M* | ![]() |
Demory et al. 2013 | |||
Star rotation period | P* | 20.70 ± 0.15 d | Biddle et al. 2014 | |||
Star age | τ* | ~2 Gyr | This work | |||
Heliocentric stellar radial velocity | γ*∕⊙ | 26.51691 ± 5.3 × 10−4 km s−1 | Bonfils et al. 2012 | |||
Planet radius (358 nm) | Rp | 4.8 ± 0.2 REarth | Chen et al. 2017 | |||
Planet mass | Mp | 13.9 ± 1.5 MEarth | Demory et al. 2013 | |||
Orbital period | Pp | 3.33665173 ± 5.9 × 10−7 days | Chen et al. 2017 | |||
Transit center | T0 | 2455983.70417 ± 0.00011 BJDTDB | Chen et al. 2017 | |||
Semi-major axis | ap | 0.0355 ± 0.0019 au | Awiphan et al. 2016 | |||
Eccentricity | e | ![]() |
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Argument of periastron | ω | ![]() |
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Inclination | ip | ![]() |
Awiphan et al. 2016 |
Notes. The distance from GJ 3470 was derived from its Gaia parallax measurement (33.96 ± 0.06 mas; Gaia Collaboration 2016, 2018). The values for e and ω were derived from radial velocity measurements of GJ 3470 (X. Bonfils, priv. comm.).
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