Planet HD 3651 b

Name HD 3651 b
Planet Status Confirmed
Discovered in 2003
Mass 0.23 ( -0.013 +0.297 ) MJ
Mass*sin(i) 0.228 (± 0.011) MJ +
Semi-Major Axis 0.295 (± 0.029) AU +
Orbital Period 62.25 (± 0.004) day +
Eccentricity 0.645 (± 0.002) +
ω 243.0 (± 3.0) deg +
Tperi 2453932.6 (± 0.6) JD +
Radius
Inclination 83.0 ( -56.0 +56.0 ) deg
Update 2019-03-04
Detection Method Radial Velocity
Mass Detection Method
Radius Detection Method
Primary transit
Secondary transit
λ
Impact Parameter b
Time Vr=0
Velocity Semiamplitude K 16.6 (± 0.6) m/s
Calculated temperature
Measured temperature
Hottest point longitude
Geometric albedo
Surface gravity log(g/gH)
Alternate Names 54 Psc b, 54 Piscium A b

Star

HD 3651
Name HD 3651
Distance 11.0 pc
Spectral type K0 V
Apparent magnitude V 5.8
Mass 0.79 MSun
Age 5.13 Gyr
Effective temperature 5173.0 K
Radius 0.947 (± 0.032) RSun
Metallicity [Fe/H] 0.05 (± 0.05)
Detected Disc IR Excess
Magnetic Field
RA2000 00:39:21.0
Dec2000 +21:15:01
Alternate Names 54 Psc
Planetary system
2 planets

Remarks

Sibthorpe et al. 2018 : A debris disk is detected in Herschel data.

More data

AMD-Stability Calculator for the System

Observability Predictor

Remarks

19 Oct 2010: Simpson et al. (2010) infer the orbital inclination from the parent star rotation, deriving a planet mass 0.2+0.2-0MJ; but the coplanarity of stellar equator with planet orbits is generally not demonstrated.
24 Aug. 2006: A brown dwarf companion (M = 20 to 60 MJup, projected separation 480 AU) has been detected by direct imaging (Luhman et al. 2006, Mugrauer et al 2006). The brown dwarf is added in the base as HD 3651 B.

Other web-pages


Related publications

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