Planet HD 37124 c

Name HD 37124 c
Planet Status Confirmed
Discovered in 2005
Mass 0.652 ( -0.052 +0.052 ) MJ
Mass*sin(i) 0.652 ( -0.052 +0.052 ) MJ
Semi-Major Axis 1.71 (± 0.0065) AU
Orbital Period 885.5 (± 5.1) day
Eccentricity 0.125 (± 0.055)
ω 53.0 (± 17.0) deg
Tperi 2449534.0 (± 11.0) JD
Radius
Inclination
Update 2013-05-20
Detection Method Radial Velocity
Mass Detection Method
Radius Detection Method
Primary transit
Secondary transit
λ
Impact Parameter b
Time Vr=0
Velocity Semiamplitude K
Calculated temperature
Measured temperature
Hottest point longitude
Geometric albedo
Surface gravity log(g/gH)
Alternate Names

Star

HD 37124
Name HD 37124
Distance 33.0 pc
Spectral type G4 V
Apparent magnitude V 7.68
Mass 0.83 MSun
Age 3.33 Gyr
Effective temperature 5610.0 (± 70.0) K
Radius 0.82 RSun
Metallicity [Fe/H] -0.442
Detected Disc
Magnetic Field
RA2000 05:37:02.0
Dec2000 +20:43:50
Alternate Names
Planetary system
3 planets

Remarks

24 Dec 2010: In agreement with Feroz et al. (2011) and Wright et al. (2009), the planet d is the long period planet and planet c the intermediate period planet
08 Oct 2009: According to J. Wright, Keck data has resolved the ambiguity for planet c and favors the long period 2295 d solution (Wright "A Survey of Multiple Planet Systems" in Extrasolar planets in multi-body systems: theory and observation, Torun 2008)
24 Jun 2005: An alternate model (Vogt et al 2005) gives for planet d: Period = 29.92

More data

AMD-Stability Calculator for the System

Observability Predictor

Remarks

07 Jan 2011: Ralative inclination between orbits of planets b and c must be less than ~30 - 40 deg. in order to be stable (Wright et al 2011)

Related publications

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