Planet HD 60532 c

Name HD 60532 c
Discovered in 2008
Mass 7.46 MJ
Semi-major axis 1.58 AU
Orbital period 607.06 (± 2.1) day
Eccentricity 0.038 (± 0.008)
ω 119.49 (± 9.14) deg
Tperi 54000.0 JD
Radius
Inclination 20.0 (± 0.0) deg;
Update Jan. 31, 2012
Detection Method Radial Velocity
Mass Detection Method
Radius Detection method
Molecules detected
Primary transit
Secondary transit
Anomaly angle
impact Parameter b
Time Vr=0
Velocity Semiamplitude K
Calculated temperature
Measured temperature
Hottest point longitute
Geometric albedo
Surface gravity log(g/gH)
Alternate Names

Observability Predictor

Other web-pages

Papers with primary data:

Star

Name HD 60532
Distance 25.7 pc
Spectral type F6IV-V
Apparent magnitude V 4.45
Mass 1.44 ( -0.1 +0.1 ) MSun
Age 2.7 (± 0.1) Gyr
Effective temperature 6095.0 K
Radius
Metallicity [Fe/H] -0.26
Detected Disc
Magnetic Field
RA2000 07:34:03.0
Dec2000 -22:17:46
Alternate Names
Planetary system 2 planets

Remarks

05 Feb 08: In Corriea & Laskar 2009, the orbits of planets b and c are assumed to be co-planar.

More data


Related publications

Long-lived Chaotic Orbital Evolution of Exoplanets in Mean Motion Resonances with Mutual Inclinations
2015 BARNES R., DEITRICK R., GREENBERG R., QUINN Th. & RAYMOND S.
ApJ, accepted
arxiv  

HD60532, a planetary system in a 3:1 mean motion resonance
2009 LASKAR J. & CORREIA A.
Astron. & Astrophys., 496, L5
paper

Extrasolar planets and brown dwarfs around A–F type stars - V. A planetary system found with HARPS around the F6IV–V star HD 60532
2008 DESORT M., LAGRANGE A.-M., GALLAND F., BEUST H., UDRY S., MAYOR M. & LO CURTO G.
Astron. & Astrophys., 491, 883
paper
Erratum