Planet Kepler-32 b

Name Kepler-32 b
Planet Status Confirmed
Discovered in 2011
Mass < 4.1 MJ
Mass*sin(i)
Semi-Major Axis 0.05 AU
Orbital Period 5.90124 (± 0.0001) day
Eccentricity
ω
Tperi
Radius 0.196 ( -0.018 +0.018 ) RJ
Inclination
Update 2021-02-05
Detection Method Primary Transit
Mass Detection Method
Radius Detection Method
Primary transit 2454974.902 (± 0.008) JD
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 2MASS J19512217+4634273 b, K00952.01, KIC 9787239 b, KOI-952 b, KOI-952.01, WISE J195122.14+463427.5 b

Star

Kepler-32
Name Kepler-32
Distance 326.85 ( -3.44 +3.44 ) pc
Spectral type M1 V
Apparent magnitude V 16.0
Mass 0.58 (± 0.05) MSun
Age
Effective temperature 3900.0 (± 200.0) K
Radius 0.53 (± 0.04) RSun
Metallicity [Fe/H] 0.0
Detected Disc
Magnetic Field
RA2000 19:51:22.2
Dec2000 +46:34:27
Alternate Names 2MASS J19512217+4634273, KIC 9787239, KOI-952, WISE J195122.14+463427.5
Planetary system
5 planets

Remarks

Alias KOI 952
Alias KIC 9787239
Alias 2MASS 19512217+4634273

More data

Observability Predictor

Remarks

28 Jan 2012: The upper mass limit is inferred from tranist time variations, simple planet models and dynamical stability (Fabrycky et al; 2012)

Related publications

There might be giants: unseen Jupiter-mass planets as sculptors of tightly-packed planetary systems
2016 HANDS T. & ALEXANDER R.
MNRAS, 456, 4121
paper  arxiv  ADS

Gravitational quantization of exoplanet orbits in HD 10180, Kepler-32, Kepler-33, Kepler-102, and Kepler-186
2015 GEROYANNIS V.
arxiv  

Understanding the assembly of Kepler's compact planetary systems
2014 HANDS, T., ALEXANDER, R. & W. DEHNEN
MNRAS, 445, 749
paper  arxiv 

Transit Timing Observations from Kepler: IV. Confirmation of 4 Multiple Planet Systems by Simple Physical Models
2012 FABRYCKY D., FORD E., STEFFEN J., ROWE J., CARTER J. & 29 additional authors
ApJ., 750, 114
paper   arxiv

Transit Timing Observations from Kepler. IV. Confirmation of Four Multiple-planet Systems by Simple Physical Models
2012 FABRYCKY D. C., FORD E. B., STEFFEN J. H., ROWE J. F., CARTER J. A. et al.
The Astrophysical Journal, 750, 114
ADS

The Exoplanet Handbook
2011 Michael Perryman
Content
Content and Chapter 5