Planet Kepler-74 b

Name Kepler-74 b
Planet Status Confirmed
Discovered in 2012
Mass 0.68 ( -0.09 +0.09 ) MJ
Mass*sin(i)
Semi-Major Axis 0.084 (± 0.014) AU
Orbital Period 7.340718 (± 1e-06) day +
Eccentricity 0.287 (± 0.062)
ω 64.0 (± 21.0) deg
Tperi 2454967.04 ( -0.21 +0.34 ) JD
Radius 1.32 ( -0.14 +0.14 ) RJ
Inclination 85.55 (± 0.96) deg
Update 2016-02-24
Detection Method Primary Transit
Mass Detection Method
Radius Detection Method
Primary transit 2454967.3453 (± 0.0003) 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 KOI-200 b

Star

Kepler-74
Name Kepler-74
Distance 1330.0 (± 170.0) pc
Spectral type F8V
Apparent magnitude V 14.23
Mass 1.4 ( -0.11 +0.14 ) MSun
Age 2.9 ( -0.8 +1.5 ) Gyr
Effective temperature 6050.0 (± 110.0) K
Radius 1.51 (± 0.14) RSun
Metallicity [Fe/H] 0.34 (± 0.14)
Detected Disc
Magnetic Field
RA2000 19:32:22.0
Dec2000 +41:21:20
Alternate Names
Planetary system 1 planet

Remarks

Alias 2MASS 19322220+4121198

More data

Observability Predictor

Remarks

Alias KOI-200.01

Related publications

The Densities of Planets in Multiple Stellar Systems
2017 FURLAN E. & HOWELL S.
Astron. J., 154, 66
arxiv   paper   ADS  

A comprehensive study of Kepler phase curves and secondary eclipses -- temperatures and albedos of confirmed Kepler giant planets
2015 ANGERHAUSEN, D. DELARME, E. & J. MORSE
PASP, in press
paper  arxiv 

Improved parameters of seven Kepler giant companions characterized with SOPHIE and HARPS-N
2015 BONOMO A., SOZZETTI A., SANTERNE A., DELEUIL M., ALMENARA J.-M. et al.
Astron. & Astrophys., 575, A85
paper  paper  ADS  

KOI-200b and KOI-889b: two transiting exoplanets detected and characterized with Kepler, SOPHIE and HARPS-N
2013 HEBRARD G., ALMENARA J.-M., SANTERNE A., DELEUIL M., DAMIANI C. & 6 additional authors
Astron. & Astrophys., 554, A114
paper   arxiv  

SOPHIE velocimetry of Kepler transit candidates VI. A false positive rate of 35% for Kepler close-in giant candidates
2012 SANTERNE A., DIAZ ., MOUTOU C., BOUCHY F., HEBRARD G. & 4 additional authors
Astron. & Astrophys., 545, A76
paper   arxiv