Planet Kepler-1625 b

Name Kepler-1625 b
Planet Status Confirmed
Discovered in 2016
Mass 11.6 ( -11.6 +0.0 ) MJ +
Mass*sin(i)
Semi-Major Axis
Orbital Period 287.378949 ( -0.002983 +0.002983 ) day
Eccentricity
ω
Tperi
Radius 0.6 RJ +
Inclination
Update 2020-01-30
Detection Method Primary Transit
Mass Detection Method Spectrum
Radius Detection Method Primary Transit
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

Kepler-1625
Name Kepler-1625
Distance 2460.0 (± 200.0) pc
Spectral type
Apparent magnitude V
Mass 0.96 ( -0.06 +0.06 ) MSun
Age
Effective temperature 5677.0 ( -162.14 +107.4 ) K
Radius 1.793 ( -0.488 +0.263 ) RSun
Metallicity [Fe/H] 0.01 ( -0.189 +0.134 )
Detected Disc
Magnetic Field
RA2000 19:41:43.0
Dec2000 +39:53:12
Alternate Names
Planetary system 1 planet

More data

Observability Predictor

Remarks

4 Oct 2018: The planet has a 4 REarth and ~ 20 MEarth companion at ~ 40 RJup (Teatchey & Kipping 2018). See Kepler-1625 b I
1 May 2019: The moon Kepler-1625 b I is challenged by Kreidberg et al. (2019).

Related publications

The Exomoon Corridor: Half of all exomoons exhibit TTV frequencies within a narrow window due to aliasing
2021 KIPPING D.
MNRAS, 500, 1851
paper  arxiv  

Radial velocity constraints on the long-period transiting planet Kepler-1625 b with CARMENES
2020 TIMMERMANN A., HELLER R., REINERS A. & ZECHMEISTER M.
Astron. & Astrophys., 635, A59
paper  arxiv  

Loose Ends for the Exomoon Candidate Host Kepler-1625b
2020 TEACHEY A., KIPPING D., BURKE Ch., ANGUS R. & HOWARD A.
Astron. J., 159, 142
paper  arxiv  

Impact of Tides on the Potential for Exoplanets to Host Exomoons
2020 TOKADJIAN A. & PIRO A.
Astron. J., 160, 194
paper  arxiv

Exploring formation scenarios for the exomoon candidate Kepler 1625b I
2020 MORAES R. & VIERA NETO E.
MNRAS, 495, 3763
paper

Exploring formation scenarios for the exomoon candidate Kepler 1625b I
2020 MORAES R. & NETO E.
MNRAS, accepted
arxiv

Orbital Stability of Exomoons and Submoons with Applications to Kepler 1625b-I
2020 ROSARIO-FRANCO M., QUARLES B., MUSIELAK Z. & CUNTZ M.
Astron. J., 159, 260
paper   arxiv

Astrophysical Simulations and Data Analyses on the Formation, Detection, and Habitability of Moons Around Extrasolar Planets
2020 HELLER R.
Habilitation thesis, Georg August University G\"ottingen,
arxiv

Exomoon indicators in high-precision transit light curves
2020 RODENBECK K., HELLER R. & GIZON L.
Astron. & Astrophys., 638, A43
paper   arxiv  

An Independent Analysis of the Six Recently Claimed Exomoon Candidates
2020 KIPPING D.
Astron. J., 900, L44
paper  arxiv  

Formation of exoplanetary satellites by pull-down capture
2019 B. HANSEN
Science Advance, 5, eaaw8665
paper  

Transits of Inclined Exomoons - Hide and Seek and an Application to Kepler-1625
2019 MARTIN D., FABRYCKY D. & MONTET B.
ApJ, 875, L25
paper   arxiv  

An alternative interpretation of the exomoon candidate signal in the combined Kepler and Hubble data of Kepler-1625
2019 HELLER R., RODENBECK K. & BRUNO G. An alternative interpretation of the exomoon candidate signal in the combined Kepler and Hubble data of Kepler-1625
Astron. & Astrophys., 624, A95
paper  arxiv  

No Evidence for Lunar Transit in New Analysis of HST Observations of the Kepler-1625 System
2019 KREIDBERG L., LUGER R. & BEDELL M.
ApJ. Letters, 877, L15
paper  arxiv  

Climate Modeling of Hypothetical Moon-moons in the Kepler-1625b System
2018 FORGAN D.
AAS Reseach Notes, 2, 191
paper  arxiv  

Evidence for a large exomoon orbiting Kepler-1625b
2018 TEACHEY A. & KIPPING D.
Science Adv., 4, eaav1784
paper arxiv  

HEK VI: On the Dearth of Galilean Analogs in Kepler and the Exomoon Candidate Kepler-1625b I
2017 TEACHEY A., KIPPING D. & SCHMITT A.
Astron. J., 155, 36
paper  arxiv   ADS  

False Positive Probabilities for all Kepler Objects of Interest: 1284 Newly Validated Planets and 428 Likely False Positives
2016 MORTON T., BRYSON S., COUGHLIN J., ROWE J., RAVICHANDRAN G. et al.
ApJ, 822, 86
paper  arxiv   ADS