Planet Kepler-1647 (AB) b

Name	Kepler-1647 (AB) b
Planet Status	Confirmed
Discovered in	2015
Mass	1.52 ( _-0.65 ^+0.65 ) M_J
Mass*sin(i)	—
Semi-Major Axis	2.7205 (± 0.007) AU
Orbital Period	1107.5923 (± 0.0227) day
Eccentricity	0.0581 (± 0.0689)
ω	155.0464 (± 146.5723) deg
T_peri	—
Radius	1.06 ( _-0.01 ^+0.01 ) R_J
Inclination	90.0972 (± 0.0035) deg
Update	2016-10-14
Detection Method	Primary Transit
Mass Detection Method	—
Radius Detection Method	Primary Transit
Primary transit	—
Secondary transit	—
λ	—
Impact Parameter b	—
Time V_r=0	—
Velocity Semiamplitude K	—
Calculated temperature	—
Measured temperature	—
Hottest point longitude	—
Geometric albedo	—
Surface gravity log(g/g_H)	—
Alternate Names	—

Star

Kepler-1647 (AB)

Name	Kepler-1647 (AB)
Distance	—
Spectral type
Apparent magnitude V	13.78
Mass	2.1885 (± 0.01) M_Sun
Age	—
Effective temperature	6210.0 (± 100.0) K
Radius	1.79 (± 0.006) R_Sun
Metallicity [Fe/H]	—
Detected Disc	—
Magnetic Field	—
RA₂₀₀₀	19:52:36.0
Dec₂₀₀₀	+40:39:22
Alternate Names
Planetary system	1 planet

Remarks

2 Dec 2015: The parent star is an eclipsing binary with an orbital period 11 d. The mass given in this page is the sum of the primary and secondary masses. The full parameters are:
Star A: M = 1.22 ± 0.01 M_Sun, R = 1.79 ± 0055 R_Sun, T = 6210 u 100 K
Star B: M = 0.97 ± 0.0039 M_Sun, R = 0.966 ± 0055 R_Sun, T = 5770 u 125 K

More data

Simbad
Most recent references (ADS)

Observability Predictor

Remarks

02 Dec 2015: Three planetary transits have been observed as of Dec 2015, two for the primary star, the third one at the time of eclipse of the parent eclipsing binary star. The planet revolves around an 11-day period eclipsing binary (Kostov et al. 2015).

Related publications

Analyzing the Habitable Zones of Circumbinary Planets Using Machine Learning
2022 KONG Zh., JIANG J., BURN R., FAHY K. & ZHU Z.
ApJ, 929, 187
paper arxiv

Formation of Earth-sized planets within the Kepler-1647 System Habitable Zone
2021 BARBOSA G., WINTER O., AMARANTE A. & MACAU E.
MNRAS, 504, 6144
paper arxiv

Circumbinary habitable zones in the presence of a giant planet
2021 GEORGAKARATOS N., EGGL S. & DOBBS-DIXON I.
Frontiers in Astronomy and Space Sciences, accepted
arxiv

On the Detection of Habitable Trojan Planets in the Kepler Circumbinary Systems
2021 SUDOL J. & HAGHIGHPOUR N.
Astron. J., 161, 223
paper arxiv

Multiple Transits during a Single Conjunction: Identifying Transiting Circumbinary Planetary Candidates from TESS
2020 KOSTOV V., WELSH W., HAGHIGHIPOUR N., AGOL E., FABRYCKY D. et al.
Astron. J., 160, 174
paper arxiv

Tidal evolution of circumbinary systems with arbitrary eccentricities: applications for Kepler systems
2020 ZOPPETTI F., LEIVA A. & BEAUGE C.
Astron. & Astrophys., 634, A12
paper arxiv

Orbital Evolution of a Circumbinary Planet in a Gaseous Disk
2019 YAMANAKA A. & SASAKI T.
Earth, Planets and Space, accepted
arxiv

Could there be an undetected inner planet near the stability limit in Kepler-1647?
2019 HONG Z., QUARLES B., LI G. & OROSZ J.
Astron. J., 158, 8
paper arxiv

Stability Limits of Circumbinary Planets: Is There a Pile-up in the Kepler CBPs?
2018 QUARLES B., SATYAL S., KOSTOV V., KAIB N. & HAGHIGHIPOUR N.
ApJ, 856, 150
paper arxiv

Fitting Formulae and Constraints for the Existence of S-type and P-type Habitable Zones in Binary Systems
2017 WANG Zh & CUNTZ M.
Astron. J., 154, 157
paper arxiv

Secular Dynamics of Multiplanetary Circumbinary Systems
2017 ANDRADE-INES E. & ROBUTEL Ph.
Cel. Mech. & Dyn. Astron., 130
arxiv paper

Circumbinary planets II - when transits come and go
2016 MARTIN D.
MNRAS, 465, 3235
paper arxiv ADS

Tatooine's Future: The Eccentric Response of Kepler's Circumbinary Planets to Common-Envelope Evolution of their Host Stars
2016 KOSTOV V., MOORE K., TAMAYO D., JAYAWARDHANA R. & RINEHART S.
ApJ, 832, 183
paper arxiv ADS

Kepler-1647 b: the largest and longest-period Kepler transiting circumbinary planet
2016 KOSTOV V., OROSZ J., WELSH W., DOYLE L., FABRYCKY D. et al.
ApJ, 827, 86
arxiv paper ADS