Planet Kepler-80 d
| Name | Kepler-80 d | ||
| Planet Status | Confirmed | ||
| Discovered in | 2014 | ||
| Mass | 0.02124 ( -0.0016 +0.00217 ) MJ |  |
|
| Mass*sin(i) | — | ||
| Semi-Major Axis | 0.0372 ( -0.0005 +0.0005 ) AU | |
|
| Orbital Period | 3.07222 ( -4e-05 +6e-05 ) day | |
|
| Eccentricity | — | ||
| ω | — | ||
| Tperi | — | ||
| Radius | 0.136 ( -0.006 +0.008 ) RJ | |
|
| Inclination | 88.35 ( -1.51 +1.12 ) deg | |
|
| Update | 2021-02-05 | ||
| Detection Method | Primary Transit | ||
| Mass Detection Method | TTV | ||
| Radius Detection Method | — | ||
| 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 | KOI-500 d, 2MASS J19442701+3958436 d, K00500.03, KIC 4852528 d, KOI-500.03, WISE J194427.01+395843.5 d |
Star
Kepler-80| Name | Kepler-80 | ||
| Distance | 357.0 pc | ||
| Spectral type | K5 | ||
| Apparent magnitude V | 15.0 | ||
| Mass | 0.73 ( -0.03 +0.03 ) MSun | ||
| Age | 2.0 ( --1.0 +1.0 ) Gyr | ||
| Effective temperature | 4540.0 ( -100.0 +100.0 ) K | ||
| Radius | 0.68 ( -0.02 +0.02 ) RSun | ||
| Metallicity [Fe/H] | 0.04 ( -0.08 +0.08 ) | ||
| Detected Disc | — | ||
| Magnetic Field | — | ||
| RA2000 | 19:44:27.0 | ||
| Dec2000 | +39:58:44 | ||
| Alternate Names | KOI-500, 2MASS J19442701+3958436, KIC 4852528, WISE J194427.01+395843.5 | ||
| Planetary system | 6 planets |
Remarks
Alias KIC 4852528Alias 2MASS 19442701+3958436
More data
- Simbad
- Most recent references (ADS)
Observability Predictor 
Remarks
Alias KOI-500.033 Sep 2012: The TTVs constrain the planet mass (Ragozzine et al. 2012)
Related publications
Tidal interactions' shape period ratios in planetary systems with three-body resonant chains
2023
CHARALAMBOUS C., TEYSSANDIER J. & LIBERT A.-S.
Astron. & Astrophys., 677, A160
paper
Mean motion resonance capture in the context of type I migration
2023
KAJTAZI K., PETIT A. & JOHANSEN A.
Astron. & Astrophys., 669, A53
paper arxiv
Kepler-80 Revisited: Assessing the Participation of a Newly Discovered Planet in the Resonant Chain
2023
WEISSERMAN D., BECKER J. & VANDERBURG A.
Astron. J., 165, 89
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exoMMR: a New Python Package to Confirm and Characterize Mean Motion Resonances
2023
MacDONALD M., POLANIA VIVAS M., D'ANGIOLILLO S., FERNANDEZ A. & QUINN T.
Astron. J., accepted
arxiv
A Criterion for the Stability of Planets in Chains of Resonances
2022
GOLDBERG M., BATYGIN K. & MORBIDELLI A.
Icarus, accepted
arxiv
Architectures of Compact Super-Earth Systems Shaped by Instabilities
2022
GOLDBERG M. & BATYGIN K.
Astron. J., 163, 201
paper arxiv
Is the orbital distribution of multiplanet systems influenced by pure three-planet resonances?
2022
CERIONI M., BEAUGE C. & GALLARDO T.
MNRAS, 513, 541
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A Five-Planet Resonant Chain: Reevaluation of the Kepler-80 System
2021
MacDONALD M., SHAKZSPEARE C. & RAGOZZINE D.
Astron. J., 162, 114
paper arxiv
How Close are Compact Multi-Planet Systems to the Stability Limit?
2021
YEE S., TAMAYO D., HADDEN S. & WINN J.
Astron. J., 162, 55
paper arxiv
Chains of Planets in Mean Motion Resonances Arising from Oligarchic Growth
2020
MORRISON S., DAWSON R. & MACDONALD M.
ApJ, 904, 157
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Identifying Exoplanets with Deep Learning: A Five Planet Resonant Chain around Kepler-80 and an Eighth Planet around Kepler-90
2018
SHALLUE Ch. & VANDERBURG A.
Astron. J., 155, 94
paper arxiv
A Dynamical Analysis of the Kepler-80 System of Five Transiting Planets
2016
MACDONALD, M., RAGOZZINE, D., FABRYCKY, D., FORD, E., HOLMAN, M. & 8 additional authors
Astron. J., accepted
arxiv
paper
ADS
On the formation of compact planetary systems via concurrent core accretion and migration
2016
COLEMAN G. & NELSON R.
MNRAS, 457, 2480
paper arxiv ADS
The Very Compact Five Exoplanet System KOI-500: Mass Constraints from TTVs, Resonances, and Implications
2012
RAGOZZINE D. & Kepler Team
BAAS, 44, no 5, 200.04
abstract
