Planet HD 219134 b
| Name | HD 219134 b | ||
| Planet Status | Confirmed | ||
| Discovered in | 2015 | ||
| Mass | 0.01491 (± 0.0006) MJ |  |
|
| Mass*sin(i) | — | |
|
| Semi-Major Axis | 0.038474 (± 8e-07) AU | |
|
| Orbital Period | 3.0931 (± 0.0001) day | |
|
| Eccentricity | 0.0 ( -0.0 +0.13 ) | |
|
| ω | — | ||
| Tperi | 2449999.5 (± 0.2) JD | |
|
| Radius | 0.14292 (± 0.00491) RJ | |
|
| Inclination | 85.058 (± 0.08) deg | |
|
| Update | 2018-11-28 | ||
| Detection Method | Primary Transit | ||
| Mass Detection Method | Radial Velocity | ||
| Radius Detection Method | Primary Transit | ||
| Primary transit | 2457126.7001 (± 0.001) JD | |
|
| Secondary transit | — | ||
| λ | — | ||
| Impact Parameter b | — | ||
| Time Vr=0 | — | ||
| Velocity Semiamplitude K | 1.9 (± 0.2) m/s | ||
| Calculated temperature | — | ||
| Measured temperature | — | ||
| Hottest point longitude | — | ||
| Geometric albedo | — | ||
| Surface gravity log(g/gH) | — | ||
| Alternate Names | — |
Star
HD 219134| Name | HD 219134 | ||
| Distance | 6.55 pc | |
|
| Spectral type | K3V | ||
| Apparent magnitude V | 5.57 | ||
| Mass | 0.794 MSun | |
|
| Age | — | ||
| Effective temperature | 4699.0 (± 16.0) K | |
|
| Radius | 0.778 (± 0.005) RSun | ||
| Metallicity [Fe/H] | 0.11 (± 0.04) | |
|
| Detected Disc | — | ||
| Magnetic Field | — | ||
| RA2000 | 23:13:17.0 | ||
| Dec2000 | +57:10:06 | ||
| Alternate Names | |||
| Planetary system | 6 planets |
Observability Predictor 
Remarks
17 Nov 2015: The names an characteristics of planets HD 219134 d, e, f, g and h raise two specific problems since there are two papers: Motalebi et al. 2015 and Vogt et al. 2015 with different sets of parameters. We adopt the following solution, at least provisionally:- names: The standard rule is two give names NNN b, c, d etc by order of discovery, the criterion being the date of submission of a paper. The Motalebi et al paper has been submitted on June 24th 2015, the Vogt et al. paper on July 17th 2015. The four Motalebi planets are there fore named b, c, d and e and the new Vogt planets named f, g and h.
- parameter values: The Vogt et al. planet data are based on 276 observation points while the Motalebi et al data are based on 98 data points. We therefore adopt Vogt et al. values for all planet.
- remark: It is not impossible that more data will change this situation. In particular HD 219134 e and h may merge in a single object.
Related publications
A new class of Super-Earths formed from high-temperature condensates: HD219134 b, 55 Cnc e, WASP-47 e
2018
DORN C., HARRISON J., BONSOR A. & HANDS T.
MNRAS, in press
paper arxiv
Characterisation of the HD 219134 multi-planet system I. Observations of stellar magnetism, wind, and high-energy flux
2018
FOLSOM, C., FOSSATI, L., WOOD, B. SREEJITH, A., CUBILLOS, P. et al.
MNRAS, 481, 5286
paper
arxiv
ADS
Characterisation of the HD219134 multi-planet system II. Stellar-wind sputtered exospheres in rocky planets b & c
2018
VIDOTTO, A., LICHTENEGGER, H., FOSSATI, L. FOLSOM, P. WOOD, B. et al.
MNRAS, 481, 5296
paper arxiv
ADS
A grid of upper atmosphere models for 1--40 MEARTH planets: application to CoRoT-7 b and HD219134 b,c
2018
KUBYSHKINA D., FOSSATI L., ERKAEV N., JOHNSTONE C., CUBILOS P. et al.
Astron. & Astrophys., 619, A151
paper arxiv
Secondary atmospheres on HD 219134 b and c
2017
DORN C. & HENG K.
ApJ, accepted
arxiv
Two massive rocky planets transiting a K-dwarf 6.5 parsecs away
2017
GILLON M., DEMORY B.-O., VAN GROOTEL V., MOTALEBI F., LOVIS Ch. et al.
Nature Astronomy, 1, 0056
paper arxiv
ADS
A 12-Year Activity Cycle for the Nearby Planet Host Star HD 219134
2016
JOHNSON M., ENDL M., COCHRAN W., MESCHIARI S., ROBERTSON P. et al.
ApJ, 821, 74
paper arxiv ADS
Bayesian analysis of interiors of HD 219134b, Kepler-10b, Kepler-93b, CoRoT-7b, 55 Cnc e, and HD 97658b using stellar abundance proxies
2016
DORN C., HINKEL N. & VENTURI J.
Astron. & Astrophys., 597, A38
paper arxiv ADS
The HARPS-N Rocky Planet Search I. HD219134b: A transiting rocky planet in a multi-planet system at 6.5 pc from the Sun
2015
MOTALEBI, F., UDRY, S., GILLON, M.. LOVIS, SEGRANSAN & 34 additional authors
Astron. & Astrophys., 584, A72
paper arxiv
ADS
Mass-Radius Relation for Rocky Planets based on PREM
2015
ZENG L., SASSELOV D. & JACOBSEN S.
ApJ, submitted
arxiv
A Six-Planet System Orbiting HD 219134
2015
VOGT S., BURT J., MESCHIARI S., BUTLER P., HENRY G. et al.
ApJ, 814, 12
paper arxiv ADS
