Planet HD 3651 c
| Name | HD 3651 c | ||
| Planet Status | Retracted | ||
| Discovered in | 2013 | ||
| Mass | 0.09 ( -0.03 +0.03 ) MJ | ||
| Mass*sin(i) | 0.09 ( -0.03 +0.03 ) MJ |  |
|
| Semi-Major Axis | 0.186 (± 0.002) AU | |
|
| Orbital Period | 31.0 (± 0.02) day | |
|
| Eccentricity | 0.04 (± 0.2) | |
|
| ω | 55.0 (± 66.0) deg | |
|
| Tperi | — | ||
| Radius | — | ||
| Inclination | — | ||
| Update | 2019-03-04 | ||
| Detection Method | Radial Velocity | ||
| Mass Detection Method | — | ||
| 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 | — |
Star
HD 3651| Name | HD 3651 | ||
| Distance | 11.0 pc | |
|
| Spectral type | K0 V | ||
| Apparent magnitude V | 5.8 | ||
| Mass | 0.79 MSun | |
|
| Age | 5.13 Gyr | |
|
| Effective temperature | 5173.0 K | |
|
| Radius | 0.947 (± 0.032) RSun | |
|
| Metallicity [Fe/H] | 0.05 (± 0.05) | |
|
| Detected Disc | IR Excess | |
|
| Magnetic Field | — | ||
| RA2000 | 00:39:21.0 | ||
| Dec2000 | +21:15:01 | ||
| Alternate Names | 54 Psc | ||
| Planetary system | 2 planets |
Remarks
Sibthorpe et al. 2018 : A debris disk is detected in Herschel data.More data
- Simbad
- Most recent references (ADS)
AMD-Stability Calculator for the System 
Observability Predictor
Remarks
Wittenmeyer et al. (2013) : the presence of HD3651 c improves the fit of the data.Wittenmyer et al. (2018) : New data show no evidence for second planet.
Related publications
Truly eccentric - I. Revisiting eight single-eccentric planetary systems
2019
WITTENMYER R., CLARCK J., ZHAO J., HORNER J., WANG S. & JOHNS D.
MNRAS, 484, 5859
arxiv
article
ADS
Analysis of the Herschel DEBRIS Sun-like star sample
2018
SIBTHORPE, B., KENNEDY, G., WYATT, M. et al.
MNRAS, 475, 3046
paper
ADS
Orbital stability of coplanar two-planet exosystems with high eccentricities
2016
ANTONIADOU K. & VOYATZIS G.
MNRAS, 461, 3822
arxiv
paper
ADS
Highly eccentric exoplanets trapped in mean-motion resonances
2015
ANTONIADOU K. & VOYATZIS G.
in "12th Hel.A.S Conference", Thessaloniki
arxiv
Forever alone? Testing single eccentric planetary systems for multiple companions
2013
WITTENMYER R., WANG S., HORNER J., TINNEY Ch., BUTLER P. & 6 additional authors
ApJ. Suppl., accepted
paper arxiv
Eleven Exoplanet Host Star Angular Diameters from the Chara Array
2008
BAINES E., McALISTER H., ten BRUMMELAAR Th., TURNER N., STURMANN J., STURMANN L., GOLDFINGER P., & RIDGWAY S.
ApJ., 701, 154
paper
On the Ages of Exoplanet Host Stars
2005
SAFFE C., GOMEZ M. & CHAVERO C.
Astron. & Astrophys., 443, 609
paper arxiv
A Sub-Saturn Mass Planet Orbiting HD 3651.
2003
FISCHER D., BUTLER P., MARCY G., VOGT S. & HENRY G.
ApJ., 590, 1081
paper
