Planet GJ 667 C d
| Name | GJ 667 C d | ||
| Planet Status | Candidate | ||
| Discovered in | 2012 | ||
| Mass | — | ||
| Mass*sin(i) | 0.01604 ( -0.00535 +0.00566 ) MJ |  |
|
| Semi-Major Axis | 0.276 ( -0.03 +0.024 ) AU | |
|
| Orbital Period | 91.61 ( -0.89 +0.81 ) day | |
|
| Eccentricity | 0.03 ( -0.03 +0.2 ) | |
|
| ω | 40.11 (± 360.0) deg | |
|
| Tperi | 2454499.0 (± 1.0) JD | ||
| Radius | — | ||
| Inclination | — | ||
| Update | 2021-10-05 | ||
| 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
GJ 667 C| Name | GJ 667 C | ||
| Distance | 6.84 (± 0.4) pc | |
|
| Spectral type | M1.5V | ||
| Apparent magnitude V | 10.22 | ||
| Mass | 0.33 MSun | |
|
| Age | > 2.0 Gyr | |
|
| Effective temperature | 3600.0 K | |
|
| Radius | — | ||
| Metallicity [Fe/H] | -0.55 | |
|
| Detected Disc | — | ||
| Magnetic Field | — | ||
| RA2000 | 17:18:57.0 | ||
| Dec2000 | -34:59:23 | ||
| Alternate Names | |||
| Planetary system | 5 planets |
Other web-pages
Papers with primary data:- Radial Velocity:
More data
- Simbad
- Most recent references (ADS)
Observability Predictor 
Remarks
04 Feb 2012: The planet GJ667C d is uncertain, the RV signal being affected by the rotation period of the star at ~106 days (Anglada-Escudé et al. 2012, Delfosse et al. 2012).Related publications
The Surface UV Environment on Planets Orbiting M-Dwarfs: Implications for Prebiotic Chemistry & Need for Experimental Follow-Up
2017
RANJAN S., WORDSWORTH R. & SASSELOV D.
ApJ, submitted
arxiv
The Spin-Orbit Evolution of GJ 667C System: The Effect of Composition and Other Planet's Perturbations
2016
CUARTAS-RESTREPO P., MELITA M., ZULUAGA J., PORTILLA B.SUCERQUIA M. & MILONI D.
MNRAS, 463, 1592
arxiv paper ADS
Living with a Red Dwarf: Rotation and X-ray and Ultraviolet Properties of the Halo Population Kapteyn's Star
2016
GUINAN E., ENGLE S. & DURBIN A.
ApJ, accepted
arxiv
Dynamical evolution and spin-orbit resonances of potentially habitable exoplanets. The case of GJ 667C
2014
MAKAROV V. & BERGHEA C.
ApJ, 780, 124
paper arxiv
Disentangling Planets and Stellar Activity for Gliese 667C
2014
ROBERTSON, P. & S. MAHADEVAN
ApJ Letters, 793, L24
paper arxiv
The Solar Neighborhood. XXXIV. a Search for Planets Orbiting Nearby M Dwarfs Using Astrometry
2014
LURIE J., HENRY T., JAO W.-Ch., QUINN S., WINTERS J. et al.
Astron. J., 148, 91
paper
A dynamically-packed planetary system around GJ667C with three super-Earths in its habitable zone
2013
ANGLADA-ESCUDE G., TUOMI M., GERLACH E., BARNES R., HELLER R. & 6 additional authors
Astron. & Astrophys., 556
arxiv
paper
Bayesian analysis of radial velocity data of GJ667C with correlated noise: evidence for no more than 3 planets
2013
FEROZ F., & HOBSON M.
MNRAS, in press
paper arxiv
Resonant periodic orbits in the exoplanetary systems
2013
ANTONIADOU K. & VOYATZIS G.
Astrophys. & Spa. Sci., in press
paper arxiv
The HARPS search for southern extra-solar planets XXXV. Super-Earths around the M-dwarf neighbors Gl433 and Gl667C
2013
DELFOSSE X., BONFILS X., FORVEILLE Th., UDRY S., MAYOR M. & 9 additional authors
Astron. & Astrophys., 553, A8
paper arxiv
Evidence for Multiple Planets in the Habitable Zone of Gliese 667C: A Bayesian Re-analysis of the HARPS data
2012
GREGORY Ph.
MNRAS, submitted
arxiv
A planetary system around the nearby M dwarf GJ 667C with at least one super-Earth in its habitable zone
2012
ANGLADA-ESCUDE G., ARRIAGADA P., VOGT S., RIVERA E., BUTLER P. & 12 additional authors
ApJ. Letters, 751, L16
paper arxiv
The Exoplanet Handbook
2011
Michael Perryman
Content
Content and Chapter 5
