Planet HD 3167 b
| Name | HD 3167 b | ||
| Planet Status | Confirmed | ||
| Discovered in | 2016 | ||
| Mass | 0.0158 ( -0.0012 +0.0012 ) MJ |  |
|
| Mass*sin(i) | — | ||
| Semi-Major Axis | 0.0186 ( -0.0003 +0.0003 ) AU | |
|
| Orbital Period | 0.959624 ( -2.8e-05 +2.8e-05 ) day | |
|
| Eccentricity | — | ||
| ω | — | ||
| Tperi | — | ||
| Radius | 0.152 ( -0.013 +0.016 ) RJ | |
|
| Inclination | 83.4 ( -7.7 +4.6 ) deg | |
|
| Update | 2022-03-09 | ||
| Detection Method | Primary Transit | ||
| Mass Detection Method | Radial Velocity | ||
| Radius Detection Method | Primary Transit | ||
| Primary transit | 2457394.37454 (± 0.00043) JD | |
|
| Secondary transit | — | ||
| λ | 6.6 ( -6.6 +7.9 ) deg | |
|
| Impact Parameter b | 0.39 ( -0.27 +0.28 ) | |
|
| Time Vr=0 | — | ||
| Velocity Semiamplitude K | 3.58 ( -0.26 +0.25 ) m/s | ||
| Calculated temperature | 1669.0 ( -52.0 +52.0 ) K | |
|
| Measured temperature | — | ||
| Hottest point longitude | — | ||
| Geometric albedo | — | ||
| Surface gravity log(g/gH) | — | ||
| Alternate Names | EPIC 220383386 b, HIP 2736 b, 2MASS J00345752+0422531 b, BD+03 68 b, EPIC 220383386.01, K2-96 b, SAO 109291 b, TYC 0013-00894-1 b, WISE J003457.60+042251.4 b |
Star
HD 3167| Name | HD 3167 | ||
| Distance | 47.36 ( -0.15 +0.15 ) pc | ||
| Spectral type | K0 V | ||
| Apparent magnitude V | 8.94 | ||
| Mass | 0.94 ( -0.04 +0.04 ) MSun | ||
| Age | 5.0 (± 4.0) Gyr | |
|
| Effective temperature | 5528.0 ( -162.0 +162.0 ) K | ||
| Radius | 0.87 ( -0.01 +0.01 ) RSun | ||
| Metallicity [Fe/H] | -0.02 ( -0.17 +0.17 ) | ||
| Detected Disc | — | ||
| Magnetic Field | — | ||
| RA2000 | 00:34:57.5 | ||
| Dec2000 | +04:22:53 | ||
| Alternate Names | EPIC 220383386, HIP 2736, 2MASS J00345752+0422531, BD+03 68, K2-96, SAO 109291, TYC 0013-00894-1, WISE J003457.60+042251.4 | ||
| Planetary system | 4 planets |
Observability Predictor 
Remarks
09 Mar 2022Bourrier et al. (2022) find a possible other value for λb:: -6.6 deg.
Related publications
A CHEOPS-enhanced view of the HD3167 system
2022
BOURRIER V., DELINE A., KRENN A., EGGER J., PETIT A. et al.
Astron. & Astrophys., 668, A31
paper arxiv
The Rossiter-McLaughlin effect Revolutions: an ultra-short period planet and a warm mini-Neptune on perpendicular orbits
2021
BOURRIER V., LOVIS Ch., CRETIGNIER M., ALLART R., DUMUSQUE X. et al.
Astron. & Astrophys., 654, A152
paper arxiv
A compositional link between stars and their rocky planets
2021
ADIBEKYAN V., DORN C., SOUSA S., SANTOS N., BITSCH B. et al.
Science, 374, 330
paper arxiv
A disk-driven resonance as the origin of high inclinations of close-in planets
2020
PETROVICH C., MUÑOZ D., KRATTER K. & MALHOTRA R.
ApJ, submitted
arxiv
Searching for volcanic activity and a Mercury-like exosphere of the super-Earth HD3167 b
2019
GUENTHER E. & KISLYAKOVA K.
MNRAS, 491, 3974
paper arxiv
Close-in sub-Neptunes reveal the past rotation history of their host stars: atmospheric evolution of planets in the HD3167 and K2-32 planetary systems
2019
KUBYSHKINA D., CUBILLOS P., FOSSATI L., ERKAEV N., JOHNSTONE C. et al.
ApJ, 879, 26
paper arxiv
Sixty Validated Planets from K2 Campaigns 5-8
2018
LIVINGSTON J., CROSSFIELD I., PETIGURA E., GONZALES E., CIARDI D. et l.
Astron. J., 156, 277
paper arxiv
Three's Company: An additional non-transiting super-Earth in the bright HD 3167 system, and masses for all three planets
2017
CHRISTIANSEN J., VANDERBURG A., BURT J., FULTON B., BATYGIN K. et al.
Astron. J., 154, 122
paper arxiv
The transiting multi-planet system HD3167: a 5.7 MEarth Super-Earth and a 8.3 MEarth mini-Neptune
2017
GANDOLFI D., BARRAGAN O., HATZES A., FRIDLUND M., FOSSATI L. et al.
Astron. J., 154, 123
paper arxiv
Two Small Planets Transiting HD 3167
2016
VANDERBURG, A., BIERYLA, A., DUEV, D., JENSEN-CLEM, R. LATHAM, D. & 8 additional authors
ApJL, 829, L9
arxiv
paper
ADS
