Planet V396 Hya b
| Name | V396 Hya b | ||
| Planet Status | Confirmed | ||
| Discovered in | 2016 | ||
| Mass | 18.3 ( -12.2 +12.2 ) MJ | ||
| Mass*sin(i) | — | ||
| Semi-Major Axis | — | ||
| Orbital Period | — | ||
| Eccentricity | — | ||
| ω | — | ||
| Tperi | — | ||
| Radius | — | ||
| Inclination | 52.0 (± 27.0) deg |  |
|
| Update | 2019-05-17 | ||
| 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
V396 Hya| Name | V396 Hya | ||
| Distance | — | ||
| Spectral type | DD D | ||
| Apparent magnitude V | 17.3 | ||
| Mass | > 0.32 MSun | |
|
| Age | — | ||
| Effective temperature | — | ||
| Radius | — | ||
| Metallicity [Fe/H] | — | ||
| Detected Disc | — | ||
| Magnetic Field | — | ||
| RA2000 | 13:12:46.5 | ||
| Dec2000 | -23:21:32 | ||
| Alternate Names | |||
| Planetary system | 1 planet |
Observability Predictor 
Remarks
Kupfer et al. (2016) : the object is detected with Doppler tomogramsRelated publications
Close-in Exoplanets as Candidates of Strange Quark Matter Objects
2019
KUERBAN A., GENG J.-J., HUANG Y.-F., ZONG H.-Sh. & GONG H.
ApJ, submitted
arxiv
Comment on "Gravitational waves from ultra-short period exoplanets"
2018
WONG K., BERTI E., GABELLA W. & HOLLEY-BOCKELMANN K.
arxiv
UVES and X-Shooter spectroscopy of the emission line AM CVn systems GP Com and V396 Hya
2016
KUPFER, T., STEEGHS, D., GROOT, P. & 3 additional authors
MNRAS, 457, 1828
arxiv
paper
ADS
