Planet HIP 41378 g
| Name | HIP 41378 g | ||
| Planet Status | Candidate | ||
| Discovered in | 2019 | ||
| Mass | — | ||
| Mass*sin(i) | 0.022 (± 0.0047) MJ |  |
|
| Semi-Major Axis | 0.3227 (± 0.0036) AU | |
|
| Orbital Period | 62.06 (± 0.32) day | |
|
| Eccentricity | 0.06 ( -0.04 +0.06 ) | |
|
| ω | — | ||
| Tperi | — | ||
| Radius | — | ||
| Inclination | — | ||
| Update | 2022-03-16 | ||
| Detection Method | Radial Velocity | ||
| Mass Detection Method | TTV | ||
| Radius Detection Method | — | ||
| Primary transit | — | ||
| Secondary transit | — | ||
| λ | — | ||
| Impact Parameter b | — | ||
| Time Vr=0 | — | ||
| Velocity Semiamplitude K | — | ||
| Calculated temperature | 605.0 (± 4.7) K | ||
| Measured temperature | — | ||
| Hottest point longitude | — | ||
| Geometric albedo | — | ||
| Surface gravity log(g/gH) | — | ||
| Alternate Names | — |
Star
HIP 41378| Name | HIP 41378 | ||
| Distance | 116.0 (± 18.0) pc | |
|
| Spectral type | |||
| Apparent magnitude V | 8.9 | ||
| Mass | 1.15 (± 0.064) MSun | |
|
| Age | — | ||
| Effective temperature | 6199.0 (± 50.0) K | |
|
| Radius | 1.4 (± 0.19) RSun | |
|
| Metallicity [Fe/H] | -0.11 (± 0.08) | |
|
| Detected Disc | — | ||
| Magnetic Field | — | ||
| RA2000 | 08:26:28.0 | ||
| Dec2000 | +10:04:49 | ||
| Alternate Names | |||
| Planetary system | 5 planets |
Observability Predictor 
Remarks
Santerne et al. 2019 : The planet mass assumes an inclination of 88°Related publications
An extremely low-density and temperate giant exoplanet
2019
SANTERNE A., KOSIAREK M., DAI F., DRESSING C., DUMUSQUE X. et al.
Nature Astronomy, submitted
arxiv
Five Planets Transiting a Ninth Magnitude Star
2016
VANDERBURG A., BECKER J., KRISTIANSEN M., BIERYLA A., DUEV D. et al.
ApJ Letters, 827, L10
arxiv
paper
ADS
