Planet HD 158259 c
| Name | HD 158259 c | ||
| Planet Status | Confirmed | ||
| Discovered in | 2019 | ||
| Mass | — | ||
| Mass*sin(i) | 0.01762 ( -0.00186 +0.0019 ) MJ |  |
|
| Semi-Major Axis | — | ||
| Orbital Period | 3.432 ( -0.00016 +0.0003 ) day | |
|
| Eccentricity | — | ||
| ω | — | ||
| Tperi | — | ||
| Radius | — | ||
| Inclination | — | ||
| Update | 2021-09-07 | ||
| Detection Method | Radial Velocity | ||
| Mass Detection Method | Spectrum | ||
| Radius Detection Method | — | ||
| Primary transit | — | ||
| Secondary transit | — | ||
| λ | — | ||
| Impact Parameter b | — | ||
| Time Vr=0 | — | ||
| Velocity Semiamplitude K | 2.261 ( -0.201 +0.189 ) m/s | |
|
| Calculated temperature | — | ||
| Measured temperature | — | ||
| Hottest point longitude | — | ||
| Geometric albedo | — | ||
| Surface gravity log(g/gH) | — | ||
| Alternate Names | — |
Star
HD 158259| Name | HD 158259 | ||
| Distance | 27.08 (± 0.01) pc | ||
| Spectral type | G0 | ||
| Apparent magnitude V | 6.46 | ||
| Mass | 1.08 (± 0.1) MSun | ||
| Age | — | ||
| Effective temperature | — | ||
| Radius | 1.21 ( -0.08 +0.03 ) RSun | ||
| Metallicity [Fe/H] | — | ||
| Detected Disc | — | ||
| Magnetic Field | — | ||
| RA2000 | 17:25:24.0 | ||
| Dec2000 | +52:47:26 | ||
| Alternate Names | |||
| Planetary system | 5 planets |
Related publications
Mean motion resonance capture in the context of type I migration
2023
KAJTAZI K., PETIT A. & JOHANSEN A.
Astron. & Astrophys., 669, A53
paper arxiv
The orbital evolution of resonant chains of exoplanets incorporating circularisation produced by tidal interaction with the central star with application to the HD 158259 and EPIC 245950175 systems
2021
PAPALOIZOU J.
Cel. Mech. & Dyn. Astron., accepted
arxiv
The SOPHIE search for northern extrasolar planets. XVI. HD 158259: A compact planetary system in a near-3:2 mean motion resonance chain
2020
HARA N., BOUCHY F., STALPORT M., BOISSE I., RODRIGUEZ J. et al.
Astron. & Astrophys., 636, L6
paper
