Planet TYC 8998-760-1 c
| Name | TYC 8998-760-1 c | ||
| Planet Status | Confirmed | ||
| Discovered in | 2020 | ||
| Mass | 6.0 (± 1.0) MJ |  |
|
| Mass*sin(i) | — | ||
| Semi-Major Axis | 320.0 AU | |
|
| Orbital Period | — | ||
| Eccentricity | — | ||
| ω | — | ||
| Tperi | — | ||
| Radius | — | ||
| Inclination | — | ||
| Update | 2020-07-23 | ||
| Detection Method | Imaging | ||
| Mass Detection Method | Spectrum | ||
| 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
TYC 8998-760-1| Name | TYC 8998-760-1 | ||
| Distance | 94.6 (± 0.3) pc | ||
| Spectral type | K3IV | ||
| Apparent magnitude V | 11.13 | ||
| Mass | 1.0 (± 0.02) MSun | |
|
| Age | 0.0167 (± 0.0014) Gyr | |
|
| Effective temperature | 4573.0 (± 10.0) K | |
|
| Radius | — | ||
| Metallicity [Fe/H] | — | ||
| Detected Disc | — | ||
| Magnetic Field | — | ||
| RA2000 | 13:25:12.1 | ||
| Dec2000 | -64:56:21 | ||
| Alternate Names | |||
| Planetary system | 2 planets |
Related publications
Direct Imaging Spectroscopy of Two Jovian Exoplanets: Characterization of the TYC 8998-760-1 Multi-Planetary System
2021
WILCOMB K, PERRIN M., KONOPACKY Q. et al.
JWST GO Programme
abtract
The 12CO/13CO isotopologue ratio of a young, isolated brown dwarf. Possibly distinct formation pathways of super-Jupiters and brown dwarfs
2021
ZHANG Y., SNELLEN I. & MOLLIERE P.
Astron. & Astrophys., 656, A76
paper arxiv
Two Directly Imaged, Wide-orbit Giant Planets around the Young, Solar Analog TYC 8998-760-1
2020
BOHN A., KENWORTHY M., GINSKI Ch., RIEDER S., MAMAJEK E. et al.
ApJ. Letters, 898, L16
paper arxiv
The Young Suns Exoplanet Survey: Detection of a wide orbit planetary mass companion to a solar-type Sco-Cen member
2020
BOHN A., KENWORTHY M., GINSKI C., MANARA C., PECAUT M. et al.
MNRAS, 492, 431
paper arxiv
