Planet HIP 67522 b
| Name | HIP 67522 b | ||
| Planet Status | Confirmed | ||
| Discovered in | 2020 | ||
| Mass | 5.0 ( -5.0 +0.0 ) MJ |  |
|
| Mass*sin(i) | — | ||
| Semi-Major Axis | — | ||
| Orbital Period | 6.959503 (± 1.6e-05) day | ||
| Eccentricity | 0.059 ( -0.046 +0.193 ) | ||
| ω | 343.0 ( -140.0 +92.0 ) deg | ||
| Tperi | — | ||
| Radius | 0.8984 (± 0.0419) RJ | ||
| Inclination | 89.34 ( -0.54 +0.45 ) deg | ||
| Update | 2021-09-10 | ||
| Detection Method | Primary Transit | ||
| Mass Detection Method | — | ||
| Radius Detection Method | Primary Transit | ||
| Primary transit | 2458604.02371 (± 0.00037) JD | ||
| Secondary transit | — | ||
| λ | 5.1 ( -3.7 +2.5 ) deg | |
|
| Impact Parameter b | — | ||
| Time Vr=0 | — | ||
| Velocity Semiamplitude K | — | ||
| Calculated temperature | 1174.0 (± 21.0) K | ||
| Measured temperature | — | ||
| Hottest point longitude | — | ||
| Geometric albedo | — | ||
| Surface gravity log(g/gH) | — | ||
| Alternate Names | — |
Star
HIP 67522| Name | HIP 67522 | ||
| Distance | 127.27 (± 1.0) pc | |
|
| Spectral type | — | ||
| Apparent magnitude V | 9.9 | ||
| Mass | 1.22 (± 0.05) MSun | |
|
| Age | 0.017 (± 0.002) Gyr | |
|
| Effective temperature | 5675.0 K | |
|
| Radius | 1.38 (± 0.06) RSun | |
|
| Metallicity [Fe/H] | — | ||
| Detected Disc | — | ||
| Magnetic Field | — | ||
| RA2000 | 13:50:06.0 | ||
| Dec2000 | -40:50:09 | ||
| Alternate Names | |||
| Planetary system | 1 planet |
Related publications
Characterizing Undetected Stellar Companions with Combined Datasets
2021
WOOD M., MANN A. & KRAUS A.
Astron. J., 162, 128
paper arxiv
The obliquity of HIP 67522 b: a 17 Myr old transiting hot Jupiter-sized planet
2021
HEITZMANN A., ZHOU G., QUINN S., MARSDEN S., WRIGHT D. et al.
ApJ. Letters, 922, L1
paper arxiv
The Atmosphere of a 17Myr Old Hot Jupiter
2021
MANN A. et al.
JWST GO Programme
arxiv
TESS Hunt for Young and Maturing Exoplanets (THYME) II: A 17 Myr Old Transiting Hot Jupiter in the Sco-Cen Association
2020
RIZZUTO A., NEWTON E., MANN A., TOFFLEMIRE B., VANDERBURG A. et al.
Astron. J., 160, 33
paper arxiv
