Planet HAT-P-36 b
| Name | HAT-P-36 b | ||
| Planet Status | Confirmed | ||
| Discovered in | 2012 | ||
| Mass | 1.832 ( -0.099 +0.099 ) MJ | ||
| Mass*sin(i) | — | ||
| Semi-Major Axis | 0.0238 (± 0.0004) AU |  |
|
| Orbital Period | 1.327347 (± 3e-06) day | |
|
| Eccentricity | 0.063 (± 0.032) | |
|
| ω | 95.0 (± 63.0) deg | |
|
| Tperi | — | ||
| Radius | 1.264 ( -0.071 +0.071 ) RJ | |
|
| Inclination | 86.0 (± 1.3) deg | |
|
| Update | 2012-01-14 | ||
| Detection Method | Primary Transit | ||
| Mass Detection Method | — | ||
| Radius Detection Method | — | ||
| Primary transit | 2455565.18144 (± 0.0002) JD | |
|
| 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
HAT-P-36| Name | HAT-P-36 | ||
| Distance | 317.0 (± 17.0) pc | |
|
| Spectral type | — | ||
| Apparent magnitude V | 12.26 | ||
| Mass | 1.022 (± 0.049) MSun | |
|
| Age | 6.6 ( -1.8 +1.8 ) Gyr | |
|
| Effective temperature | 5580.0 (± 100.0) K | |
|
| Radius | 1.096 (± 0.056) RSun | |
|
| Metallicity [Fe/H] | 0.26 (± 0.08) | |
|
| Detected Disc | — | ||
| Magnetic Field | — | ||
| RA2000 | 12:33:03.0 | ||
| Dec2000 | +44:54:55 | ||
| Alternate Names | |||
| Planetary system | 1 planet |
Related publications
Transiting Exoplanet Monitoring Project (TEMP). V. Transit Follow Up for HAT-P-9b, HAT-P-32b, and HAT-P-36b
2019
WANG Y.-H., WANG S., HINSE T., WU Zh.-Y., DAVIS A. et al.
Astron. J., 157, 82
paper
Orbital decay of hot Jupiters due to nonlinear tidal dissipation within solar-type hosts
2016
ESSICK R. & WEINBERG N.
ApJ, 216, 18
paper arxiv
ADS
The GAPS Programme with HARPS-N at TNG VIII: Observations of the Rossiter-McLaughlin effect and characterisation of the transiting planetary systems HAT-P-36 and WASP-11/HAT-P-10
2015
MANCINI L., ESPOSITO M., COVINO E., RAIA G., SOUTHWORTH et al.
Astron. & Astrophys;, submitted
arxiv
HAT-P-34b -- HAT-P-37b: Four Transiting Planets More Massive Than Jupiter Orbiting Moderately Bright Stars
2012
BAKOS G., HARTMAN J., TORRES G., BEKY B., LATHAM D. & 21 additional authors
Astron. J., 144, 19
paper arxiv
A Uniformly Derived Catalogue of Exoplanets from Radial Velocities
2012
HOLLIS M., BALAN S., LEVER G. & LAHAV O.
MNRAS, 423, Issue 3, 2800-2814
paper arxiv
The Exoplanet Handbook
2011
Michael Perryman
Content
Content and Chapter 5
