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 | 2012-01-13 | ||
| 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
Analysis of the Most Precise Light Curves of HAT-P-36 Detrended From Spot Signals
2021
YALCINKAYA S., BASTÜRK Ö., HELWEH F., ESMER E. et al.
Acta Astron., accepted
arxiv
Probing Transit Timing Variations of Three Hot-Jupiters: HATP-36b, HATP-56b, and WASP-52b
2021
SONBAS E., KARAMAN N., Özdönmez A., ER H., DHUGA K. et al.
MNRAS, in press
paper arxiv
Original Research By Young Twinkle Students (ORBYTS): Ephemeris Refinement of Transiting Exoplanets II
2020
EDWARDS B., ANISMAN L., CHANGEAT Q., MORVAN M., WRIGHT S. et al.
Res. Notes AAS, 4, 109
paper
arxiv
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
Precise photometric transit follow-up observations of five close-in exoplanets : update on their physical properties
2019
CHAKRABARTY A. & SENGUPTA S.
Astron. J., 158, 39
paper arxiv
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
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
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
The Exoplanet Handbook
2011
Michael Perryman
Content
Content and Chapter 5
