TEPCat: HAT-P-11


 

This page summarises the information held within TEPCat for the transiting planetary system HAT-P-11. Please see here for descriptions of the quantities given below.

 

Discovery and basic observable quantities:
 
Quantity Value Unit
Reference of discovery paper 2010ApJ...710.1724B  
Date of discovery paper 2009 / 1 / 2 y / m / d
Data/telescope used for discovery HAT  
Right ascension 19 50 50.25 h m s
Declination +48 04 51.1 d m s
Right ascension (decimal) 297.70938 degrees
Declination (decimal) 48.08086 degrees
V-band apparent magnitude 9.47 mag
K-band apparent magnitude 7.01 mag
Transit duration 0.0980
( 2.352 )
day
hour
Transit depth 0.43 %
Time of mid-transit   2454957.813207 ± 0.000005     HJD or BJD
Orbital period 4.887802443 ± 0.000000032 days
Reference for orbital ephemeris   2017A+A...597A.113H  

 

Physical properties from the most recent detailed study:
 
Quantity Value Unit
Stellar effective temperature 4780 ± 50 K
Stellar metal abundance ([Fe/H] or [M/H])   +0.31 ± 0.05 dex
Stellar mass 0.802 ± 0.028   Msun
Stellar radius 0.683 ± 0.009 Rsun
Stellar logarithmic surface gravity 4.663 ± 0.012 c.g.s.
Stellar mean density 2.415 ± 0.097
( 3.41 ± 0.14 )
ρsun
g cm-3
Orbital eccentricity 0.2644 ± 0.0006  
Orbital semimajor axis   0.05259 ± 0.00062  AU
Planetary mass 0.0873 ± 0.0097
( 27.8 ± 3.1 )
Mjup
Mearth
Planetary radius 0.3890 ± 0.0053
( 4.360 ± 0.059 )
Rjup
Rearth
Planetary surface gravity 13.2 ± 1.1
3.12 ± 0.03
m/s2
log(cgs)
Planetary mean density 1.26 ± 0.12
( 1.67 ± 0.16 )
ρjup
g cm-3
Planetary equilibrium temperature 838 ± 10 K
Reference of detailed study 2018Sci...362.1384A  

 

Entries in the catalogue of orbital obliquity measurements:
 
Reference λ (degrees)
Winn et al. (2010)   103   + 26   - 10  
Hirano et al. (2010)   103   + 22   - 18  
Sanchis-Ojeda et al. (2011) solution 1   106   + 15   - 12  
Sanchis-Ojeda et al. (2011) solution 2   121   + 24   - 21  
Deming et al. (2011)almost polar orbit
Bourrier et al. (2023)   133.9   + 7.1   - 8.3  

 

 


Page generated on 2023/09/01           John Southworth   (Keele University, UK)