OGLE-TR-56 Overview
OGLE-TR-56
1.15
R⦿
6119.00
K
OGLE-TR-56 b
1.363
RJup
- Architecture
- OGLE-TR-56
- OGLE-TR-56
- Other Data
- Bibliography 18
- Exoplanet Archive Notes 2
- Nearby Data 4
Discovery Data
Host | Planet | Method | Year | Reference | Disposition |
---|---|---|---|---|---|
OGLE-TR-56 | OGLE-TR-56 b | Transit | 2002 | Konacki et al. 2003 | Confirmed Planet |
OGLE-TR-56
- Star is in a crowded field - possibly ambiguous TIC match. (TICv8)
- Inclination value and uncertainties estimated from range given in ref. (Bouchy et al. 2005)
- RA
- 17h56m35.51s
- Dec
- -29d32m21.2s
- Distance
- ---
- Parallax
- ---
- Ecliptic Latitude
- -6.10215 deg
- Ecliptic Longitude
- 269.25062 deg
- Galactic Latitude
- -2.3654 deg
- Galactic Longitude
- 0.70525 deg
- Total Proper Motion
- ---
- Proper Motion (RA)
- ---
- Proper Motion (Dec)
- ---
- Photometry
-
mV15.300
-
mTESS---
-
mGaia---
-
Abundances
(Hypatia Catalog) -
[Fe/H] 0.36±0.10 dex
-
[Na/H] 0.45±0.04 dex
-
[Mg/H] 0.23±0.07 dex
-
[Al/H] 0.40±0.06 dex
-
[Si/H] 0.35±0.05 dex
-
[Ca/H] 0.37±0.06 dex
Source | Gaia DR2 | Bonomo et al. 2017 | Mortier et al. 2013 | Southworth 2012 | Adams et al. 2011 | Southworth 2010 | Torres et al. 2008 | Pont et al. 2007 | Santos et al. 2006 | Bouchy et al. 2005 | Sasselov 2003 | Konacki et al. 2003 |
---|---|---|---|---|---|---|---|---|---|---|---|---|
Teff
(K)
|
5086.0+65.0-136.4
|
6050±100 | 6119±62 | 6119±62 | --- | 6119±62 | 6050±100 | 6119±62 | 6119±62 | 5970±150 | 5900±80 | 5900 |
Metallicity
(dex)
|
--- | 0.220±0.100 | 0.25±0.08 [Fe/H] | 0.25±0.08 [Fe/H] | --- | 0.25±0.08 [Fe/H] | --- | 0.25±0.08 | 0.25±0.08 | 0.17±0.19 [Fe/H] | --- | --- |
M✶
(M⦿)
|
--- |
1.228+0.072-0.078
|
1.30±0.13 | 1.339±0.101 | 1.228±0.078 | 1.233±0.045 | --- | 1.17±0.04 | 1.17±0.04 | 1.100±0.078 | 1.04±0.05 | 1.04±0.05 |
R✶
(R⦿)
|
0.8575266+0.0479326-0.0215056
|
1.363+0.089-0.086
|
1.48±0.43 | 1.737±0.045 | 1.363±0.089 | 1.26±0.14 | --- | 1.32±0.06 | 1.15±0.06 | 1.120±0.069 | 1.10±0.10 | 1.10±0.10 |
log g
(log10(cm/s2))
|
--- | --- | 4.21±0.19 | 4.086±0.019 | --- | 4.331±0.094 | --- | 4.21±0.19 | 4.21±0.19 | 4.20±0.38 | 4.5 | --- |
Sp. T
|
--- | --- | --- | --- | --- | --- | --- | --- | F8 V | --- | --- | --- |
γ
(km/s)
|
110.48601017744119±5.48033206599279 | --- | --- | --- | --- | --- | --- | --- | --- | -48.324±0.018 | --- | -49.49±0.02 |
v sin i
(km/s)
|
--- | 3.2±1.0 | --- | --- | --- | --- | --- | --- | --- | <5 | --- | 3 |
L✶
(log10(L⦿))
|
-0.35330468+0.00559333-0.00566632
|
--- | --- | --- | --- | --- | 0.350±0.085 | --- | --- | --- | --- | --- |
ρ✶
(g/cm3)
|
--- | --- | 0.26±0.01 | 0.361±0.015 | --- | 0.870±0.300 | --- | --- | --- | --- | --- | --- |
Age
(Gyr)
|
--- |
3.0+1.0-1.3
|
--- |
3.0+2.9-1.4
|
--- |
1.7+1.4-2.0
|
--- | --- | --- | --- | 3±1 | --- |
- Status
- Confirmed Planet
- Detected By
- Radial Velocity, Transit
Source | Torres et al. 2008 | Ivshina & Winn 2022 | Bonomo et al. 2017 | Southworth 2012 | Adams et al. 2011 | Southworth 2010 | Pont et al. 2007 | Santos et al. 2006 | Bouchy et al. 2005 | Konacki et al. 2003 |
---|---|---|---|---|---|---|---|---|---|---|
Mp
(M⨁)
|
441.77 +57.21-54.03
|
--- |
1049+1271-509
|
448±57 | 441.765±57.207 | 413.2±25.7 | 410±38 | 394±41 | 375±44 | 286±95 |
Mp
(MJup)
|
1.39 +0.18-0.17
|
--- |
3.3+4.0-1.6
|
1.41±0.18 | 1.39±0.18 | 1.300±0.081 | 1.29±0.12 | 1.24±0.13 | 1.18±0.14 | 0.90±0.30 |
Rp
(R⨁)
|
15.278+1.031-1.009
|
--- |
15.28+1.03-1.01
|
19.44±0.66 | 15.446±1.009 | 13.5±1.9 | 14.6±0.6 | 14.0±0.9 | 14.0±1.0 | 14.6±1.7 |
Rp
(RJup)
|
1.3630+0.0920-0.0900
|
--- |
1.363+0.092-0.090
|
1.734±0.059 | 1.378±0.090 | 1.20±0.17 | 1.30±0.05 | 1.25±0.08 | 1.25±0.09 | 1.30±0.15 |
e
|
--- | --- | <0.67 | --- | 0.0 | --- | --- | --- | 0 | 0 |
i
(deg)
|
77.60 +0.91-1.0
|
--- |
77.60+0.91-1.00
|
73.47±0.37 | 73.72±0.18 | 79.8±2.4 | --- | --- | 82±1 | 86±2 |
P
(days)
|
1.2119189 | 1.21191126±0.00000028 | 1.21191096±0.00000065 | 1.21191096±0.00000065 | 1.21191096±0.00000065 | 1.211909±0.000001 | 1.211909 | --- | 1.2119189 | 1.21190±0.00001 |
ρ
(g/cm3)
|
0.68 +0.18-0.14
|
--- |
1.59+2.00-0.81
|
0.336±0.042 | --- | 1.00±0.64 | --- | --- | --- | 0.5±0.3 |
K
(m/s)
|
225±27 | --- |
313.0+1100.0-69.0
|
212±22 | --- | 212±22 | --- | --- | 212±22 | 167±27 |
a
(au)
|
0.02383 +0.00046-0.00051
|
--- |
0.02385+0.00047-0.00049
|
0.02453±0.00062 | 0.01942±0.00015 | 0.02386±0.00029 | --- | --- | --- | 0.0225 |
TC
(days)
|
--- | 2454995.81093±0.00031 | 2453936.60070±0.00044 | --- | 2453936.60070±0.00044 | --- | 2453936.598 | --- | 2452075.1046 | 2452072.685±0.003 |
a/R✶
|
3.74 +0.19-0.15
|
--- | --- |
3.0377+0.0449-0.0437
|
--- |
4.082+0.485-0.392
|
3.84±0.16 | --- | --- | --- |
Teq
(K)
|
2212 +61-63
|
--- | --- | 2482±30 | --- | 2140±120 | --- | --- | --- | --- |
b
|
0.817 +0.016-0.031
|
--- | --- | --- | --- | --- | 0.80±0.02 | --- | 0.69 | --- |
Rp/R✶
|
0.1027±0.0019 | --- | --- | --- | --- | --- | 0.101±0.002 | --- | 0.114±0.004 | --- |
δ
(%)
|
0.9168 | --- | --- | --- | 1.080±0.008 | --- | --- | --- | --- | --- |
T14
(hours)
|
--- | --- | --- | --- | 2.2032±0.0096 | --- | --- | --- | --- | --- |
Literature Time Series
(2 File Types, 7 Files)
File Type | Data Points | Filter | Reference |
---|---|---|---|
Photometric Light Curve | 67 | R (Bessel) | Pont et al. 2007 |
Photometric Light Curve | 68 | V (Bessel) | Pont et al. 2007 |
Photometric Light Curve | 1113 | Ic (Cousins) | Udalski et al. 2004 |
Photometric Light Curve | 1113 | Ic (Cousins) | Udalski et al. 2002 |
Radial Velocity Curve | 11 | Optical Spectra | Torres et al. 2004 |
Radial Velocity Curve | 3 | Optical Spectra | Konacki et al. 2003 |
Radial Velocity Curve | 5 | Optical Spectra | Konacki et al. 2003 |
- Known Objects
- 1 Confirmed Planets
- 28 2MASS Point Source Catalog
- Data Files
- 2432 UKIRT Time Series
- 1 Associated Literature Data
-
TESS Transit Timing of Hundreds of Hot Jupiters
Ivshina & Winn 2022 | Reference Overview -
The Revised TESS Input Catalog and Candidate Target List
TICv8 | Reference Overview -
Gaia Data Release 2
Gaia DR2 | Reference Overview -
The GAPS Programme with HARPS-N at TNG . XIV. Investigating giant planet migration history via improved eccentricity and mass determination for 231 transiting planets
Bonomo et al. 2017 | Reference Overview -
New and updated stellar parameters for 90 transit hosts. The effect of the surface gravity
Mortier et al. 2013 | Reference Overview -
Homogeneous studies of transiting extrasolar planets - V. New results for 38 planets
Southworth 2012 | Reference Overview -
Twenty-one New Light Curves of OGLE-TR-56b: New System Parameters and Limits on Timing Variations
Adams et al. 2011 | Reference Overview -
Homogeneous studies of transiting extrasolar planets - III. Additional planets and stellar models
Southworth 2010 | Reference Overview -
Improved Parameters for Extrasolar Transiting Planets
Torres et al. 2008 | Reference Overview -
The "666" collaboration on OGLE transits. I. Accurate radius ofthe planets OGLE-TR-10b and OGLE-TR-56b with VLT deconvolutionphotometry
Pont et al. 2007 | Reference Overview -
High resolution spectroscopy of stars with transiting planets.The cases of OGLE-TR-10, 56, 111, 113, and TrES-1
Santos et al. 2006 | Reference Overview -
Doppler follow-up of OGLE transiting companions in the Galacticbulge
Bouchy et al. 2005 | Reference Overview -
The Optical Gravitational Lensing Experiment. Planetary and Low-Luminosity Object Transits in the Fields of Galactic Disk. Results of the 2003 OGLE Observing Campaigns
Udalski et al. 2004 | Reference Overview -
New Data and Improved Parameters for the Extrasolar Planet OGLE-TR-56
Torres et al. 2004 | Reference Overview -
High-Resolution Spectroscopic Follows-ups of OGLE Planetary Transit Candidates in the Galactic Bulge: Two Possible Jupiter-Mass Planets and Two Blends
Konacki et al. 2003 | Reference Overview -
The New Transiting Planet OGLE-TR-56b: Orbit and Atmosphere
Sasselov 2003 | Reference Overview -
An extrasolar planet that transits the disk of its parent star
Konacki et al. 2003 | Reference Overview -
The Optical Gravitational Lensing Experiment. Search for Planetary and Low- Luminosity Object Transits in the Galactic Disk. Results of 2001 Campaign -- Supplement
Udalski et al. 2002 | Reference Overview
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