TEPCat: Orbital obliquity observations for transiting planetary systems


 

This table catalogues measurements of orbital obliquity for the known (published) transiting extrasolar planetary systems. This effect is normally observed spectroscopically (usually via radial velocity measurements) but can be obtained photometrically, by analysis of starspot crossing events during transits.

The radial-velocity anomaly known as the Rossiter-McLaughlin effect was originally predicted by Holt (1893) and observed (but not definitively) in the eclipsing binary star systems δ Librae (Schlesinger 1910) and λ Tauri (Schlesinger 1916). It was subsequently described and clearly demonstrated by Rossiter (1924) for β Lyrae and McLaughlin (1924) for β Persei. The designation "Rossiter-McLaughlin effect" arose from the latter two papers.

All known orbital obliquity constraints are included. Many systems have multiple measurements, often resulting from the same data. In these cases the most recent is normally the most reliable but it is important to check the published papers to be sure. I indicate the preferred value for each object using the "Pflag" column in the ASCII and CSV files (not in the HTML table below). Pflag is set to "y" for the best value for a given object, and to "n" for all other values for this object.

The quantity most commonly observed is the sky-projected angle between the axes of the stellar rotation and the planetary orbit. This quantity is normally called the sky-projected obliquity and denoted λ. There is an alternative definition of the co-ordinate system which yields the value β instead. The two quantities are related by   λ = -β   i.e. one is the negative value of the other.

The orbital obliquity is more difficult to determine than the sky-projected orbital obliquity, and only a few measurements exist. This quantity is called ψ and it is always closer to 90 degrees than λ:
ψ ≥ |λ|   for λ < 90 degrees
ψ ≤ |λ|   for λ > 90 degrees
This means that objects with a constraint on λ also have a constraint on ψ, but this is often not given explicitly.

Click here for details of the quantities and their units
Click here for the table in machine-readable ASCII format
Click here for the table in machine-readable CSV format
Click here to return to the TEPCat main page

 

System Teff (K) λ (degrees) ψ (degrees) Reference
55 Cnc e5172 ± 18   72.4   + 12.7   - 11.5  
indeterminate
  10   + 17   - 20  


  23   + 14   - 12  
Bourrier & Hébrard (2014)
López-Morales et al. (2014)
Zhao et al. (2023)
AU Mic b3700 ± 100   −4.7   + 6.8   - 6.4  
  −0.1   + 5.1   - 5.0  
  −3.0   + 10.4   - 10.3  
  5   + 16   - 15  




Hirano et al. (2020)
Martioli et al. (2021)
Palle et al. (2020)
Addison et al. (2021)
CoRoT-15950 ± 150   77   ±   11  

Pont et al. (2010)
CoRoT-25598 ± 50   7.2   ±   4.5  
  4.7   ±   12.3  
  −1.0   + 6.0   - 7.7  
  4.0   + 5.9   - 6.1  




Bouchy et al. (2008)
Nutzmann et al. (2011)
Czesla et al. (2012)
Gillon et al. (2010)
CoRoT-36558 ± 44   −37.6   + 22.3   - 10.0  

Triaud et al. (2009)
CoRoT-116343 ± 72 prograde
  0.1   ±   2.6  


Gandolfi et al. (2010)
Gandolfi et al. (2012)
CoRoT-185440 ± 100   −10   ±   20  
  20   ±   20  
Hébrard et al. (2011)
CoRoT-196090 ± 70   −52   + 27   - 22  

Guenther et al. (2012)
CoRoT-366730 ± 140   275.8   ±   11.3  

Sebastian et al. (2022)
DS Tuc5598
+ 28 − 59
  2.93   + 0.88   - 0.87  
  12.1   + 2.6   - 2.1  


Zhou et al. (2020)
Benatti et al. (2021)
GJ 4363416 ± 54   72   + 33   - 24  
  114   + 23   - 17  
  80   + 21   - 18  
  103   + 13   - 12  
Bourrier et al. (2018)
Bourrier et al. (2022)
GJ 34703725 ± 54   101   + 29   - 14  
  97   + 16   - 11  
Stefánsson et al. (2022)
HAT-P-15975 ± 50   3.7   ±   2.1  

Johnson et al. (2008)
HAT-P-26290 ± 60   1.2   ±   13.4  
  0.2   + 12.2   - 12.5  
  9   ±   10  



Winn et al. (2007)
Loeillet et al. (2008)
Albrecht et al. (2012)
HAT-P-35190 ± 80   21.2   ±   8.7  
  −25.3   + 29.4   - 22.8  

  75.7   + 8.5   - 7.9  
Mancini et al. (2018)
Bourrier et al. (2023)
HAT-P-46036 ± 46   −4.9   ±   11.9  

Winn et al. (2011)
HAT-P-66570 ± 80   166   ±   10  
  165   ±   6  


Hébrard et al. (2011)
Albrecht et al. (2012)
HAT-P-76310 ± 15   182.5   ±   9.4  
  −132.6   + 10.5   - 16.3  
  155   ±   37  
  220.3   + 8.2   - 9.3  

  142   + 12   - 16  
  136   + 16   - 22  

  94.6   + 5.5   - 3.0  


  115   + 19   - 16  
  97   ±   14  
  101   ±   2  
  87   ±   2  
  116.4   + 30.2   - 14.7  
Winn et al. (2009)
Narita et al. (2009)
Albrecht et al. (2012)
Benomar et al. (2014)
Lund et al. (2014)
Masuda (2015) solution 1
Masuda (2015) solution 2
Campante et al. (2016)
HAT-P-86200 ± 80   −9.7   + 9.0   - 7.7  
  −17   + 9.2   - 11.5  


Simpson et al. (2011)
Moutou et al. (2011)
HAT-P-96350 ± 150   −16   ±   8  

Moutou et al. (2011)
HAT-P-114780 ± 50   103   + 26   - 10  
  103   + 22   - 18  
  106   + 15   - 12  
  121   + 24   - 21  
almost polar orbit
  133.9   + 7.1   - 8.3  


  106   + 15   - 11  
  97   + 8   - 4  

  104.9   + 8.6   - 9.1  
Winn et al. (2010)
Hirano et al. (2011)
Sanchis-Ojeda et al. (2011) solution 1
Sanchis-Ojeda et al. (2011) solution 2
Deming et al. (2011)
Bourrier et al. (2023)
HAT-P-124665 ± 45   −54   + 41   - 13  

Mancini et al. (2018)
HAT-P-135653 ± 90   1.9   ±   8.6  

Winn et al. (2010)
HAT-P-146600 ± 90   189.1   ±   5.1  

Winn et al. (2011)
HAT-P-155620 ± 20   13   ±   6  

Mancini et al. (2022)
HAT-P-166140 ± 72   −10   ±   16  
  −2   + 55   - 46  


Moutou et al. (2011)
Albrecht et al. (2012)
HAT-P-175350 ± 20   19   + 14   - 16  
  −27.5   ±   6.7  


Fulton et al. (2013)
Mancini et al. (2022)
HAT-P-184870 ± 50   132   ±   15  

Esposito et al. (2014)
HAT-P-204595 ± 45   −8.0   ±   6.9  
  36   + 10   - 12  
Esposito et al. (2017)
HAT-P-215695 ± 45   −0.7   ±   12.5  

Mancini et al. (2022)
HAT-P-225314 ± 50   −2.1   ±   3.0  
  24   ±   18  
Mancini et al. (2018)
HAT-P-235885 ± 72   15   ±   22  

Moutou et al. (2011)
HAT-P-246373 ± 80   20   ±   16  

Albrecht et al. (2012)
HAT-P-275316 ± 55   24.2   + 76.0   - 44.5  

Brown et al. (2012)
HAT-P-296140 ± 30   −26   ±   16  

Mancini et al. (2022)
HAT-P-306338 ± 42   73.5   ±   9.0  
  70.5   + 2.9   - 2.8  


Johnson et al. (2011)
Cegla et al. (2023)
HAT-P-326269 ± 64   85   ±   1.5  

Albrecht et al. (2012)
HAT-P-336446 ± 88   −5.9   ±   4.1  

Bourrier et al. (2023)
HAT-P-346442 ± 88   0   ±   14  

Albrecht et al. (2012)
HAT-P-365620 ± 40   −14   ±   18  
  0   + 63   - 0  
Mancini et al. (2015)
HAT-P-416390 ± 100   −22.1   + 0.8   - 6.0  

Johnson et al. (2017)
HAT-P-496820 ± 52   −97.7   ±   1.8  

Bourrier et al. (2023)
HAT-P-566566 ± 50   8   ±   2  

Zhou et al. (2016)
HAT-P-676406
+ 65 − 61
  2.2   ±   0.4  

Sicilia et al. (2024)
HAT-P-697724
+ 250 − 360
  30.3   + 6.1   - 7.3  

Zhou et al. (2019)
HAT-P-708450 ± 195   113.1   + 5.1   - 3.4  
  107.9   + 2.0   - 1.7  


Zhou et al. (2019)
Bello-Arufe et al. (2022)
HATS-25227 ± 95   8   ±   8  
  3   ±   18  

  38   ±   27  
Mohler-Fischer et al. (2013)
Biagiotti et al. (2024)
HATS-36351 ± 76   3   ±   25  

Addison et al. (2014)
HATS-145346 ± 60   76   + 4   - 5  

Zhou et al. (2015)
HATS-707930 ± 180   8.9   + 5.6   - 4.5  

Zhou et al. (2019)
HD 3167b5300 ± 73   −6.6   + 6.6   - 7.9  
  29.5   + 7.2   - 9.4  
Bourrier et al. (2021)
HD 3167c5300 ± 73   −98   ±   23  
  −108.9   + 5.4   - 5.5  

  107.7   + 5.1   - 4.9  
Dalal et al. (2019)
Bourrier et al. (2021)
HD 171566046
+ 76 − 72
  62   ±   25  
  9.4   ±   9.3  
  −4.8   ±   5.3  
  10.0   ±   5.1  




Narita et al. (2008)
Cochran et al. (2008)
Barbieri et al. (2009)
Narita et al. (2009)
HD 63433b5700
+ 76 − 75
  8.0   + 33.0   - 45.0  

Mann et al. (2020)
HD 806065584 ± 13 prograde
  50   + 61   - 36  
  53   + 34   - 21  
  42   ±   8  




Moutou et al. (2009)
Pont et al. (2009)
Winn et al. (2009)
Hébrard et al. (2010)
HD 106315c6364 ± 87   −10.9   + 3.6   - 3.8  
  −2.7   + 2.7   - 2.6  


Zhou et al. (2018)
Bourrier et al. (2023)
HD 1490266147 ± 50   −12   ±   15  
  12   ±   7  


Wolf et al. (2007)
Albrecht et al. (2012)
HD 1897334969 ± 43   −1.4   ±   1.1  
  0.85   + 0.28   - 0.32  
  −0.50   ±   0.30  

  −0.4   ±   0.2  
  −0.31   + 0.18   - 0.17  
  −1.00   + 0.22   - 0.23  



  4   + 18   - 4  
  7   + 12   - 4  

  13.6   ±   6.9  
Winn et al. (2006)
Triaud et al. (2009)
Collier Cameron et al. (2010)
Dumusque (2014)
Cegla et al. (2016)
Casasayas-Barris et al. (2017)
Cristo et al. (2023)
HD 2094586117 ± 50   3.9   + 18   - 21  
  −4.4   ±   1.4  
  −5   ±   7  
  0.6   ±   0.4  
  1.58   ±   0.08  





Queloz et al. (2000)
Winn et al. (2005)
Albrecht et al. (2012)
Santos et al. (2020)
Casasayas-Barris et al. (2021)
HD 3322316089
+ 97 − 96
  −42   ±   11  
  −2   ±   6  


Sedaghati et al. (2022)
Knudstrup & Albrecht (2022)
HIP 675225675 ± 75   −5.8   + 2.8   - 5.7  
  20.2   + 10.3   - 8.7  
Heitzmann et al. (2021)
K2-25b3207 ± 58   1.7   + 5.8   - 3.7  
  3   ±   16  

  17   + 11   - 8  
Gaidos et al. (2020)
Stefansson et al. (2020)
K2-295358 ± 38   1.5   ±   8.7  

Santerne et al. (2016)
K2-333540 ± 70   −10   + 22   - 24  

Hirano et al. (2024)
K2-346131 ± 47   −1   + 10   - 9  

Hirano et al. (2016)
K2-93d6320
+ 60 − 30
  57   + 26   - 18  

Grouffal et al. (2022)
K2-1055430 ± 70   −81   + 50   - 47  

Bourrier et al. (2023)
K2-1405654 ± 55   0.5   ±   9.7  

Rice et al. (2021)
K2-2326154 ± 60   −11.1   ±   6.6  

Wang et al. (2021)
K2-2345622
+ 70 − 71
  74   + 34   - 33  
  80   + 22   - 23  
Bourrier et al. (2023)
K2-2676189
+ 47 − 52
  −1.48   ±   0.85  
  3.4   + 3.5   - 1.6  
Yu et al. (2018)
K2-290b6302 ± 120   173   + 45   - 53  

Hjorth et al.(2021)
K2-290c6302 ± 120   153   ±   8  
  124   ±   6  
Hjorth et al.(2021)
KELT-16471
+ 50 − 49
  2   ±   16  

Siverd et al. (2012)
KELT-66246 ± 88   −36   ±   11  

Damasso et al. (2015)
KELT-76699 ± 24   9.7   ±   5.2  
  2.7   ±   0.6  
  −10.55   ±   0.27  


  12.4   ±   11.7  
Bieryla et al. (2015)
Zhou et al. (2016)
Tabernero et al. (2022)
KELT-99329 ± 118   −84.8   ±   1.4  
  −85.78   ±   0.46  
  −85.01   ±   0.23  
  −88   ±   15  
  −84.8   ±   0.3  



  87   + 10   - 11  
  87.47   + 0.18   - 0.19  
Gaudi et al. (2017)
Borsa et al. (2019)
Wyttenbach et al. (2020)
Ahlers et al. (2020)
Stephen et al. (2022)
KELT-105948 ± 74   −5.2   ±   3.4  

Steiner et al. (2023)
KELT-115375 ± 25   −77.9   + 2.4   - 2.3  

Mounzer et al. (2022)
KELT-177454 ± 49   −115.9   ±   4.1  
  116   ±   4  
Zhou et al. (2016)
KELT-197500 ± 110   −179.7   + 3.7   - 3.8  
  −179.7   + 3.7   - 3.8  

  155   + 17   - 21  
Siverd et al. (2018)
Kawai et al. (2024)
KELT-208652 ± 160   3.4   ±   2.1  
  0.6   ±   4  
  1.6   ±   3.1  
  3.9   ±   1.1  



  5   ±   11  
Lund et al. (2017)
Talens et al. (2018)
Hoeijmakers et al. (2020)
Singh et al. (2024)
KELT-217598
+ 81 − 84
  −5.6   + 1.7   - 1.9  

Johnson et al. (2018)
KELT-246508 ± 49   2.6   + 5.1   - 3.6  
  1.2   + 8.2   - 7.4  


Rodriguez et al. (2019)
Hjorth et al. (2019)
Kepler-86213 ± 150   −26.4   ±   10.1  
  5   ±   7  


Jenkins et al. (2010)
Albrecht et al. (2012)
Kepler-9b5774 ± 60   −13   ±   16  

Wang et al. (2018)
Kepler-137650 ± 250   23   ±   4  
  58.6   ±   2  
  58.6   ±   2  
  59.20   ±   0.05  
  −27.9   ±   1.1  


  60   ±   2  
  60.25   ±   0.05  

Barnes et al. (2011)
Johnson et al. (2014)
Masuda (2015)
Howarth & Morello (2017)
Herman et al. (2018)
Kepler-175781 ± 85   0   ±   15  
  0   ±   15  
Désert et al. (2011)
Kepler-25c6270 ± 79   −0.5   ±   5.7  
  9.4   ±   7.1  

  −0.9   + 7.7   - 6.4  

  26.9   + 7.0   - 9.2  
  12.6   + 6.7   - 11.0  
  24.1   + 9.29   - 9.3  
Albrecht et al. (2013)
Benomar et al. (2014)
Campante et al. (2016)
Bourrier et al. (2023)
Kepler-30b5498 ± 54   4   ±   10  
  −1   ±   10  


Sanchis-Ojeda et al. (2012) method 1
Sanchis-Ojeda et al. (2012) method 2
Kepler-50b6225 ± 66 aligned

Chaplin et al. (2013)
Kepler-50c6225 ± 66 aligned

Chaplin et al. (2013)
Kepler-56b4840 ± 97 misaligned

Huber et al.(2013)
Kepler-56c4840 ± 97 misaligned

Huber et al.(2013)
Kepler-635576 ± 50   −110   + 22   - 14  
  −135   + 21   - 27  
  104   + 9   - 14  
  115   + 17   - 13  
Sanchis-Ojeda et al. (2013)
Bourrier et al. (2023)
Kepler-65b6211 ± 66 aligned

Chaplin et al. (2013)
Kepler-65c6211 ± 66 aligned

Chaplin et al. (2013)
Kepler-65d6211 ± 66 aligned

Chaplin et al. (2013)
Kepler-89d6182 ± 82   −6   + 13   - 11  
  −11   ±   11  


Hirano et al. (2012)
Albrecht et al. (2013)
Kepler-4086088 ± 65
  48   + 4   - 5  
Kamiaka et al. (2019)
Kepler-4205520 ± 80   74   + 32   - 46  

Santerne et al. (2014)
Kepler-4486820 ± 120   12.6   + 3.0   - 2.9  
  −7.1   + 4.2   - 2.8  


Bourrier et al. (2015)
Johnson et al. (2017)
MASCARA-17554 ± 150   69.5   ±   3  
  69.2   + 3.1   - 3.4  

  72.1   + 2.5   - 2.4  
Talens et al. (2017)
Hooton et al. (2022)
MASCARA-47810 ± 165   247.5   + 1.5   - 1.7  
  244   ±   15  
  250.34   ±   0.14  

  104   + 7   - 13  

Dorval et al. (2020)
Ahlers et al. (2020)
Zhang et al. (2022)
NGTS-26450 ± 50   −11.3   ±   4.8  

Anderson et al. (2018)
Qatar-14820 ± 85   −8.4   ±   7.1  

Covino et al. (2013)
Qatar-24645 ± 50   4.3   ±   4.5  
  0   ±   8  
  0   ±   10  
  15   ±   20  



  0   + 43   - 0  
Mancini et al. (2014)
Mocnik et al. (2017)
Dai et al. (2017)
Esposito et al. (2017)
Qatar-65063 ± 42   0.1   ±   2.6  
  22   + 9   - 18  
Rice et al. (2023)
TOI-1136d5770 ± 50   5   ±   5  
  0   + 28   - 0  
Dai et al. (2023)
TOI-12685257 ± 40   40.0   + 7.2   - 9.9  

Dong et al. (2022)
TOI-14317690
+ 400 − 250
  −155   + 20   - 10  

Stangret et al. (2021)
TOI-14785597
+ 83 − 82
  6.2   + 5.9   - 5.5  

Rice et al. (2022)
TOI-15187300 ± 100   240.34   + 0.93   - 0.98  
  −118.96   + 0.68   - 0.65  
  −117.24   + 0.64   - 0.69  



Cabot et al. (2021)
Watanabe et al. (2024) 2020 data
Watanabe et al. (2024) 2023 data
TOI-1670c6170 ± 61   −0.3   ±   2.2  

Lubin et al. (2023)
TOI-18426230 ± 50   −68   + 21   - 15  
  73   + 16   - 13  
Hixenbaugh et al. (2023)
TOI-18596341
+ 68 − 70
  38.9   + 2.8   - 2.7  

Dong et al. (2023)
TOI-19375814
+ 91 − 93
  4.0   ±   3.5  

Yee et al. (2023)
TOI-20255880 ± 53   9   + 36   - 34  

Knudstrup et al. (2022)
TOI-2076b5187
+ 54 − 53
  −3   + 15   - 16  
  18   + 10   - 9  
Frazier et al. (2023)
TOI-21096530
+ 160 − 150
  1.7   ±   1.7  

Wong et al. (2021)
TOI-33626800 ± 100   1.2   + 2.8   - 2.7  

Espinoza-Retamal et al. (2023)
TOI-38843180 ± 88   75   ±   10  

Libby-Roberts et al.(2023)
TOI-46416560
+ 300 − 340
  1.41   ±   0.76  
  2.4   ±   1.3  
Bieryla et al.(2024)
TOI-5126b6150
+ 110 − 130
  1   ±   48  

Radzom et al.(2024)
TOI-5398b6000 ± 75   3.0   + 6.8   - 4.2  
  −24   + 14   - 13  
  13.2   ±   8.2  

Mantovan et al.(2024)
Radzom et al.(2024)
TOI-6406460
+ 130 − 150
  184   ±   3  
  104   ±   2  
Knudstrup et al. (2023)
TOI-6776295 ± 80   0.3   ±   1.3  
  3.2   + 1.6   - 1.5  


Sedaghati et al. (2023)
Hu et al. (2024)
TOI-7786643 ± 150   18   ±   11  

Clark et al. (2023)
TOI-858B5842
+ 84 − 79
  99.3   + 3.8   - 3.7  

Hagelberg et al. (2023)
TOI-942b4928
+ 125 − 85
  1   + 41   - 33  
  2   + 27   - 33  
Wirth et al. (2021)
TRAPPIST-1b2566 ± 26   15   + 26   - 30  

Hirano et al.(2020)
TRAPPIST-1e2566 ± 26   9   + 45   - 51  

Hirano et al.(2020)
TRAPPIST-1f2566 ± 26   21   ±   32  

Hirano et al.(2020)
TrES-15226 ± 50   30   ±   21  

Narita et al. (2007)
TrES-25850 ± 50   −9   ±   12  

Winn et al. (2008)
TrES-46295 ± 65   6.3   ±   4.7  

Narita et al. (2010)
V1298 Tau b5050 ± 100   2   + 12   - 4  
  15   + 15   - 16  
  4   + 7   - 10  


  8   + 4   - 7  
Gaidos et al. (2022) LPVs
Gaidos et al. (2022) RV
Johnston et al. (2021)
V1298 Tau c5050 ± 100   4.9   + 15.0   - 15.1  

Feinstein et al. (2021)
WASP-16160 ± 64   −79.0   + 4.5   - 4.3  
  −59   + 99   - 26  


Simpson et al. (2011)
Albrecht et al. (2011)
WASP-25170 ± 60   −153   + 15   - 11  
indeterminate


Triaud et al. (2010)
Albrecht et al. (2011)
WASP-36340 ± 90   15   + 10   - 9  
  3.3   + 2.5   - 4.4  
  5   + 6   - 5  
  20.0   ±   3.3  




Simpson et al. (2010)
Tripathi et al. (2010)
Miller et al. (2010)
Oshagh et al. (2013)
WASP-45540 ± 55   4   + 34   - 43  
  −1   + 14   - 12  


Triaud et al. (2010)
Sanchis-Ojeda et al. (2011)
WASP-55770 ± 65   12.1   + 8.0   - 10.0  
  7.2   ±   9.5  


Triaud et al. (2010)
Fukui et al. (2011)
WASP-65375 ± 65   −11   + 18   - 14  
  7.2   ±   3.7  


Gillon et al. (2009)
Tregloan-Reed et al. (2015)
WASP-76520 ± 70   86   ±   6  

Albrecht et al. (2012)
WASP-85690 ± 36   −123.3   + 3.4   - 4.4  
  −143.0   + 1.6   - 1.5  


Queloz et al. (2010)
Bourrier et al. (2017)
WASP-114900 ± 65   7   ±   5  

Mancini et al. (2015)
WASP-126265 ± 50   59   + 15   - 20  

Albrecht et al. (2012)
WASP-136025 ± 21   8   + 13   - 12  

Brothwell et al. (2014)
WASP-146462 ± 75   −14   + 21   - 13  
  −33.1   ±   7.4  


Joshi et al. (2009)
Johnson et al. (2009)
WASP-156573 ± 70   −139.6   + 4.3   - 5.2  

Triaud et al. (2010)
WASP-165630 ± 70   −4.2   + 11.0   - 13.9  
  11   + 26   - 19  


Brown et al. (2012)
Albrecht et al. (2012)
WASP-176550 ± 100   −147   + 49   - 11  
  167.4   ±   11.2  
  −148.5   + 4.2   - 5.4  
  −148.7   + 7.7   - 6.7  




Anderson et al. (2010)
Bayliss et al. (2010)
Triaud et al. (2010)
Anderson et al. (2011)
WASP-186400 ± 70   4.0   ±   5.0  
  13   ±   7  


Triaud et al. (2010)
Albrecht et al. (2012)
WASP-195460 ± 90   4.6   ±   5.2  
  15   ±   11  
  1.0   ±   1.2  
  −1.9   ±   1.1  
  0   ±   20  



Hellier et al. (2011)
Albrecht et al. (2012)
Tregloan-Reed et al. (2013)
Sedaghati et al. (2021)
WASP-205987 ± 20   12.7   ±   4.2  

Anderson et al. (2015)
WASP-215924 ± 55   8   + 26   - 27  

Chen et al. (2020)
WASP-226153 ± 46   22   ±   16  

Anderson et al. (2011)
WASP-235046 ± 99 prograde

Triaud et al. (2011)
WASP-246107 ± 77   −4.7   ±   4.0  
  −5.8   ±   4.1  


Simpson et al. (2011)
Smith et al. (2012)
WASP-255736 ± 35   14.6   ±   6.7  

Brown et al. (2012)
WASP-266015 ± 55 indeterminate
  −34   + 36   - 26  


Anderson et al. (2011)
Albrecht et al. (2012)
WASP-286084 ± 45   8   ±   18  
  6   ±   17  


Anderson et al. (2015)
Mocnik et al. (2020)
WASP-306208 ± 85   −7   + 27   - 19  

Triaud et al. (2013)
WASP-316175 ± 70   2.8   ±   3.1  
  −6   ±   6  


Brown et al. (2012)
Albrecht et al. (2012)
WASP-326100 ± 100   10.5   + 6.4   - 6.5  
  −2   + 17   - 19  

  11   ±   14  
Brown et al. (2012)
Brothwell et al. (2014)
WASP-337430 ± 100   252   ±   2  
  −110.06   + 0.40   - 0.27  
  −112.93   + 0.23   - 0.22  


  −111.28   + 0.47   - 0.48  
  −114.01   + 0.22   - 0.20  
  −112.91   ±   0.24  
  −109.29   + 0.20   - 0.17  
  −111.70   ±   0.39  
  −111.64   ±   0.28  
  −94.9   ±   21.4  



  99   + 5   - 4  
  103   + 5   - 4  




  113.99   ±   0.22  
  108.19   + 0.95   - 0.97  
  91.3   ±   18.5  
Collier Cameron et al. (2010)
Johnson et al. (2015) 2008 data
Johnson et al. (2015) 2014 data
Iorio (2016) 2008 data
Iorio (2016) 2014 data
Watanabe et al. (2020) 2008 data
Watanabe et al. (2020) 2011 data
Watanabe et al. (2020) 2014 data
Cauley et al. (2021)
Borsa et al. (2021)
Watanabe et al. (2022)
Kálmán et al. (2022)
WASP-386436 ± 60   15   + 33   - 43  
  7.5   + 4.7   - 6.1  


Simpson et al. (2011)
Brown et al. (2012)
WASP-395485 ± 50   0   ±   11  

Mancini et al. (2018)
WASP-415546 ± 33   29   + 10   - 14  
  6   ±   11  


Neveu-VanMalle et al. (2016)
Southworth et al. (2016)
WASP-434240
+ 30 − 20
  3.5   ±   6.8  
  0   + 20   - 0  
Esposito et al. (2017)
WASP-47b5576 ± 67   0   ±   24  


  29   + 11   - 13  
Sanchis-Ojeda et al. (2015)
Bourrier et al. (2023)
WASP-495600 ± 150   54   + 79   - 58  

Wyttenbach et al. (2017)
WASP-525000 ± 100   24   + 17   - 9  
  3.8   ±   8.4  
  1.1   ±   1.1  
  0.60   + 0.93   - 0.94  

  20   ±   50  


Hébrard et al. (2013)
Mancini et al. (2017)
Chen et al. (2020)
Cegla et al. (2023)
WASP-534950 ± 60   −1   ±   12  

Triaud et al. (2017)
WASP-606105 ± 50   −129   ±   17  

Mancini et al. (2018)
WASP-616250 ± 150   4.0   + 17.1   - 18.4  

Brown et al. (2017)
WASP-626230 ± 80   19.4   + 5.1   - 4.9  

Brown et al. (2017)
WASP-666600 ± 150   −4   ±   22  

Addison et al. (2016)
WASP-694700 ± 50   0.4   + 2.0   - 1.9  

Casasayas-Barris et al. (2017)
WASP-716180 ± 52   20.1   ±   9.7  
  −1.9   + 7.1   - 7.5  


Smith et al. (2013)
Brown et al. (2017)
WASP-726250 ± 100   −7   + 11   - 12  

Addison et al. (2018)
WASP-745984 ± 57   0.77   ±   0.99  

Luque et al.(2020)
WASP-766329 ± 65 misaligned
  61.3   + 7.6   - 5.1  


Brown et al. (2017)
Ehrenreich et al. (2020)
WASP-775605 ± 41   −8   + 19   - 18  

Zak et al. (2024)
WASP-786100 ± 150   −6.4   ±   5.9  

Brown et al. (2017)
WASP-796600 ± 100   −106   + 19   - 13  
  −95.2   + 0.9   - 1.0  
  −99.1   + 4.1   - 3.9  



Addison et al. (2013)
Brown et al. (2017)
Johnson et al. (2017)
WASP-804145 ± 100   0   ±   20  
  −14   ±   14  


Triaud et al. (2013)
Triaud et al. (2015)
WASP-84b5280 ± 80   −0.3   ±   1.7  
  17.3   ±   7.7  
Anderson et al. (2015)
WASP-855685 ± 65   0   ±   14  
  −16.2   ±   2.9  


Mocnik et al. (2016)
Jiang et al. (2023)
WASP-876450 ± 120   −8   ±   11  

Addison et al. (2016)
WASP-946170 ± 80   151   + 16   - 23  
  123.0   ±   3.0  


Neveu-VanMalle et al. (2014)
Ahrer et al. (2024)
WASP-1006940 ± 120   79   + 19   - 10  

Addison et al. (2018)
WASP-1016380 ± 120   34   ±   3  

Zak et al. (2024)
WASP-1036110 ± 160   3   ±   33  
  2   + 35   - 36  


Addison et al. (2016)
Zak et al. (2024)
WASP-1055070 ± 130   −14   + 28   - 24  

Zak et al. (2024)
WASP-1066265 ± 36   −1   ±   11  
  6   + 17   - 18  

  26   + 12   - 17  
Wright et al. (2023)
Wright et al. (2023)
WASP-1074425 ± 70
  118   + 38   - 19  
  −158   + 15   - 19  
  90   ±   50  

  103.5   + 1.79   - 1.8  
Dai et al. (2017)
Rubenzahl et al. (2021)
Bourrier et al. (2023)
WASP-1096520 ± 140   99   + 10   - 9  

Addison et al. (2018)
WASP-1116400 ± 150   −5   ±   16  

Anderson et al. (2014)
WASP-1176040 ± 90   44   ±   11  
  −46.9   + 5.5   - 4.8  
  69.5   + 3.6   - 3.1  

Lendl et al. (2014)
Carone et al. (2021)
WASP-1206450 ± 120   −2   ±   4  

Zak et al. (2024)
WASP-1216586 ± 59   −257.8   + 5.5   - 5.3  
  87.20   + 0.41   - 0.45  
  −87.08   + 0.29   - 0.27  

  88.1   ±   0.25  

Delrez et al. (2016)
Bourrier et al. (2020)
Borsa et al. (2021)
WASP-1275750 ± 100   −128.4   + 5.6   - 5.5  
  −150.6   + 8.1   - 8.7  


Allart et al. (2020)
Cristo et al. (2022)
WASP-1315990 ± 50   162.4   + 1.3   - 1.2  
  161   ±   5  
  123.7   + 12.8   - 8.0  

Doyle et al. (2023)
Zak et al. (2024)
WASP-1345700 ± 100   −43.7   ±   9.9  

Anderson et al. (2018)
WASP-1485437 ± 21   −8.2   + 8.7   - 9.7  

Wang et al. (2022)
WASP-1564910 ± 61   106   ±   14  

Bourrier et al. (2023)
WASP-1666050 ± 50   −3   ±   5  
  −15.5   + 2.9   - 2.8  
  −0.7   ±   0.6  


  0   + 56   - 0  
Hellier et al. (2019)
Doyle et al. (2022)
Bourrier et al. (2023)
WASP-1676900 ± 150   −165   ±   5  

Temple et al. (2017)
WASP-1746400 ± 100   31   ±   1  

Temple et al. (2018)
WASP-1806500 ± 150   −157   ±   2  

Temple et al. (2019)
WASP-1898000 ± 80   89.3   ±   1.4  
  86.4   + 2.9   - 4.4  
  91.7   ±   1.2  
  90.07   ±   0.24  
  90.0   + 5.9   - 5.8  
  85.4   ±   4.3  
  89.6   ±   1.2  

Anderson et al. (2018)
Lendl et al. (2020)
Deline et al. (2022)
Prinoth et al. (2024)
WASP-1906400 ± 100   21   ±   6  

Temple et al. (2019)
XO-25332 ± 57   10   ±   72  
  7   ±   11  

  27   + 12   - 27  
Narita et al. (2011)
Damasso et al. (2015)
XO-36471
+ 83 − 82
  70   ±   15  
  37.3   ±   3.7  
  37.3   ±   3.0  



Hébrard et al. (2008)
Winn et al. (2009)
Hirano et al. (2011)
XO-46397 ± 70   −46.7   + 8.1   - 6.1  

Narita et al. (2010)
XO-66720 ± 100   −20.7   ±   2.3  

Crouzet et al. (2017)
pi Men c5998 ± 62   −24.0   ±   4.1  
  26.9   + 5.8   - 4.7  
Hozdic et al. (2021)

 


Last modified: 2024/04/19           John Southworth   (Keele University, UK)