Table 2
Observed wide-orbit planets around stars.
| System | Age | Spectral type | Planets | rproj | M p | Predicted phase | Ref. |
| [Myr] | [AU] | [MJup] | |||||
|
|
|||||||
| 1RXS J1609 | 5 | M0± 1V | b | ~330 |
|
B/C | 1, 2 |
| AB Pic | ~30 | K2V | b | ~260 | 13−14 | C | 3 |
| β Pic |
|
A6V | b | 8−15 | 9 ± 3 | A/C | 4, 5 |
| Fomalhaut | 440 | A3V | b∗ | ~ 119 | ≲ 3 | B/C | 6, 7 |
| GJ 504 |
|
G0V | b | 43.5 |
|
C | 8 |
| HD 106906 | 13 ± 2 | F5V | b | ~ 650 | 11 ± 2 | B/C | 9, 10 |
| HD 95086 | 10−17 | A8V | b | 56.4 ± 0.7 | 5 ± 2 | A/B/C | 11, 12 |
| HR 8799 |
|
A5V to F0V | b | 68 |
|
A | 13, 14, 15, 16 |
| c | 38 |
|
13, 14, 15 | ||||
| d | 24 |
|
13, 14, 15 | ||||
| e | 15 | 5 ± 2 | 14, 15 | ||||
| κ And |
|
B9IV | b | 55 ± 2 |
|
A/C | 17, 18 |
Notes.
Note news of Fomalhaut b being dust cloud from collision with asteroid belt (Kennedy & Wyatt 2011; Kenyon et al. 2014).
Reference. 1 – Bowler et al. (2014); 2 – Lafrenière et al. (2010); 3 – Chauvin et al. (2005); 4 – Lagrange et al. (2010); 5 – Zuckerman et al. (2001); 6 – Mamajek (2012); 7 – Kalas et al. (2008); 8 – Kuzuhara et al. (2013); 9 – Bailey et al. (2014); 10 – Pecaut et al. (2012); 11 – Rameau et al. (2013); 12 – Galicher et al. (2014); 13 – Marois et al. (2008); 14 – Marois et al. (2010); 15 – Currie et al. (2011); 16 – Gray & Kaye (1999); 17 – Carson et al. (2013); 18 – Wu et al. (2011).
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