Summary of the Single Systems Modelled
Since the work of Menou &
Tabachnik (2003), 22 new extrasolar planets have been found [as of Feb
2004]. Four of these were discarded due to poor parameter constraints
and another four were discarded because of extremely short planetary periods
(< 5 days). Thus we are left with 14 new systems since the work of M&T.
We also list 3 systems used to compare with M&T's results.
| System |
Mstar(Msun) |
Mpl(Mjup) |
a (AU) |
ecc |
HZin (AU) |
HZout (AU) |
dt (days) |
| HD 70642 |
1.0 |
2.0 |
3.3 |
0.1 |
0.7 |
1.55 |
10.7 |
| HD 41004A |
0.7 |
2.3 |
1.31 |
0.39 |
0.34 |
0.76 |
4.38 |
| HD 104985 |
1.5 |
6.3 |
0.78 |
0.03 |
1.58 |
3.49 |
10.25 |
| HD 216770 |
0.9 |
0.65 |
0.46 |
0.37 |
0.57 |
1.26 |
6.0 |
| HD 219542B |
1.06 |
0.3 |
0.46 |
0.32 |
0.79 |
1.74 |
5.53 |
| HD 3651 |
0.79 |
0.2 |
0.284 |
0.63 |
0.44 |
0.97 |
3.11 |
| HD 192263 |
0.79 |
0.72 |
0.15 |
0.0 |
0.44 |
0.97 |
1.19 |
| HD 162020 |
0.7 |
13.75 |
0.072 |
0.277 |
0.34 |
0.76 |
0.42 |
| HD 142415 |
1.03 |
1.62 |
1.05 |
0.5 |
0.743 |
1.597 |
11.52 |
| HD 65216 |
0.92 |
1.21 |
1.37 |
0.4 |
0.592 |
1.426 |
8.68 |
| HD 10647 |
1.07 |
0.91 |
2.1 |
0.2 |
0.801 |
1.659 |
12.67 |
| HD 111232 |
0.78 |
6.8 |
1.97 |
0.2 |
0.426 |
1.209 |
5.747 |
| HD 2039 |
0.98 |
4.85 |
2.19 |
0.7 |
0.672 |
1.519 |
10.169 |
| HD 216435 |
1.25 |
1.49 |
2.7 |
0.3 |
1.094 |
1.928 |
18.685 |
|
|
|
|
|
|
|
|
| HD 169830 |
1.4 |
2.88 |
0.81 |
0.31 |
1.372 |
3.038 |
11.24 |
| HD 114783 |
0.92 |
0.9 |
1.2 |
0.1 |
0.592 |
1.312 |
8.68 |
| HD 210277 |
0.99 |
1.28 |
1.097 |
0.45 |
0.686 |
1.519 |
10.45 |