Table B.1
Possible locations of long-term stable inner terrestrial planets in the 22 single-giant planet systems with e2 ≥ 0.4.
| MMR | ||||||||||||||||||||||
|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
| 3∕2 | 5∕3 | 2∕1 | 7∕3 | 5∕2 | 8∕3 | 3∕1 | 7∕2 | 4∕1 | 9∕2 | 5∕1 | 11∕2 | 6∕1 | 13∕2 | 7∕1 | 15∕2 | 9∕1 | 19∕2 | 12∕1 | 25∕2 | 19∕1 | 23∕1 | |
| a1∕a2 | ||||||||||||||||||||||
| 0.7631 | 0.7113 | 0.6299 | 0.5684 | 0.5428 | 0.5200 | 0.4807 | 0.4337 | 0.3968 | 0.3668 | 0.3419 | 0.3209 | 0.3028 | 0.2871 | 0.2732 | 0.2609 | 0.2311 | 0.2229 | 0.1907 | 0.1856 | 0.1404 | 0.1236 | |
| System HD | ||||||||||||||||||||||
| 20782 | e1 ≥ 0.3 | e1 ≥ 0.3 | (e1 ≥ 0.3) | (e1 = 0.5) | (e1 = 0.5) | (e1 = 0.5) | (e1 = 0.5) | (e1 = 0.5) | ||||||||||||||
| 108341 | e1 ≥ 0.3 | e1 ≥ 0.3 | (e1 ≥ 0.3) | e1 = 0.5 E | e1 = 0.5 E | e1 = 0.5 E | (e1 = 0.5) E | e1 = 0.5 E | ||||||||||||||
| 4113 | e1 ≥ 0.3 | e1 ≥ 0.3 | (e1 ≥ 0.3) | (e1 = 0.5) | ||||||||||||||||||
| 28254 | e1 ≥ 0.3 | e1 = 0.5 | e1 = 0.02 E | e1 = 0.5 E | (e1 = 0.02) | (e1 ≥ 0.02) | e1 = 0.3 E | |||||||||||||||
| 45350 | e1 ≥ 0.3 | (e1 = 0.3) | e1 = 0.5 | e1 = 0.02 | (e1 = 0.3) | (e1 = 0.3) | ||||||||||||||||
| 30562 | e1 ≥ 0.3 | (e1 = 0.3) | e1 = 0.02 | e1 = 0.5 | (e1 = 0.1) E | (e1 = 0.3) E | (e1 = 0.3) E | (e1 = 0.1) E | (e1 = 0.1, 0.3) E | (e1 = 0.3) E | (e1 = 0.3) E | (e1 = 0.3) E | (e1 = 0.3) E | |||||||||
| 86226 | e1 ≥ 0.02 E | e1 ≥ 0.02 E | e1 = 0.5 | e1 ≥ 0.02 E | e1 ≥ 0.02 | (e1 ≥ 0.02) E | (e1 = 0.3) E | (e1 = 0.1) E | (e1 = 0.5) E | (e1 = 0.3) E | (e1 = 0.5) E | (e1 = 0.3) E | (e1 = 0.5) E | (e1 = 0.1) E | (e1 = 0.5) E | (e1 = 0.3) E | (e1 = 0.5) E | (e1 = 0.3) E | (e1 = 0.5) E | (e1 = 0.1) E | (e1 = 0.3) E | (e1 = 0.3) E |
| 129445 | e1 = 0.5 E | (e1 = 0.1) E | (e1 = 0.3) E | |||||||||||||||||||
| 120084 | e1 ≥ 0.02 E | e1 ≥ 0.02 E | e1 = 0.5 | e1 ≥ 0.02 E | e1 ≥ 0.02 | (e1 ≥ 0.02) E | e1 = 0.5 E | (e1 = 0.3) E | (e1 = 0.3) E | (e1 = 0.3) E | (e1 = 0.3) E | (e1 = 0.3) E | (e1 = 0.3) E | (e1 = 0.1) E | (e1 = 0.3) E | |||||||
| 16175 | ||||||||||||||||||||||
| 152079 | e1 ≥ 0.02 E | e1 ≥ 0.02 E | e1 = 0.5 | e1 ≥ 0.02 E | e1 ≥ 0.02 | (e1 ≥ 0.02) E | (e1 = 0.3) E | (e1 = 0.3) E | e1 = 0.5 E | (e1 = 0.3) E | e1 = 0.5 E | (e1 = 0.3) E | (e1 = 0.3) E | (e1 = 0.3) E | (e1 = 0.3) E | (e1 = 0.1) E | (e1 = 0.3) E | |||||
| 171028 | e1 ≥ 0.02 E | e1 ≥ 0.02 E | e1 = 0.5 E | e1 ≥ 0.02 E | e1 ≥ 0.02 | (e1 ≥ 0.02) E | (e1 = 0.3) E | (e1 = 0.3) E | (e1 = 0.3) E | (e1 = 0.3) E | (e1 = 0.3) E | (e1 = 0.3) E | (e1 = 0.1) E | (e1 = 0.3) E | ||||||||
| 79498 | ||||||||||||||||||||||
| 220773 | e1 ≥ 0.02 E | e1 ≥ 0.02 E | e1 ≥ 0.02 E | e1 ≥ 0.02 | (e1 ≥ 0.02) E | (e1 ≥ 0.02) E | (e1 ≥ 0.02) E | e1 = 0.5 E | (e1 ≥ 0.02) E | (e1 ≥ 0.02) E | (e1 ≥ 0.02) E | (e≥0.02) E | (e1 ≥ 0.02) E | (e1 ≥ 0.02) E | ||||||||
| 142415 | ||||||||||||||||||||||
| 29021 | ||||||||||||||||||||||
| 210277 | ||||||||||||||||||||||
| 66428 | ||||||||||||||||||||||
| 213240 | ||||||||||||||||||||||
| 23127 | ||||||||||||||||||||||
| 162004 | ||||||||||||||||||||||
| 171238 | ||||||||||||||||||||||
| – | ||||||||||||||||||||||
Notes. Possible locations of long-term stable inner terrestrial planets in the 22 single-giant planet systems with e2 ≥ 0.4. As in Fig. 11, whenever a survival of a terrestrial is favoured, we note the minimum value of e1 (among 0.02, 0.1, 0.3, and 0.5) in the MMR’s column. The symbol E refers to additional possible captures in MMRs allowed by the observational errors in e2. When the survival is not probable, because the regular domain is not broad or the giant is located at its borders, the value e1 is displayed in parentheses. We note that only the main MMRs are reported here (other tongues exist; they are narrower than those already mentioned and survival is far more improbable for them).
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