Table 2
Input data concerning the planets: mass, radius, orbital period, semi-major axis, excentricity.
| Name | MP (M⊕) | RP (R⊕) | Porb (day) | a (AU) | e |
|
|
|||||
| PSR 1257+12 a | 0.02 | 0.28 | 25. | 0.19 | 0 |
| PSR 1257+12 b | 4.3 | 1.68 | 66. | 0.36 | 0.0186 |
| PSR 1257+12 c | 3.9 | 1.62 | 98. | 0.46 | 0.0252 |
|
|
|||||
| PSR 1620-26 a | 794 | 9,5 | 36367. | 23. | |
|
|
|||||
| PSR 1 s b 10 000 km | 3.5 | 1.57 | 30. | 0.21 | 0. |
|
|
|||||
| PSR 10 ms b 100 km | 2. × 10-6 | 0.016 | 20. | 0.16 | 0.3 |
| PSR 10 ms b 1 km | 2. × 10-12 | 1.6 × 10-4 | 20. | 0.16 | 0.3 |
|
|
|||||
| PSR 1 s b 100 km | 2. × 10-6 | 0.016 | 20. | 0.16 | 0.3 |
| PSR 1 s b 1 km | 2. × 10-12 | 1.6 × 10-4 | 20. | 0.16 | 0.3 |
Notes. Source: M⊕, Porb, a, e from “The Extrasolar Planets Encyclopaedia” (http://exoplanet.eu/index.php). The estimate of RP is based on the hypothesis of an average mass density ρP = 5000 kg m-3.
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