Table 2
Masses of the planets used in the simulation.
| Mass model | M1 | M2 | M2a | M2d |
|---|---|---|---|---|
| “Mass-radius” | “Peas-in-a-pod” | |||
| mb(m⊕) | 5.09 | 5.09 | 5.09 | 5.09 |
| mc(m⊕) | 9.08 | 5.09 | 6.50 | 6.50 |
| md(m⊕) | 8.52 | 5.09 | 5.09 | 10.18 |
| me(m⊕) | 11.55 | 5.09 | 5.09 | 5.09 |
Notes. In mass model M1, the masses of the planets follow the massradius relationship given by Chen & Kipping (2017). Mass model M2 assumes all planets have the same mass around 5 M⊕ consistent with the peas-in-a-pod mass model (Weiss & Petigura 2020; Weiss et al. 2023). Mass models M2a and M2d are variations of Model 2 following the mass constraint in Section 6.2.
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