Table 3
Pebble flux and isolation mass for the nominal setup (Z0 = 0.01, a = 0.2 au).
α | Md,0 [M⊙ ] | Final Mcore [M⊕ ] | Time when Miso [Myr] | Time when pebble | Integrated | ɛ [%] (2) |
---|---|---|---|---|---|---|
is achieved | flux is negligible [Myr] (1) | pebble flux [M⊕] | ||||
0.01 | 0.037 | Never | 0.44 | 0.20 | 13.5 | |
10−3 | 0.03 | 0.026 | Never | 1.13 | 0.56 | 2.86 |
0.06 | 0.017 | Never | 1.92 | 1.00 | 0.7 | |
0.1 | 0.015 | Never | 2.80 | 1.66 | 0.3 | |
0.01 | 0.25 | Never | 0.88 | 7.77 | 3.09 | |
10−4 | 0.03 | 0.87 | Never | 1.16 | 23.4 | 3.68 |
0.06 | 1.38 | 3.70 | 2.23 | 45.7 | 3.00 | |
0.1 | 1.95 | 3.73 | 3.71 | 74.2 | 2.61 | |
0.01 | 1.76 | 0.069 | 2.43 | 25.9 | 6.76 | |
10−5 | 0.03 | 2.58 | 0.047 | 2.31 | 76.2 | 3.37 |
0.06 | 4.60 | 0.046 | 2.32 | 157 | 2.92 | |
0.1 | 7.30 | 0.047 | 2.17 | 267 | 2.73 |
Notes. (1) Negligible means that the pebble flux falls below 10−8 M⊕ yr−1. (2) ɛ is the efficiency of pebble accretion, defined as the amount of pebbles accreted by the planet over the integrated pebble flux at the position of the planet (Guillot et al. 2014; Lambrechts & Johansen 2014).
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