Table 3
General characteristics of the Earth-like planets formed within the HZ in the two sets of simulations.
| Simulations | Planet | M (M⊕) | W (%) | t50.class - D (Myr) | t50.class - W (Myr) | T50% (Myr) | T75% (Myr) |
|
|
|||||||
| First set | b | 1.19 | 4.51 | 21.9 | 81.3 | 35 | 35 |
| d | 0.66 | 8.10 | 21.8 | 67.3 | 2.9 | 13.4 | |
|
|
|||||||
| Second set | a | 2.21 | 8.75 | 21.8 | 56.6 | 51.7 | 51.7 |
| c | 2.00 | 10.76 | 39.8 | 66.9 | 6 | 20.5 | |
| e | 1.37 | 7.49 | 27.1 | 67.8 | 4.4 | 18.4 | |
Notes. M (M⊕) represents the final mass, t50.class - D represents the timescale in Myr for a planet to accrete half of the class D planetesimals that will accrete, t50.class - W represents the timescale in Myr for a planet to accrete half of the class W planetesimals that will accrete, T50% represents the timescale in Myr for a planet to achieve 50% of its final mass, and T75% represents the timescale in Myr for a planet to acquire 75% of its final mass. Planet b of the first set shows the same T50% and T75%. This means that the planet suddenly accreted enough mass to change from having less than 50% of its final mass to have more than 75% of its final mass. The same occurs with planet a of the second set.
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