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Table 4
Most numerous non-gravitational parameter da/dt populations among the clones of the 21 numbered retrograde asteroids after a 10 Myr integration forward.
| Range of the non-gravitational parameter, da/dt | |||
|---|---|---|---|
| (10−5 au Myr−1) | |||
| Negative | Positive | ||
| Range | Number of clones | Range | Number of clones |
| −0.0001;−0.04 | 463 | +0.0;+0.04 | 1355 |
| −0.04;−0.08 | 124 | +0.04;+0.08 | 36 |
| −0.08;−0.12 | 10 | +0.08;+0.12 | 4 |
| −0.12;−0.16 | 16 | +0.12;+0.16 | 2 |
| −0.16;−0.20 | 8 | +0.16;+0.20 | 4 |
| −0.20;−0.24 | 21 | +0.20;+0.24 | 6 |
| −0.24;−0.28 | 3 | +0.24;+0.28 | 4 |
| −0.28;−0.32 | 2 | +0.28;+0.32 | 3 |
| −0.32;−0.36 | 2 | +0.32;+0.36 | 0 |
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