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Table 3
The number of revolutions to become a NEO.
| Object | Activity’s probability | Number of clones on NEO-type orbits | ||||
|---|---|---|---|---|---|---|
| 20% | 40% | 60% | 80% | 100% | ||
| 238P | 0.1 | 30 862 | 31 990 | 33 831 | 34 522 | 44 433 |
| 0.4 | 7728 | 8109 | 8206 | 8447 | 8521 | |
| 324P | 0.1 | 8183 | 8808 | 9070 | 9239 | 9422 |
| 0.4 | 2157 | 2188 | 2190 | 2278 | 2305 | |
| 358P | 0.1 | 953 | 1003 | 1074 | 1149 | 1370 |
| 0.4 | 222 | 227 | 247 | 269 | 289 | |
Notes. The stronger cometary-type NG forces (see the A1 , A2 and A3 coefficients in Table 2), the shorter time to transfer to NEO-type orbit. All clones of bodies with A2 < 0 and values larger than –10−8 have evolved to NEO-type orbits.
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