Table 3
Total and mean (averaged) values of Yarkovsky drift in proper a, estimated numerically with the application of two various spin axis orientations models (ΔT = −2 Gyr).
| Asteroid no. and name | D (km) | Total drift Δa (au) |  (mean drift rate) (au Myr−1) |
Pole coordinates λ,β (deg) |
|---|---|---|---|---|
| (956) Elisa | 10.474 | 2.62e−02 | 1.31e−05 | 62 ± 6, −54 ± 6 |
| ± 0.208 | 1.67e−02 | 8.35e−06 | 255 ± 4, −35 ± 3 | |
| (1914) Hartbee- | 9.561 | 2.29e−02 | 1.15e−05 | 37 ± 33, 29 ± 20 |
| spoortdam | ± 0.186 | 8.29e−02 | 4.15e−05 | 175±4, 52±6 |
| (1946) Walraven | 9.205 | 7.80e−02 | 3.90e−05 | 259±20, −80±20 |
| ± 0.109 | 3.36e−01 | 1.68e−04 | 80 ± 20, −59 ± 20 | |
| (2432) Soomana | 7.387 | 4.21e−02 | 2.10e−05 | −, 60 ± 8 |
| ± 0.083 | ||||
| (2566) Kirghizia | 7.816 | 4.30e−02 | 2.15e−05 | 98 ± 1, −50 ± 2 |
| ± 0.172 | 6.25e−02 | 3.12e−05 | 262 ± 1, −60 ± 4 | |
| (2579) Spartacus | 4.604 | 6.58e−01 | 3.29e−04 | 312 ± 5, −57 ± 5 |
| ± 0.369 | 6.55e−01 | 3.28e−04 | 113 ± 5, −60 ± 5 | |
| (2653) Principia | 9.882 | 1.86e−02 | 9.30e−06 | 67 ± 2, 29 ± 2 |
| ± 0.984 | 2.11e−02 | 1.06e−05 | 241 ± 2, 37 ± 4 | |
| (2704) Julian Loewe | 5.199 | 4.90e−02 | 2.45e−05 | 37 ± 40, −88 ± 23 |
| ± 0.291 | 4.32e−02 | 2.16e−05 | 250 ± 50, −64 ± 11 | |
| (2763) Jeans | 7.514 | 1.45e−01 | 7.24e−05 | 85 ± 5, 62 ± 5 |
| ± 0.157 | 1.05e+02 | 5.27e−02 | 255 ± 8, 48 ± 8 | |
| (2851) Harbin | 8.838 | 5.72e−03 | 2.86e−06 | 99 ± 5, 10 ± 5 |
| ± 0.236 | 1.14e+00 | 5.68e−04 | 282 ± 5, 1 ± 5 | |
| (2912) Lapalma | 6.519 | 4.90e−02 | 2.45e−05 | 205± 15, −75 ±6 |
| ± 0.289 | ||||
| (3307) Athabasca | 3.628 | 5.67e−02 | 2.84e−05 | 46 ± 3, 39 ± 8 |
| ± 0.167 | 4.50e−01 | 2.25e−04 | 218 ±3, 30 ± 8 | |
| (3536) Schleicher | 3.145 | 7.49e−02 | 3.75e−05 | 78± 3, −34±6 |
| ± 0.161 | 1.19e−01 | 5.97e−05 | 260 ± 3, −51 ± 5 | |
| (3849) Incidentia | 5.798 | 2.70e−02 | 1.35e−05 | 165 ± 6, 30 ± 9 |
| ± 0.125 | 1.89e−02 | 9.45e−06 | 331 ± 13, 19±6 | |
| (4796) Lewis | 5.56 W | 8.29e−02 | 4.15e−05 | 260 ± 52, 75 ± 15 |
| 7.26e−01 | 3.63e−04 | 328 ± 28, 81 ± 9 | ||
| (5150) Fellini | 5.401 | 5.92e−02 | 2.96e−05 | 7 ± 3, 86 ± 5 |
| ± 0.229 | 5.22e−02 | 2.61e−05 | 257 ± 3, 73 ± 5 | |
| (5524) Lecacheux | 19.902 | 1.79e−02 | 8.93e−06 | -, −57 ± 9 |
| ± 12.768 | ||||
| (5525) 1991 TS4 | 5.281 | 1.56e+00 | 7.80e−04 | 43 ± 50, −48 ± 4 |
| ± 0.104 | 5.43e−02 | 2.71e−05 | 223 ± 40, −65 ± 8 | |
| (5754) 1992 FR2 | 6.337 | 4.83e−02 | 2.41e−05 | 122 ± 40, −85 ± 11 |
| ± 0.078 | ||||
| (5952) Davemonet | 4.861 | 8.48e−02 | 4.24e−05 | 108 ± 4, −75 ± 4 |
| ± 0.275 | 8.14e−02 | 4.07e−05 | 351 ±3, −73±6 | |
| (6406) Mikejura | 4.062 | 6.20e−02 | 3.10e−05 | 17 ±5, −61 ± 5 |
| ± 0.233 | 6.09e−02 | 3.05e−05 | 216 ± 5, −52 ± 5 | |
| (7558) Yurlov | 6.04 (*) | 7.24e−02 | 3.62e−05 | 121 ± 20, −75 ± 12 |
| 6.28e−02 | 3.14e−05 | 345 ± 48, −64 ± 11 | ||
| (7899) Joya | 3.902 | 2.54e−02 | 1.27e−05 | -, −47 ± 17 |
| ± 0.379 | ||||
| (17028) 1999 FJ5 | 1.951 | 1.85e+00 | 9.27e−04 | 40 ±5, 18 ± 5 |
| ± 0.388 | 3.10e−02 | 1.55e−05 | 221 ± 5, 13±5 | |
| (18641) 1998 EG10 | 3.717 | 8.46e−02 | 4.23e−05 | −, prograde (**) |
| ± 0.650 | ||||
| (25327) 1999 JB63 | 4.362 | 1.91e+00 | 9.54e−04 | 148 ± 2, −56 ± 6 |
| ± 0.077 | 1.58e+00 | 7.91e−04 | 339 ± 5, −55 ± 9 | |
| (25542) Garabedian | 2.726 | 7.88e−02 | 3.94e−05 | 141 ±5, 37 ± 5 |
| ± 0.385 | 1.05e−01 | 5.25e−05 | 312 ± 5, 61 ± 5 |
Notes. (*)Data from ALCDEF (Warner et al. 2009). (**)For asteroid (18641) 1998 EG10, we only know the sense of rotation, so we use the angle at which the Yakrovsky drift is maximum.
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