Table 5
Known rotation parameters from lightcurve observations of Datura family members.
| Asteroid | P | A |
|
|
| [hr] | [mag] | [deg] | ||
|
|
||||
| 1270 | Datura | 3.3581 | 0.5 | 12 |
| 90265 | 2003 CL5 | 23.4153 | 1.8 | 6 |
| 60151 | 1999 UZ6 | 13.8836 | 0.75 | 5 |
| 89309 | 2001 VN36 | 73.145 | 1.4 | 7 |
| 203370 | 2001 WY35 | 8.344 | 1.6 | 32 |
| 215619 | 2003 SQ168 | 4.646 | 0.11 | 26 |
| 2002 RH291 | 5.3 | 1.2 | 16 | |
Notes. P is the rotation period and A is amplitude of the lightcurve. Reported rotation periods are synodic values, except for (1270) Datura, (90265) 2003 CL5, (60151) 1999 UZ6, and (89309) 2001 VN36 for which observations allowed to determine sidereal value (Sects. 4.1−4.3, and Vokrouhlický et al. 2009). In the case of (215619) 2003 SQ165 we cannot exclude also period twice as long. The last column, , gives the mean phase angle of the dense lightcurves used for the estimate of its amplitude.
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