Table 5
Properties and ejection velocities of individual fragments.
| Met | m | d | X | Y | Z | 2σR | Ejection velocity |
|---|---|---|---|---|---|---|---|
| # | [10−3 g] | [mm] | [km] | [km] | [km] | [km] | [m s−1] |
| 01 |  |
61.7 | 0.0 | 0.0 | 0.0 | 8.7 | |
| 02 |  |
9.0 | 357.2 | 214.9 | 103.7 | 9.7 | 0.26± 0.05 |
| 03 |  |
4.7 | 535.9 | 168.2 | 109.5 | 34.2 | 0.40± 0.08 |
| 04 |  |
7.1 | 285.3 | 214.4 | 193.9 | 22.5 | 0.37± 0.07 |
| 05 |  |
4.9 | 423.4 | 165.8 | 182.9 | 13.4 | 0.39± 0.08 |
| 06 |  |
6.0 | 390.9 | 163.7 | 49.7 | 20.2 | 0.26± 0.05 |
| 07 |  |
8.3 | 355.9 | 253.4 | 160.7 | 13.3 | 0.34± 0.06 |
| 08 |  |
3.4 | 612.4 | 179.8 | 139.6 | 21.8 | 0.54± 0.10 |
| 09 |  |
3.3 | 589.6 | 195.5 | 142.5 | 16.8 | 0.61± 0.11 |
| 10 |  |
5.6 | 420.2 | 318.1 | 108.5 | 31.4 | 0.42± 0.08 |
| 11 |  |
6.8 | 404.8 | 314.3 | 146.8 | 31.7 | 0.40± 0.07 |
| 12 |  |
3.8 | 693.5 | 204.6 | 199.5 | 46.4 | 0.39± 0.08 |
| 13 |  |
7.8 | 325.0 | 356.3 | 218.9 | 33.8 | 0.47± 0.09 |
| 14 |  |
5.5 | 538.8 | 307.8 | 227.4 | 31.0 | 0.43± 0.08 |
| 15 |  |
4.7 | 775.1 | 86.6 | 106.8 | 4.6 | 0.16± 0.03 |
| 16 |  |
3.7 | 796.3 | 229.2 | 115.6 | 18.1 | 0.33± 0.06 |
| 17 |  |
4.1 | 794.1 | 326.8 | 165.4 | 17.5 | 0.41 ± 0.07 |
| S1 |  |
5.5 | 576.6 | 167.6 | 37.3 | 14.5 | 0.20± 0.04 |
| S2 |  |
4.8 | 594.3 | 320.9 | −32.2 | 22.6 | 0.38± 0.07 |
| S3 |  |
4.7 | 605.6 | 486.8 | 158.4 | 26.0 | 0.58± 0.10 |
| S4 |  |
4.3 | 868.9 | 314.3 | 196.9 | 69.7 | 0.42± 0.09 |
| S5 |  |
3.1 | 854.6 | 254.4 | 197.9 | 63.3 | 0.47± 0.10 |
Notes. The photometric pre-atmospheric mass m has two combined standard uncertainty intervals. The diameter, d, is given for a density of ρ = 1000 kg m−3. The coordinates (X, Y, Z) are expressed with respect to the system that is connected with the most massive fragment ‘01’. The x-axis points in the antisolar direction, and the z-axis points to the north pole of the ecliptic. Lastly, σR represents the combined standard uncertainty of positions. The right part of the table shows calculated mean values of velocity with two standard combined uncertainties.
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