Table 1
Properties of individual fragments.
| frag. i | mi (10−3 g) | di (mm) | Xi (km) | Yi (km) | Zi (km) |  (km) |
|---|---|---|---|---|---|---|
| 0 |  |
50.2 | 0.000 | 0.000 | 0.000 | 0.032 |
| 1 |  |
3.3 | 42.516 | 8.939 | −37.339 | 0.167 |
| 2 |  |
1.7 | 26.977 | −11.916 | −12.268 | 0.210 |
| 3 |  |
2.4 | 84.139 | −43.757 | −48.710 | 0.952 |
| 4 |  |
2.4 | 70.416 | −29.267 | −33.713 | 0.231 |
| 5 |  |
1.3 | 54.924 | 14.484 | −37.583 | 0.612 |
| 6 |  |
1.4 | 46.286 | −5.252 | −2.559 | 0.417 |
| 7 |  |
2.0 | 66.155 | −7.757 | −18.498 | 0.259 |
| 8 |  |
1.2 | 92.833 | −14.704 | −30.086 | 1.439 |
| 9 |  |
0.9 | 70.728 | −52.815 | −52.372 | 2.169 |
Notes. The photometric preatmospheric mass mi has two combined standard uncertainty intervals. Size di is for density ρ = 1000 kg m−3. The coordinates of corrected observed positions of fragments robs = (X, Y, Z) are expressed with respect to the coordinate system that is connected with the most massive fragment 0. The x-axis points in the antisolar direction, and the z-axis points to the north pole of the ecliptics. Lastly, 
represents the combined standard uncertainty of positions.
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