Table A.1
Orbital elements and physical properties for the sample of 20 observed asteroids collected at epoch 61200 mjd.
| Asteroid | a [au] | e | i [°] | Ω [°] | ω [°] | H [mag] | albedo | d [km] | m [kg] | MOID [au] | MMOID [rad] |
|---|---|---|---|---|---|---|---|---|---|---|---|
| 4179 Toutatis | 2.54 | 0.62 | 0.45 | 125.37 | 277.86 | 15.30 | 0.254 | 2.64 | 2.12 × 1013 | 4.10 × 10−4 | (6.19, 2.74) |
| 69230 Hermes | 1.66 | 0.62 | 6.07 | 34.03 | 92.93 | 17.57 | 0.265 | 0.82 | 6.35 × 1011 | 1.45 × 10−4 | (0.40, 2.07)* |
| 2002 PZ39 | 1.47 | 0.55 | 1.67 | 328.72 | 260.19 | 19.10 | − | − | 1.79 × 1011 | 9.89 × 10−5 | (0.51, 3.83)* |
| 2013 FA8 | 1.93 | 0.67 | 3.12 | 165.42 | 281.06 | 20.93 | − | − | 1.43 × 1010 | 2.28 × 10−5 | (0.30, 5.50) |
| 1997 BR | 1.34 | 0.31 | 17.25 | 116.63 | 133.86 | 17.80 | 0.51 | 0.56 | 2.02 × 1011 | 1.31 × 10−4 | (0.42, 5.56)** |
| 2007 UY1 | 0.95 | 0.18 | 1.02 | 337.45 | 274.12 | 23.08 | − | − | 7.28 × 108 | 7.64 × 10−6 | (4.60, 0.68)* |
| 2003 QQ47 | 1.09 | 0.19 | 62.10 | 0.98 | 104.97 | 17.37 | − | − | 1.96 × 1012 | 4.38 × 10−4 | (0.96, 1.46)* |
| 1999 MN | 0.67 | 0.67 | 2.03 | 81.38 | 9.21 | 20.57 | − | − | 2.35 × 1010 | 6.29 × 10−5 | (1.90, 0.57) |
| 2003 YK118 | 1.70 | 0.49 | 7.83 | 326.73 | 233.28 | 18.81 | 0.07 | 0.90 | 8.40 × 1011 | 3.44 × 10−4 | (5.97, 5.05) |
| 2011 BO24 | 1.38 | 0.28 | 20.37 | 91.46 | 178.67 | 18.78 | − | − | 2.78 × 1011 | 2.42 × 10−4 | (0.01, 5.14)** |
| 2003 AC23 | 2.17 | 0.58 | 2.06 | 43.73 | 126.41 | 21.90 | − | − | 3.72 × 109 | 3.97 × 10−5 | (0.16, 6.17) |
| 2020 FR1 | 1.41 | 0.61 | 13.11 | 26.37 | 255.89 | 21.20 | − | − | 9.86 × 109 | 8.58 × 10−5 | (0.54, 2.92) |
| 2018 DA1 | 1.21 | 0.73 | 25.49 | 139.90 | 233.94 | 18.85 | − | − | 2.52 × 1011 | 3.37 × 10−4 | (0.62, 4.95) |
| 2016 CU193 | 1.47 | 0.36 | 49.89 | 322.37 | 323.12 | 19.94 | − | − | 5.59 × 1010 | 1.73 × 10−4 | (0.29, 1.83) |
| 2014 UC192 | 1.41 | 0.36 | 11.66 | 34.92 | 304.61 | 23.72 | − | − | 3.03 × 108 | 1.78 × 10−5 | (0.44, 3.06) |
| 2005 TU50 | 1.43 | 0.60 | 12.42 | 22.18 | 259.71 | 21.45 | − | − | 6.92 × 109 | 1.14 × 10−4 | (0.53, 2.84) |
| 2006 BC10 | 2.02 | 0.66 | 0.91 | 20.25 | 235.24 | 19.50 | − | − | 1.03 × 1011 | 7.24 × 10−4 | (6.01, 5.62) |
| 2024 QP2 | 2.54 | 0.62 | 1.64 | 205.32 | 202.15 | 21.57 | − | − | 5.83 × 109 | 1.78 × 10−4 | (6.20, 4.98)* |
| 2015 DU180 | 1.93 | 0.92 | 4.86 | 51.74 | 315.41 | 21.03 | 0.28 | 0.39 | 6.83 × 1010 | 1.08 × 10−3 | (6.05, 0.17) |
| 2014 WK7 | 1.56 | 0.36 | 23.91 | 233.74 | 180.93 | 22.17 | − | − | 2.59 × 109 | 1.68 × 10−4 | (6.27, 1.32)** |
Notes. The mass was computed using Eq. 2 either using the values of observed properties or assuming the intermediate values. MMOID indicates the mean anomalies needed for the asteroid and spacecraft 2 (* for spacecraft 1, ** for spacecraft 3) to be in a close approach configuration at the MOID, respectively.
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