IAA Minor Planet Database| Epoch (TDB) | 2025-11-21 (JD 2461000.5) |
|---|---|
| Eccentricity (e) | 0.1414005730 ± 2.00e+00 |
| Semi-major axis (a) | 1.1599963666 AU ± 3.00e+00 |
| Inclination (i) | 31.75826063° ± 4.00e+00 |
| Long. of Asc. Node (Ω) | 169.47976565° ± 5.00e+00 |
| Arg. of Perihelion (ω) | 121.03552314° ± 6.00e+00 |
| Mean Anomaly (M) | 239.35344816° ± 1.60e-05 |
| Mean Motion (n) | 0.7889097669°/day ± 3.06e+00 |
| Perihelion dist (q) | 0.99597222 AU ± 3.47e+00 |
| Aphelion dist (Q) | 1.32402052 AU ± 4.14e+00 |
| Orbital Period | 1.24935237 yr ± 4.85e+00 |
| NGA Model | r2 |
| A2 | 2.91680648e-06 AU/d² |
| H (abs. magnitude) | 20.31 |
|---|---|
| G (slope) | 0.15 |
| Source | IAA |
|---|---|
| Solution Date | 2026-04-28 |
| RMS Residual | 0.386″ |
| Uncertainty | 0 |
| Orbit Type | Apollo |
| MOID | 0.049870 AU |
| Observations Used | 356 |
| Oppositions | 4 |
| Arc Total | 2002-2022 |
| First Observation Used | 2002-03-12 |
| Last Observation Used | 2022-09-12 |
| Date | Type | RA | Dec | Mag | Band | Observatory |
|---|---|---|---|---|---|---|
| 2022-04-07 05:52:54 | C | 10 41 33.079 | +52 29 57.44 | – | V | G96 |
| 2022-04-07 06:06:52 | C | 10 41 32.741 | +52 30 29.23 | – | V | 703 |
| 2022-04-07 06:30:02 | C | 10 41 31.934 | +52 31 22.55 | – | V | 703 |
| 2022-09-07 21:02:23 | C | 17 49 06.35 | +24 52 35.3 | – | V | L18 |
| 2022-09-07 21:06:26 | C | 17 49 07.35 | +24 52 03.1 | – | V | L18 |
| 2022-09-07 21:10:30 | C | 17 49 08.31 | +24 51 29.4 | – | V | L18 |
| 2022-09-08 06:17:19 | C | 17 51 27.959 | +23 37 22.31 | – | U | F51 |
| 2022-09-08 06:37:06 | C | 17 51 32.622 | +23 34 38.12 | – | U | F51 |
| 2022-09-08 07:17:06 | C | 17 51 42.138 | +23 29 03.61 | – | U | F51 |
| 2022-09-10 21:49:47 | C | 18 07 55.12 | +14 05 32.0 | – | q | J69 |
| 2022-09-10 21:59:47 | C | 18 07 57.77 | +14 03 55.9 | – | q | J69 |
| 2022-09-10 22:19:47 | C | 18 08 02.86 | +14 00 40.7 | – | q | J69 |
| 2022-09-12 19:10:35 | C | 18 20 05.48 | +06 33 13.8 | – | V | 130 |
| 2022-09-12 19:13:50 | C | 18 20 06.35 | +06 32 40.1 | – | V | 130 |