IAA Minor Planet Database| Epoch (TDB) | 2025-11-21 (JD 2461000.5) |
|---|---|
| Eccentricity (e) | 0.5067352288 ± 2.00e+00 |
| Semi-major axis (a) | 0.9051333949 AU ± 3.00e+00 |
| Inclination (i) | 23.64113598° ± 4.00e+00 |
| Long. of Asc. Node (Ω) | 166.67288055° ± 5.00e+00 |
| Arg. of Perihelion (ω) | 47.73088466° ± 6.00e+00 |
| Mean Anomaly (M) | 280.24867793° ± 3.41e-05 |
| Mean Motion (n) | 1.1445727273°/day ± 5.69e+00 |
| Perihelion dist (q) | 0.44647042 AU ± 2.34e+00 |
| Aphelion dist (Q) | 1.36379637 AU ± 4.87e+00 |
| Orbital Period | 0.86113032 yr ± 4.28e+00 |
| NGA Model | r2 |
| A2 | -3.75660344e-06 AU/d² |
| H (abs. magnitude) | 20.17 |
|---|---|
| G (slope) | 0.15 |
| Source | IAA |
|---|---|
| Solution Date | 2026-04-26 |
| RMS Residual | 0.404″ |
| Uncertainty | 0 |
| Orbit Type | Aten |
| MOID | 0.006510 AU |
| Observations Used | 129 |
| Oppositions | 4 |
| Arc Total | 1998-2023 |
| First Observation Used | 1998-09-21 |
| Last Observation Used | 2023-10-04 |
| Date | Type | RA | Dec | Mag | Band | Observatory |
|---|---|---|---|---|---|---|
| 2023-10-02 22:40:33 | C | 23 24 07.150 | -40 29 23.68 | – | V | M22 |
| 2023-10-02 22:51:41 | C | 23 24 05.904 | -40 29 25.69 | – | V | M22 |
| 2023-10-04 03:51:10 | C | 23 21 20.578 | -40 34 49.30 | – | V | W68 |
| 2023-10-04 03:55:47 | C | 23 21 20.076 | -40 34 48.65 | – | V | W68 |
| 2023-10-04 04:03:08 | C | 23 21 19.351 | -40 34 50.63 | – | V | W68 |
| 2023-10-04 04:54:00 | C | 23 21 14.278 | -40 34 56.53 | – | V | W68 |
| 2023-11-03 08:38:40 | S | 23 08 11.23 | -37 10 03.8 | – | L | C51 |
| 2023-11-03 11:44:47 | S | 23 08 15.48 | -37 08 34.1 | – | L | C51 |
| 2023-11-03 11:44:58 | S | 23 08 15.55 | -37 08 35.6 | – | L | C51 |
| 2023-11-03 14:51:06 | S | 23 08 19.93 | -37 07 04.0 | – | L | C51 |
| 2023-11-04 01:42:57 | S | 23 08 35.58 | -37 01 50.3 | – | L | C51 |
| 2023-11-04 07:55:23 | S | 23 08 44.69 | -36 58 47.0 | – | L | C51 |
| 2023-11-04 14:07:48 | S | 23 08 53.95 | -36 55 44.0 | – | L | C51 |
| 2023-11-04 17:14:05 | S | 23 08 58.69 | -36 54 12.2 | – | L | C51 |