(3317) Paris
Object
| Object |
(3317) Paris |
| Diameter(1) |
119 km |
| Dynamic class(1) |
trojan |
| Absolute magnitude |
8.51 |
| G slop |
0.15 |
Orbital elements
| Epoch (Julian date) |
2460600.5 |
| Semi major axis |
5.229109 ± 0.000000 au |
| Eccentricity |
0.128300537 ± 0.000000008 |
| Inclination |
27.851663138 ± 0.000000444 ° |
| Longitude of ascending node |
135.892158 ± 0.000001 ° |
| Argument of perihelia |
151.127627 ± 0.000005 ° |
| Mean anomaly |
82.882806 ± 0.000003 ° |
| Orbital period |
11.96 yr |
Ephemeris & Observations
| Ephemeris version |
NIMAv9 |
| Observation file (documentation) |
omc_ast_NIMAv9.txt |
| bsp file |
3317_Paris_nima_v9.bsp |
| Date of first observation |
1963-08-21 |
| Date of last observation |
2024-07-09 |
| Number of observations used in the fit |
4486 |
| Number of rejected observations |
24 |
| Number of DES observations |
0 |
| Number of MPC observations |
4274 |
| Number of unpublished observations |
30 |
| RMS of observations |
0.096 arcsec |
Residuals
Residuals in right ascension and declination compared to NIMAv9 ephemeris.
Colours indicate the estimated precision in arcsec used as weights in the fitting process.
Orbit quality
| date |
σα (arcsec) |
σδ (arcsec) |
| 2024-01 |
0.009 |
0.002 |
| 2024-07 |
0.012 |
0.003 |
| 2025-01 |
0.012 |
0.003 |
| 2025-07 |
0.012 |
0.004 |
| 2026-01 |
0.015 |
0.005 |
| 2026-07 |
0.012 |
0.004 |
| 2027-01 |
0.016 |
0.005 |
| 2027-07 |
0.012 |
0.004 |
| 2028-01 |
0.016 |
0.005 |
Ephemeris comparison
Difference between NIMAv9 and JPL74 in right ascension (weighted by cos δ) and in declination.
Gray area represents the 1-σ uncertainty of NIMA ephemeris. Green dots represent the DES observations.
Previous NIMA versions