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For accurate long-term ephemerides, please instead use our Horizons system.This orbit viewer was implemented using two-body methods, and hence should not be used for determining accurate long-term trajectories (over several years or decades) or planetary encounter circumstances.
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Orbital Elements at Epoch 2459000.5 (2020-May-31.0) TDB
Reference: JPL 30 (heliocentric ecliptic J2000)
| Element | Value | Uncertainty (1-sigma) | Units |
| e | .2237397107932536 | 3.1171e-08 | |
| a | 2.246151911429859 | 6.2383e-09 | au |
| q | 1.743598532368829 | 7.0714e-08 | au |
| i | 5.646494097732402 | 3.6511e-06 | deg |
| node | 190.3419853369197 | 3.3655e-05 | deg |
| peri | 170.7495136551553 | 3.4376e-05 | deg |
| M | 161.1197620978326 | 7.715e-06 | deg |
| tp | 2458450.195041975439
(2018-Nov-27.69504198) | 2.5757e-05 | TDB |
| period | 1229.580917383361
3.37 | 5.1224e-06
1.402e-08 | d
yr |
| n | .2927826830348885 | 1.2197e-09 | deg/d |
| Q | 2.74870529049089 | 7.634e-09 | au |
|
| | Orbit Determination Parameters
Additional Information
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[ show covariance matrix ]
Physical Parameter Table
| Parameter |
Symbol |
Value |
Units |
Sigma |
Reference |
Notes |
| absolute magnitude |
H |
14.9 |
|
n/a |
MPO449050 |
|
|
| 14122 Josties | Discovered 1998 Aug. 27 by the Lowell Observatory Near-Earth Object Search at the Anderson Mesa Station. |
| F. Jerry Josties (b. 1937) worked at the U.S. Naval Observatory for more than four decades. He managed USNO's photographic double star program and contributed to VLBI work on the determination of polar motion, earth rotation and nutation. |
| NOTE: some special characters may not display properly (any characters within {} are an attempt to place the proper accent above a character) |
| Reference: 20030318/MPCPages.arc | Last Updated: 2003-10-02 |
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