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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 2458600.5 (2019-Apr-27.0) TDB
Reference: JPL 18 (heliocentric ecliptic J2000)
| Element | Value | Uncertainty (1-sigma) | Units |
| e | .2701613158722408 | 4.7292e-08 | |
| a | 2.6305980070515 | 1.7801e-08 | au |
| q | 1.919912187935573 | 1.3268e-07 | au |
| i | 4.635226976801444 | 5.3105e-06 | deg |
| node | 291.7103697086808 | 6.2241e-05 | deg |
| peri | 111.0998378718506 | 6.3361e-05 | deg |
| M | 4.625689374952445 | 1.2334e-05 | deg |
| tp | 2458580.475848527144
(2019-Apr-06.97584853) | 5.3269e-05 | TDB |
| period | 1558.404368711467
4.27 | 1.5818e-05
4.331e-08 | d
yr |
| n | .2310055125792918 | 2.3448e-09 | deg/d |
| Q | 3.341283826167428 | 2.261e-08 | au |
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| | 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 |
15.7 |
|
n/a |
MPO449653 |
|
|
| 109573 Mishasmirnov | Discovered 2001 Aug. 20 at the Simeis branch of the Crimean Astrophysical Observatory. |
| Mikhail Alexandrovich Smirnov (1954-2006), on the staff of the Institute of Astronomy of the Russian Academy of Sciences, studied the minor bodies of the solar system, artificial satellites and the evolution of galaxies. He also made a contribution to popular astronomy in Russia. The name was suggested by S. I. Barabanov. |
| NOTE: some special characters may not display properly (any characters within {} are an attempt to place the proper accent above a character) |
| Reference: 20080520/MPCPages.arc | Last Updated: 2008-05-22 |
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