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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.
Orbital Elements at Epoch 2459000.5 (2020-May-31.0) TDB
Reference: JPL 14 (heliocentric ecliptic J2000)
| Element | Value | Uncertainty (1-sigma) | Units |
| e | .1726250338331489 | 5.9496e-08 | |
| a | 2.358169061500259 | 1.0659e-08 | au |
| q | 1.951090047474492 | 1.3781e-07 | au |
| i | 7.63494331683798 | 6.807e-06 | deg |
| node | 45.24282333716944 | 3.1387e-05 | deg |
| peri | 313.9042236864764 | 3.5395e-05 | deg |
| M | 26.90501575691824 | 1.9139e-05 | deg |
| tp | 2458901.646606483875
(2020-Feb-22.14660648) | 6.9819e-05 | TDB |
| period | 1322.698413832153
3.62 | 8.9682e-06
2.455e-08 | d
yr |
| n | .2721708866021844 | 1.8454e-09 | deg/d |
| Q | 2.765248075526026 | 1.2499e-08 | au |
|
| | Orbit Determination Parameters
Additional Information
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Physical Parameter Table
| Parameter |
Symbol |
Value |
Units |
Sigma |
Reference |
Notes |
| absolute magnitude |
H |
15.9 |
|
n/a |
MPO437075 |
|
|
| 226672 Kucinskas | Discovered 2004 Apr. 16 by K. Cernis and J. Zdanavicius at Moletai. |
| Arunas Kucinskas (b. 1967) is a professor at the Astronomical Observatory of Vilnius University. He is an expert in stellar astronomy, astrochemistry and 3D modeling of atmospheres of red giant stars. He is an author of more than 100 scientific papers and many popular science articles. |
| NOTE: some special characters may not display properly (any characters within {} are an attempt to place the proper accent above a character) |
| Reference: MPC batch dated 2017-03-12 | Last Updated: 2017-04-19 |
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