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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 2459200.5 (2020-Dec-17.0) TDB
Reference: JPL 16 (heliocentric ecliptic J2000)
Element | Value | Uncertainty (1-sigma) | Units |
e | .1359931645992767 | 5.0837e-08 | |
a | 2.480702781210223 | 1.2589e-08 | au |
q | 2.143344159563218 | 1.2912e-07 | au |
i | 3.842749039150984 | 5.4766e-06 | deg |
node | 279.562207663338 | 7.3547e-05 | deg |
peri | 61.78052927273097 | 7.7592e-05 | deg |
M | 191.0857037265258 | 2.7505e-05 | deg |
tp | 2459870.113860458385 (2022-Oct-17.61386046) | 0.00011111 | TDB |
period | 1427.120114065053 3.91 | 1.0864e-05 2.974e-08 | d yr |
n | .2522562722310492 | 1.9203e-09 | deg/d |
Q | 2.818061402857229 | 1.4301e-08 | au |
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| | Orbit Determination Parameters
Additional Information
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Physical Parameter Table
Parameter |
Symbol |
Value |
Units |
Sigma |
Reference |
Notes |
absolute magnitude |
H |
15.13 |
|
n/a |
E2021B10 |
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42487 Ångström | Discovered 1991 Sept. 9 by F. Börngen and L. D. Schmadel at Tautenburg. |
Swedish physicist Anders Jonas Ångström (1814-1874) is a cofounder of astrospectroscopy. He measured the wavelengths of about 1000 Fraunhofer lines, discovering among them some hydrogen lines. The `angstrom', a unit of length equal to the 10-10 meters, was named for him. |
NOTE: some special characters may not display properly (any characters within {} are an attempt to place the proper accent above a character) |
Reference: 20030106/MPCPages.arc | Last Updated: 2003-10-02 |
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