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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 14 (heliocentric ecliptic J2000)
| Element | Value | Uncertainty (1-sigma) | Units |
| e | .06952460426699875 | 4.736e-08 | |
| a | 2.862208923775778 | 3.0176e-08 | au |
| q | 2.663214981020794 | 1.4174e-07 | au |
| i | 12.63251162015001 | 5.5867e-06 | deg |
| node | 99.57729918734474 | 2.3388e-05 | deg |
| peri | 350.0632781543017 | 5.099e-05 | deg |
| M | 275.3848501388235 | 4.9258e-05 | deg |
| tp | 2459616.215340787088
(2022-Feb-05.71534079) | 0.00024522 | TDB |
| period | 1768.684720512658
4.84 | 2.797e-05
7.658e-08 | d
yr |
| n | .2035410810218641 | 3.2188e-09 | deg/d |
| Q | 3.061202866530762 | 3.2274e-08 | au |
|
| | Orbit Determination Parameters
Additional Information
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Physical Parameter Table
| Parameter |
Symbol |
Value |
Units |
Sigma |
Reference |
Notes |
| absolute magnitude |
H |
16.21 |
|
n/a |
E2021B25 |
|
|
| 304233 Majaess | Discovered 2006 Sept. 14 by D. D. Balam at Mauna Kea. |
| Daniel Majaess (b. 1984) is a young Canadian observational astronomer who researches the Cepheid distance scale, variable stars, and the Milky Way's spiral structure and its many star clusters. He frequently makes innovative use of photometric surveys and data from small telescopes. |
| NOTE: some special characters may not display properly (any characters within {} are an attempt to place the proper accent above a character) |
| Reference: 20120406/MPCPages.arc | Last Updated: 2012-04-09 |
|
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Alternate Designations
| 2006 RE3 = 2003 BC91 = 2003 BH9 = 2009 JM3 |
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