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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 40 (heliocentric ecliptic J2000)
| Element | Value | Uncertainty (1-sigma) | Units |
| e | .03222041333464401 | 1.3745e-08 | |
| a | 3.49453881065808 | 2.1488e-08 | au |
| q | 3.381943325764722 | 5.5377e-08 | au |
| i | 19.37786642935036 | 3.6693e-07 | deg |
| node | 306.6445707272197 | 1.799e-06 | deg |
| peri | 111.4251219701707 | 3.3552e-05 | deg |
| M | 81.23930386422323 | 3.5866e-05 | deg |
| tp | 2458662.048090254653
(2019-Jun-27.54809025) | 0.00023622 | TDB |
| period | 2386.070267567749
6.53 | 2.2008e-05
6.025e-08 | d
yr |
| n | .1508756908349424 | 1.3916e-09 | deg/d |
| Q | 3.607134295551439 | 2.218e-08 | au |
|
| | Orbit Determination Parameters
Additional Information
|
[ show covariance matrix ]
Physical Parameter Table
| Parameter |
Symbol |
Value |
Units |
Sigma |
Reference |
Notes |
| absolute magnitude |
H |
11.05 |
|
n/a |
E2021B10 |
|
| diameter |
diameter |
27.077 |
km |
0.435 |
urn:nasa:pds:neowise_diameters_albedos::2.0[mainbelt] (http://adsabs.harvard.edu/abs/2014ApJ...791..121M) |
|
| rotation period |
rot_per |
27.441 |
h |
n/a |
LCDB (Rev. 2020-October); Warner et al., 2009 |
Result based on less than full coverage, so that the period may be wrong by 30 percent or so.
Published Reference List:
[Chang, C.K.; Ip, W.-H.; Lin, H.-W.; Cheng, Y.C.; et al. (2015) Astrophys. J. Supp. Ser. 219, A27.]
[Waszczak, A.; Chang, C.-K.; Ofeck, E.O.; Laher, F.; et al. (2015) Astron. J. 150, A75.] |
| geometric albedo |
albedo |
0.105 |
|
0.021 |
urn:nasa:pds:neowise_diameters_albedos::2.0[mainbelt] (http://adsabs.harvard.edu/abs/2014ApJ...791..121M) |
|
|
| 5833 Peterson | Discovered 1991 Aug. 5 by H. E. Holt at Palomar. |
| Colin A. Peterson (b. 1977), a research support specialist at Cornell University, and responsible for designing sequences for the NEAR spacecraft Multi-Spectral Imager and Near-Infrared Spectrometer team, has developed innovative methods for obtaining spectral maps of (433) Eros. The name was suggested by J. Veverka. |
| NOTE: some special characters may not display properly (any characters within {} are an attempt to place the proper accent above a character) |
| Reference: 19990928/MPCPages.arc | Last Updated: 2010-06-11 |
|
[ show close-approach data ]
Alternate Designations
| 1991 PQ = 1972 TN2 = 1978 PO1 |
|
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