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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 44 (heliocentric ecliptic J2000)
Element | Value | Uncertainty (1-sigma) | Units |
e | .03479223359391707 | 3.4131e-08 | |
a | 2.789499458956716 | 1.2617e-08 | au |
q | 2.692446542170589 | 9.5004e-08 | au |
i | 8.103274439287752 | 3.6763e-06 | deg |
node | 90.31027688235109 | 2.9968e-05 | deg |
peri | 200.0570331796814 | 7.6359e-05 | deg |
M | 255.2258162714329 | 7.2645e-05 | deg |
tp | 2459695.767276901524 (2022-Apr-26.26727690) | 0.00034435 | TDB |
period | 1701.719005002714 4.66 | 1.1545e-05 3.161e-08 | d yr |
n | .2115507900785452 | 1.4353e-09 | deg/d |
Q | 2.886552375742843 | 1.3056e-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 |
12.01 |
|
n/a |
E2021B10 |
|
diameter |
diameter |
10.750 |
km |
0.231 |
urn:nasa:pds:neowise_diameters_albedos::2.0[mainbelt] (http://adsabs.harvard.edu/abs/2014ApJ...791..121M) |
|
rotation period |
rot_per |
18.6632 |
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: [Pal, A.; Szakats, R.; Kiss, C.; Bodi, A.; et al. (2019) Ap. J. Supl. Ser. 247, id.26.] |
geometric albedo |
albedo |
0.222 |
|
0.046 |
urn:nasa:pds:neowise_diameters_albedos::2.0[mainbelt] (http://adsabs.harvard.edu/abs/2012ApJ...759L...8M) |
|
SMASSII spectral type |
spec_B |
Sl |
|
n/a |
EAR-A-5-DDR-TAXONOMY-V4.0 |
based on a high-resolution spectrum by Xu et al. (1995) or Bus and Binzel (2002) |
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5134 Ebilson | Discovered 1990 Sept. 17 by H. E. Holt at Palomar. |
Named in honor of Elizabeth M. Bilson (b. 1937), administrative director of the Center for Radiophysics and Space Research (CRSR), Cornell University. Raised in Hungary, Bilson studied at the Sorbonne and obtained her Ph.D. in chemistry from the University of Illinois at Champaign-Urbana. She was a research associate under Thomas Gold at the CRSR from 1969 to 1983, directing the Lunar Laboratory, and she has coauthored numerous articles related to the physical properties of lunar material, in particular explaining the reason for the low albedo of the moon. She is also a very a good cook. Name proposed by B. E. Clark, and citation written by M. Bilson. |
NOTE: some special characters may not display properly (any characters within {} are an attempt to place the proper accent above a character) |
Reference: 19990728/MPCPages.arc | Last Updated: 2010-06-11 |
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Alternate Designations
1990 SM2 = 1947 LL = 1981 WN6 = 1983 CG = 1985 PL2 = 1986 WS6 |
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