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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 39 (heliocentric ecliptic J2000)
Element | Value | Uncertainty (1-sigma) | Units |
e | .1184922053355999 | 3.5789e-08 | |
a | 3.027918314125993 | 1.2268e-08 | au |
q | 2.669133595509153 | 1.0608e-07 | au |
i | 11.48791439877861 | 3.5592e-06 | deg |
node | 156.598222468202 | 1.8096e-05 | deg |
peri | 193.1446092286774 | 2.3315e-05 | deg |
M | 73.76609667377654 | 1.5794e-05 | deg |
tp | 2458606.161698341356 (2019-May-02.66169834) | 8.4005e-05 | TDB |
period | 1924.485569907871 5.27 | 1.1696e-05 3.202e-08 | d yr |
n | .187062977051698 | 1.1369e-09 | deg/d |
Q | 3.386703032742834 | 1.3722e-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 |
11.3 |
|
n/a |
MPO265966 |
|
diameter |
diameter |
18.196 |
km |
0.156 |
urn:nasa:pds:neowise_diameters_albedos::2.0[mainbelt] (http://adsabs.harvard.edu/abs/2014ApJ...791..121M) |
|
rotation period |
rot_per |
6.318 |
h |
n/a |
LCDB (Rev. 2020-October); Warner et al., 2009 |
Published Reference List: [Behrend, R. (2003) Observatoire de Geneve web site, http://obswww.unige.ch/~behrend/page_cou.html] [Ivarsen, K.; Willis, S.; Ingleby, L.; Matthews, D.; Simet, M. (2004) Minor Planet Bull. 31, 29-33.] [Warner, B.D. (2014) Minor Planet Bull. 41, 27-32.] [Waszczak, A.; Chang, C.-K.; Ofeck, E.O.; Laher, F.; et al. (2015) Astron. J. 150, A75.] [Durech, J.; Hanus, J. (2018) Astron. Astrophys. 620, A91.] |
geometric albedo |
albedo |
0.233 |
|
0.068 |
urn:nasa:pds:neowise_diameters_albedos::2.0[mainbelt] (http://adsabs.harvard.edu/abs/2014ApJ...791..121M) |
|
SMASSII spectral type |
spec_B |
K |
|
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) |
|
1799 Koussevitzky (1950 OE) Discovered 1950-Jul-25 by Goethe Link Observatory at Brooklyn |
Discovered by the Indiana Asteroid Program, Goethe Link Observatory, University of Indiana. This program was conceived and directed by F. K. Edmondson; the plates were blinked and measured astrometrically by B. Potter and, following her retirement, by D. Owings; and the photometry was performed under the direction of T. Gehrels. During the years 1947-1967, in which the plates were exposed, a large number of people participated in various aspects of the program. |
Reference: DISCOVERY.DB | Last Updated: 2003-08-29 |
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Alternate Designations
1950 OE = 1929 QD = 1974 CF1 |
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