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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 39 (heliocentric ecliptic J2000)
Element | Value | Uncertainty (1-sigma) | Units |
e | .07656628218053112 | 2.0411e-08 | |
a | 2.878414958586633 | 9.5098e-09 | au |
q | 2.658025426634828 | 6.308e-08 | au |
i | 2.28015157093717 | 2.615e-07 | deg |
node | 160.5627996028541 | 5.2703e-06 | deg |
peri | 232.4520624792721 | 1.0398e-05 | deg |
M | 265.5380225520762 | 1.1211e-05 | deg |
tp | 2459668.540099826697 (2022-Mar-30.04009983) | 5.6524e-05 | TDB |
period | 1783.72759590493 4.88 | 8.8397e-06 2.42e-08 | d yr |
n | .2018245391429082 | 1.0002e-09 | deg/d |
Q | 3.098804490538439 | 1.0238e-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 |
11.34 |
|
n/a |
E2021B10 |
|
diameter |
diameter |
17.033 |
km |
0.209 |
urn:nasa:pds:neowise_diameters_albedos::2.0[mainbelt] (http://adsabs.harvard.edu/abs/2012ApJ...759L...8M) |
|
rotation period |
rot_per |
12.797 |
h |
n/a |
LCDB (Rev. 2020-October); Warner et al., 2009 |
Published Reference List: [Cooney, W.R., Jr.; Gross, J.; Terrell, D.; Klinglesmith III, D.A.; Hanowell, J. (2015) Minor Planet Bull. 42, 66-67.] [Durech, J.; Hanus, J.; Ali-Lagoa, V. (2018) Astron. Astrophys. 617, A57.] [Durech, J.; Hanus, J. (2018) Astron. Astrophys. 620, A91.] |
geometric albedo |
albedo |
0.201 |
|
0.022 |
urn:nasa:pds:neowise_diameters_albedos::2.0[mainbelt] (http://adsabs.harvard.edu/abs/2012ApJ...759L...8M) |
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1762 Russell (1953 TZ) Discovered 1953-Oct-08 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
1953 TZ = 1947 LM = 1953 TW2 = 1956 GF = 1963 VN |
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