[ hide orbit diagram ]
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 38 (heliocentric ecliptic J2000)
Element | Value | Uncertainty (1-sigma) | Units |
e | .02698313355264287 | 2.9295e-08 | |
a | 2.903811517805356 | 1.0616e-08 | au |
q | 2.825457583808711 | 8.2895e-08 | au |
i | 1.292093363284755 | 2.9223e-06 | deg |
node | 316.7116044408558 | 0.00013557 | deg |
peri | 304.4867716269952 | 0.00014779 | deg |
M | 155.7313506359706 | 5.988e-05 | deg |
tp | 2458418.647891751857 (2018-Oct-27.14789175) | 0.00030017 | TDB |
period | 1807.386616887907 4.95 | 9.9115e-06 2.714e-08 | d yr |
n | .1991826190568318 | 1.0923e-09 | deg/d |
Q | 2.982165451802001 | 1.0903e-08 | au |
|
| | Orbit Determination Parameters
Additional Information
|
[ show covariance matrix ]
Physical Parameter Table
Parameter |
Symbol |
Value |
Units |
Sigma |
Reference |
Notes |
absolute magnitude |
H |
13.3 |
|
n/a |
MPO502259 |
|
diameter |
diameter |
5.886 |
km |
0.790 |
urn:nasa:pds:neowise_diameters_albedos::2.0[mainbelt] (http://adsabs.harvard.edu/abs/2012ApJ...759L...8M) |
|
rotation period |
rot_per |
6.218 |
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: [Waszczak, A.; Chang, C.-K.; Ofeck, E.O.; Laher, F.; et al. (2015) Astron. J. 150, A75.] |
geometric albedo |
albedo |
0.293 |
|
0.101 |
urn:nasa:pds:neowise_diameters_albedos::2.0[mainbelt] (http://adsabs.harvard.edu/abs/2012ApJ...759L...8M) |
|
|
11762 Vogel | Discovered 1960 Sept. 24 by C. J. van Houten and I. van Houten-Groeneveld on Palomar Schmidt plates taken by T. Gehrels. |
Hermann Carl Vogel (1841-1907) was a German astronomer and spectroscopist. He invented an early scheme to classify stellar spectra and confirmed the sun's rotation. He directed the Potsdam Astrophysical Observatory from 1882 to 1907. |
NOTE: some special characters may not display properly (any characters within {} are an attempt to place the proper accent above a character) |
Reference: 20070926/MPCPages.arc | Last Updated: 2007-09-30 |
|
[ show close-approach data ]
|