[ 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 35 (heliocentric ecliptic J2000)
Element | Value | Uncertainty (1-sigma) | Units |
e | .1018490800552535 | 1.4309e-08 | |
a | 2.337227288640749 | 6.5479e-09 | au |
q | 2.099182839412655 | 3.3084e-08 | au |
i | 4.461929935220081 | 6.6087e-07 | deg |
node | 324.0719147366748 | 7.6312e-06 | deg |
peri | 157.3359123912641 | 1.0848e-05 | deg |
M | 230.4742999435557 | 6.3859e-06 | deg |
tp | 2459670.073193968738 (2022-Mar-31.57319397) | 2.4263e-05 | TDB |
period | 1305.118210170485 3.57 | 5.4846e-06 1.502e-08 | d yr |
n | .275837082951263 | 1.1592e-09 | deg/d |
Q | 2.575271737868845 | 7.2148e-09 | au |
|
| | Orbit Determination Parameters
Additional Information
|
[ show covariance matrix ]
Physical Parameter Table
Parameter |
Symbol |
Value |
Units |
Sigma |
Reference |
Notes |
absolute magnitude |
H |
13.7 |
|
n/a |
MPO381357 |
|
diameter |
diameter |
5.104 |
km |
0.079 |
urn:nasa:pds:neowise_diameters_albedos::2.0[mainbelt] (http://adsabs.harvard.edu/abs/2011ApJ...741...68M) |
|
rotation period |
rot_per |
5.191 |
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 |
0.247 |
|
0.035 |
urn:nasa:pds:neowise_diameters_albedos::2.0[mainbelt] (http://adsabs.harvard.edu/abs/2012ApJ...759L...8M) |
|
|
11503 (1990 BF) Discovered 1990-Jan-21 by Mizuno, Y., Furuta, T. at Kani |
Reference: 19990928/Numbers.arc | Last Updated: 2004-04-19 |
|
Alternate Designations
1990 BF = 1940 BB = 1958 DK1 = 1976 GE8 = 1976 GH8 = 1983 CU3 |
|
|