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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 45 (heliocentric ecliptic J2000)
Element | Value | Uncertainty (1-sigma) | Units |
e | .1292141004458163 | 1.9207e-08 | |
a | 3.148877846324935 | 1.137e-08 | au |
q | 2.741998427998299 | 6.0992e-08 | au |
i | 2.474140922492768 | 8.092e-07 | deg |
node | 106.2376457419449 | 1.7175e-05 | deg |
peri | 136.4925374353695 | 1.746e-05 | deg |
M | 34.03632297655863 | 7.271e-06 | deg |
tp | 2459007.537782024349 (2020-Jun-07.03778202) | 4.1071e-05 | TDB |
period | 2040.948974396476 5.59 | 1.1054e-05 3.026e-08 | d yr |
n | .1763885351942494 | 9.5538e-10 | deg/d |
Q | 3.55575726465157 | 1.2839e-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 |
11.87 |
|
n/a |
E2021B10 |
|
diameter |
diameter |
20.623 |
km |
0.240 |
urn:nasa:pds:neowise_diameters_albedos::2.0[mainbelt] (http://adsabs.harvard.edu/abs/2011ApJ...741...68M) |
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rotation period |
rot_per |
4.82 |
h |
n/a |
LCDB (Rev. 2020-October); Warner et al., 2009 |
Published Reference List: [Chang, C.-K.; Ip, W.-H.; Cheng, Y.-C.; Ngeow, C.-C.; et al. (2014) Astrophys. J. 788, A17.] [Waszczak, A.; Chang, C.-K.; Ofeck, E.O.; Laher, F.; et al. (2015) Astron. J. 150, A75.] |
geometric albedo |
albedo |
0.095 |
|
0.007 |
urn:nasa:pds:neowise_diameters_albedos::2.0[mainbelt] (http://adsabs.harvard.edu/abs/2011ApJ...741...68M) |
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1778 Alfven (4506 P-L) Discovered 1960-Sep-26 by PLS at Palomar |
These planets have all been discovered as a result of the Palomar survey of faint minor planets and subsequently identified with planets observed at other oppositions. In Sept. and Oct. 1960, T. Gehrels exposed 130 plates with the 122 cm Schmidt camera at Palomar. In the following years C. J. van Houten and I. van Houten-Groeneveld measured these plates astrometrically and photometrically at Leiden. P. Herget, Cincinnati, computed the orbits of the planets found on the NORC computer, Dahlgren, Virginia, USA. |
Note: "planet" implies "minor planet" |
Reference: DISCOVERY.DB | Last Updated: 2003-08-29 |
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[ show close-approach data ]
Alternate Designations
4506 P-L = 1936 HK = 1952 DD1 = 1958 FB = 1959 NN |
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