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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 46 (heliocentric ecliptic J2000)
Element | Value | Uncertainty (1-sigma) | Units |
e | .1043194808465289 | 1.2039e-08 | |
a | 2.244303903088556 | 4.8759e-09 | au |
q | 2.010179285056519 | 2.8076e-08 | au |
i | 4.162030856651289 | 6.4882e-07 | deg |
node | 75.12857252554623 | 9.5264e-06 | deg |
peri | 73.02327977063328 | 1.4099e-05 | deg |
M | 49.36036319261196 | 9.9992e-06 | deg |
tp | 2459032.117571134996 (2020-Jul-01.61757114) | 3.3915e-05 | TDB |
period | 1228.063783786635 3.36 | 4.0021e-06 1.096e-08 | d yr |
n | .2931443828511654 | 9.5531e-10 | deg/d |
Q | 2.478428521120593 | 5.3845e-09 | au |
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| | Orbit Determination Parameters
Additional Information
|
[ hide covariance matrix ]
Orbital Elements at Epoch 2456550.5 (2013-Sep-15.0) TDB
Reference: JPL 46 (heliocentric ecliptic J2000)
Element | Value | Uncertainty (1-sigma) | Units |
e | .104230270008967 | 1.2079e-08 | |
q | 2.010546356980328 | 2.8157e-08 | au |
tp | 2456575.796022920282 (2013-Oct-10.29602292) | 3.2055e-05 | TDB |
node | 75.15560288282192 | 9.5268e-06 | deg |
peri | 73.1036150992792 | 1.4094e-05 | deg |
i | 4.161805794539642 | 6.4886e-07 | deg |
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| | Orbit Determination Parameters
Additional Information
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Orbit Covariance (6×6)
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|
e |
q |
tp |
node |
peri |
i |
e |
1.458989029153741E-16 |
-3.361240830695345E-16 |
1.14805881015733E-13 |
1.731452961584042E-14 |
1.594590317682242E-14 |
-2.238447687325581E-15 |
q |
-3.361240830695345E-16 |
7.927980676000831E-16 |
-2.402920376025375E-13 |
-4.148027891785807E-14 |
-2.694076142295808E-14 |
5.104347493010875E-15 |
tp |
1.14805881015733E-13 |
-2.402920376025375E-13 |
1.027543676037592E-9 |
-8.041310326125415E-11 |
3.468496429575391E-10 |
2.847009133878144E-12 |
node |
1.731452961584042E-14 |
-4.148027891785807E-14 |
-8.041310326125415E-11 |
9.076074713937039E-11 |
-1.097798949408126E-10 |
-5.689240714211054E-12 |
peri |
1.594590317682242E-14 |
-2.694076142295808E-14 |
3.468496429575391E-10 |
-1.097798949408126E-10 |
1.986501480872016E-10 |
6.326680450264909E-12 |
i |
-2.238447687325581E-15 |
5.104347493010875E-15 |
2.847009133878144E-12 |
-5.689240714211054E-12 |
6.326680450264909E-12 |
4.210232077049837E-13 |
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Physical Parameter Table
Parameter |
Symbol |
Value |
Units |
Sigma |
Reference |
Notes |
absolute magnitude |
H |
12.34 |
|
n/a |
E2021B10 |
|
diameter |
diameter |
7.970 |
km |
0.810 |
urn:nasa:pds:neowise_diameters_albedos::2.0[mainbelt] (http://adsabs.harvard.edu/abs/2014ApJ...791..121M) |
|
rotation period |
rot_per |
2.601 |
h |
n/a |
LCDB (Rev. 2020-October); Warner et al., 2009 |
Published Reference List: [Fleenor, M.L. (2007) Minor Planet Bull. 34, 66-67.] [Vander Haagen, G. (2007) Minor Planet Bull. 34, 107.] [Pietschnig, M. (2011) http://web.utanet.at/pietschm/] [Franco, L.; Baj, G.; Tinella, V.; Bachini, M.; et al. (2017) Minor Planet Bull. 44, 311-312.] [Klinglesmith III, D.A.; Hendrickx, S.; Kimber, C.; Madden, K. (2017) Minor Planet Bull. 44, 244-246.] |
geometric albedo |
albedo |
0.297 |
|
0.095 |
urn:nasa:pds:neowise_diameters_albedos::2.0[mainbelt] (http://adsabs.harvard.edu/abs/2014ApJ...791..121M) |
|
B-V |
BV |
0.930 |
|
0.020 |
EAR-A-5-DDR-UBV-MEAN-VALUES-V1.2 |
#obs=1; phase=10.74 deg. |
U-B |
UB |
0.550 |
|
0.032 |
EAR-A-5-DDR-UBV-MEAN-VALUES-V1.2 |
#obs=1; phase=10.74 deg. |
Tholen spectral type |
spec_T |
S |
|
n/a |
EAR-A-5-DDR-TAXONOMY-V4.0 |
used 2 color indices; used ground-based radiometric albedo |
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1602 Indiana (1950 GF) Discovered 1950-Mar-14 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 GF = 1943 DJ = 1975 XR |
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