[ 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 2459000.5 (2020-May-31.0) TDB
Reference: JPL 43 (heliocentric ecliptic J2000)
| Element | Value | Uncertainty (1-sigma) | Units |
| e | .1451721856420675 | 4.2259e-08 | |
| a | 2.672113414276456 | 1.0009e-08 | au |
| q | 2.284196869642455 | 1.1468e-07 | au |
| i | 12.79975455775937 | 4.8419e-06 | deg |
| node | 36.52578175236357 | 2.0404e-05 | deg |
| peri | 307.1839998902216 | 2.6433e-05 | deg |
| M | 293.8654691298227 | 1.938e-05 | deg |
| tp | 2459293.593734222912
(2021-Mar-20.09373422) | 8.6622e-05 | TDB |
| period | 1595.441034085095
4.37 | 8.9638e-06
2.454e-08 | d
yr |
| n | .2256429365353774 | 1.2677e-09 | deg/d |
| Q | 3.060029958910457 | 1.1462e-08 | au |
|
| | Orbit Determination Parameters
Additional Information
|
[ show covariance matrix ]
Physical Parameter Table
| Parameter |
Symbol |
Value |
Units |
Sigma |
Reference |
Notes |
| absolute magnitude |
H |
9.2 |
|
n/a |
MPO384749 |
|
| diameter |
diameter |
36.06 |
km |
3.5 |
IRAS-A-FPA-3-RDR-IMPS-V6.0 |
IRAS observations used: 16 |
| rotation period |
rot_per |
7.6636 |
h |
n/a |
LCDB (Rev. 2020-October); Warner et al., 2009 |
Published Reference List:
[Pilcher, F. (2018) Minor Planet Bull. 45, 246-247.]
[Polakis, T. (2018) Minor Planet Bull. 45, 199-203.] |
| geometric albedo |
albedo |
0.2361 |
|
0.053 |
IRAS-A-FPA-3-RDR-IMPS-V6.0 |
IRAS observations used: 16 |
| SMASSII spectral type |
spec_B |
S |
|
n/a |
EAR-A-5-DDR-TAXONOMY-V4.0 |
based on a high-resolution spectrum by Xu et al. (1995) or Bus and Binzel (2002) |
|
| 597 Bandusia (A906 HE) Discovered 1906-Apr-16 by Wolf, M. at Heidelberg |
| Reference: DISCOVERY.DB | Last Updated: 2003-08-29 |
|
Alternate Designations
| A906 HE = 1938 YC = 1950 KK = 1958 HJ = A924 MA |
|
|
