[ 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.
[ revert to old Java-based viewer ]
Orbital Elements at Epoch 2459000.5 (2020-May-31.0) TDB
Reference: JPL 33 (heliocentric ecliptic J2000)
| Element | Value | Uncertainty (1-sigma) | Units |
| e | .1644811971612855 | 3.1259e-08 | |
| a | 2.258380713765068 | 7.0126e-09 | au |
| q | 1.886919550319031 | 7.1837e-08 | au |
| i | 7.662607711454973 | 3.5275e-06 | deg |
| node | 59.20768840275716 | 2.5216e-05 | deg |
| peri | 293.545667392274 | 2.7265e-05 | deg |
| M | 18.68790166756178 | 1.1002e-05 | deg |
| tp | 2458936.149459226169
(2020-Mar-27.64945923) | 3.7798e-05 | TDB |
| period | 1239.63594686452
3.39 | 5.7739e-06
1.581e-08 | d
yr |
| n | .2904078418430571 | 1.3526e-09 | deg/d |
| Q | 2.629841877211105 | 8.1661e-09 | au |
|
| | Orbit Determination Parameters
Additional Information
|
[ show covariance matrix ]
Physical Parameter Table
| Parameter |
Symbol |
Value |
Units |
Sigma |
Reference |
Notes |
| absolute magnitude |
H |
13.2 |
|
n/a |
MPO337317 |
|
| diameter |
diameter |
5.106 |
km |
0.281 |
urn:nasa:pds:neowise_diameters_albedos::2.0[mainbelt] (http://adsabs.harvard.edu/abs/2012ApJ...759L...8M) |
|
| rotation period |
rot_per |
2.6361 |
h |
n/a |
LCDB (Rev. 2019-August); 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:
[Pravec, P.; Wolf, M.; Sarounova, L. (2013) http://www.asu.cas.cz/~ppravec/neo.htm] |
| geometric albedo |
albedo |
0.390 |
|
0.052 |
urn:nasa:pds:neowise_diameters_albedos::2.0[mainbelt] (http://adsabs.harvard.edu/abs/2012ApJ...759L...8M) |
|
|
| 7355 Bottke | Discovered 1995 Apr. 25 by Spacewatch at Kitt Peak. |
| Named in honor of William F. Bottke, Jr., known for his research on the collisional and dynamical evolution of minor planets. He has also contributed to the study of the origin and evolution of NEAs, in particular by analyzing the formation of doublet craters found on the terrestrial planets. |
| NOTE: some special characters may not display properly (any characters within {} are an attempt to place the proper accent above a character) |
| Reference: 19980808/MPCPages.arc | Last Updated: 2009-11-17 |
|
[ show close-approach data ]
Alternate Designations
| 1995 HN2 = 1955 SK = 1984 BN = 1994 BC5 = A911 UG |
|
|
