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36187 Travisbarman (1999 TB37)
Classification: Main-belt Asteroid          SPK-ID: 2036187
Ephemeris | Orbit Diagram | Orbital Elements | Physical Parameters | Discovery Circumstances | Close-Approach Data ]

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Orbital Elements at Epoch 2457000.5 (2014-Dec-09.0) TDB
Reference: JPL 15 (heliocentric ecliptic J2000)
 Element Value Uncertainty (1-sigma)   Units 
e .1753340146246554 5.6272e-08  
a 3.197231009803488 3.9199e-08 AU
q 2.636647661172201 1.9296e-07 AU
i 7.071725197998815 6.2157e-06 deg
node 126.7206687041893 5.4023e-05 deg
peri 146.0143492168595 5.8406e-05 deg
M 328.5811185404834 2.5769e-05 deg
tp 2457182.741663332364
(2015-Jun-09.24166333)
0.00015146 JED
period 2088.139225585928
5.72
3.8402e-05
1.051e-07
d
yr
n .1724022975043653 3.1706e-09 deg/d
Q 3.757814358434774 4.6072e-08 AU
  Orbit Determination Parameters
   # obs. used (total)      948  
   data-arc span      7037 days (19.27 yr)  
   first obs. used      1996-02-17  
   last obs. used      2015-05-25  
   planetary ephem.      DE431  
   SB-pert. ephem.      SB431-BIG16  
   condition code      0  
   fit RMS      .51931  
   data source      ORB  
   producer      Otto Matic  
   solution date      2015-Jul-06 12:56:34  

Additional Information
 Earth MOID = 1.62547 AU 
 T_jup = 3.159 
[ show covariance matrix ]

Ephemeris | Orbit Diagram | Orbital Elements | Physical Parameters | Discovery Circumstances | Close-Approach Data ]

Physical Parameter Table
Parameter Symbol Value Units Sigma Reference Notes
absolute magnitude H 13.0 mag n/a MPO302275  
rotation period rot_per 8.65 h n/a LCDB (Rev. 2015-July); 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., in press.]

36187 Travisbarman           Discovered 1999 Oct. 13 by the Lowell Observatory Near-Earth Object Search at the Anderson Mesa Station.
Travis S. Barman (b. 1972), an assistant astronomer at Lowell Observatory, models the atmospheres of extrasolar planets using large-scale numerical simulations that predict the atmospheric structure, chemistry and emergent spectra.
NOTE: some special characters may not display properly (any characters within {} are an attempt to place the proper accent above a character)
Reference: 20110615/MPCPages.arcLast Updated: 2013-03-28

[ show close-approach data ]
Ephemeris | Orbit Diagram | Orbital Elements | Physical Parameters | Discovery Circumstances | Close-Approach Data ]
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