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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 2457600.5 (2016-Jul-31.0) TDB
Reference: JPL 15 (heliocentric ecliptic J2000)
 Element Value Uncertainty (1-sigma)   Units 
e .1757743132840008 5.6233e-08  
a 3.19869530076808 3.9497e-08 au
q 2.636446830870811 1.9309e-07 au
i 7.071093665818787 6.2152e-06 deg
node 126.717747326104 5.4027e-05 deg
peri 145.9969029666066 5.8389e-05 deg
M 71.98064444056592 2.6878e-05 deg
tp 2457182.697566574028
(2015-Jun-09.19756657)
0.00015123 JED
period 2089.573901460996
5.72
3.8702e-05
1.06e-07
d
yr
n .1722839281962192 3.191e-09 deg/d
Q 3.76094377066535 4.6439e-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 = 1.62364 au 
 Jupiter MOID = 1.39628 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. 2016-February); 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. (2016) Astron. J. 150, A75.]

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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