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1153 Wallenbergia (1924 SL)
Classification: Main-belt Asteroid          SPK-ID: 2001153
Ephemeris | Orbit Diagram | Orbital Elements | Physical Parameters | Discovery Circumstances ]

[ show orbit diagram ]
Orbital Elements at Epoch 2456800.5 (2014-May-23.0) TDB
Reference: JPL 8 (heliocentric ecliptic J2000)
 Element Value Uncertainty (1-sigma)   Units 
e .1607319151736889 6.163e-08  
a 2.195594799070527 7.8594e-09 AU
q 1.842692642070531 1.3405e-07 AU
i 3.334939370537462 5.1594e-06 deg
node 280.5671864283785 0.0001041 deg
peri 28.91620852371245 0.00010545 deg
M 233.7971729898234 2.1661e-05 deg
tp 2457217.075092644220
(2015-Jul-13.57509264)
7.2701e-05 JED
period 1188.301695807703
3.25
6.3805e-06
1.747e-08
d
yr
n .3029533672047011 1.6267e-09 deg/d
Q 2.548496956070524 9.1226e-09 AU
  Orbit Determination Parameters
   # obs. used (total)      1386  
   data-arc span      30653 days (83.92 yr)  
   first obs. used      1930-04-29  
   last obs. used      2014-04-01  
   planetary ephem.      DE431  
   SB-pert. ephem.      SB431-BIG16  
   condition code      0  
   fit RMS      .53421  
   data source      ORB  
   producer      Otto Matic  
   solution date      2014-Apr-17 13:37:41  

Additional Information
 Earth MOID = .82796 AU 
 T_jup = 3.650 
[ show covariance matrix ]

Ephemeris | Orbit Diagram | Orbital Elements | Physical Parameters | Discovery Circumstances ]

Physical Parameter Table
Parameter Symbol Value Units Sigma Reference Notes
absolute magnitude H 12.0 mag n/a MPO256870  
rotation period rot_per 4.096 h n/a Asteroid Lightcurve DataBase (Rev. 2013-Sep-12) Published Reference List:
[Wisniewski, W.Z.; Michalowski, T.M.; Harris, A.W.; McMillan, R.S. (1997) Icarus 126, 395-449; 1995, Lunar & Planetary Science XXVI, 1511-1512.]

1153 Wallenbergia (1924 SL)          Discovered 1924-Sep-05 by Belyavskij, S. at Simeis (094)
Reference: DISCOVERY.DBLast Updated: 2003-08-29

Alternate Designations
 1924 SL = 1930 HH 
Ephemeris | Orbit Diagram | Orbital Elements | Physical Parameters | Discovery Circumstances ]
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