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95593 Azusienis (2002 FU10)
Classification: Main-belt Asteroid          SPK-ID: 2095593
Ephemeris | Orbit Diagram | Orbital Elements | Mission Design | Physical Parameters | Discovery Circumstances | Close-Approach Data ]

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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.


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Orbital Elements at Epoch 2459000.5 (2020-May-31.0) TDB
Reference: JPL 22 (heliocentric ecliptic J2000)
 Element Value Uncertainty (1-sigma)   Units 
e .1026610171541347 4.0013e-08  
a 3.049908018783969 2.7988e-08 au
q 2.736801359349055 1.2314e-07 au
i 16.15335789154989 5.3815e-06 deg
node 178.979102408292 1.712e-05 deg
peri 129.8921479697534 3.2262e-05 deg
M 37.37071099393715 2.9001e-05 deg
tp 2458798.543702843319
(2019-Nov-11.04370284)
0.00015577 TDB
period 1945.487924706606
5.33
2.678e-05
7.332e-08
d
yr
n .185043554076179 2.5472e-09 deg/d
Q 3.363014678218883 3.0862e-08 au
  Orbit Determination Parameters
   # obs. used (total)      706  
   data-arc span      8013 days (21.94 yr)  
   first obs. used      1998-08-24  
   last obs. used      2020-08-01  
   planetary ephem.      DE431  
   SB-pert. ephem.      SB431-N16  
   condition code      0  
   norm. resid. RMS      .53687  
   source      ORB  
   producer      Otto Matic  
   solution date      2020-Aug-25 08:39:02  

Additional Information
 Earth MOID = 1.75364 au 
 Jupiter MOID = 2.04729 au 
 T_jup = 3.169 
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Ephemeris | Orbit Diagram | Orbital Elements | Mission Design | Physical Parameters | Discovery Circumstances | Close-Approach Data ]

Physical Parameter Table
Parameter Symbol Value Units Sigma Reference Notes
absolute magnitude H 14.6   n/a MPO474833  

95593 Azusienis           Discovered 2002 Mar. 16 by K. Cernis and J. Zdanavicius at the Moletai Astronomical Observatory
Algimantas Azusienis (b. 1930), a teacher for 50 years at the Vilnius Pedagogical University, has investigated the variable stars and the photometric systems. With V. Straizys he improved the determination of the response curves and parameters of the UBV system.
NOTE: some special characters may not display properly (any characters within {} are an attempt to place the proper accent above a character)
Reference: 20050919/MPCPages.arcLast Updated: 2005-09-26

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