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25133 Douglin (1998 SU14)
Classification: Main-belt Asteroid          SPK-ID: 2025133
Ephemeris | Orbit Diagram | Orbital Elements | Mission Design | Physical Parameters | Discovery Circumstances ]

[ show orbit diagram ]
Orbital Elements at Epoch 2459396.5 (2021-Jul-01.0) TDB
Reference: JPL 25 (heliocentric ecliptic J2000)
 Element Value Uncertainty (1-sigma)   Units 
e .1770980614456151 5.0407e-08  
a 2.567628034684476 1.2411e-08 au
q 2.112906087228441 1.3371e-07 au
i 4.44691540662435 3.6988e-06 deg
node 79.68189237655778 6.3304e-05 deg
peri 262.3127142194324 6.438e-05 deg
M 216.0089645533197 1.5708e-05 deg
tp 2459997.576216678127
(2023-Feb-22.07621668)
6.889e-05 TDB
period 1502.784095779724
4.11
1.0896e-05
2.983e-08
d
yr
n .2395553699370321 1.7369e-09 deg/d
Q 3.022349982140511 1.4609e-08 au
  Orbit Determination Parameters
   # obs. used (total)      770  
   data-arc span      9664 days (26.46 yr)  
   first obs. used      1994-10-31  
   last obs. used      2021-04-16  
   planetary ephem.      DE441  
   SB-pert. ephem.      SB441-N16  
   condition code      0  
   norm. resid. RMS      .60422  
   source      ORB  
   producer      Otto Matic  
   solution date      2021-Jul-08 19:06:24  

Additional Information
 Earth MOID = 1.10954 au 
 Jupiter MOID = 2.38451 au 
 T_jup = 3.405 
[ show covariance matrix ]

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

Physical Parameter Table
Parameter Symbol Value Units Sigma Reference Notes
absolute magnitude H 15.19   n/a MPCxxxxx  
diameter diameter 2.403 km 0.315 urn:nasa:pds:neowise_diameters_albedos::2.0[mainbelt] (http://adsabs.harvard.edu/abs/2011ApJ...741...68M)  
geometric albedo albedo 0.306   0.138 urn:nasa:pds:neowise_diameters_albedos::2.0[mainbelt] (http://adsabs.harvard.edu/abs/2011ApJ...741...68M)  

25133 Douglin           Discovered 1998 Sept. 18 by the Lowell Observatory Near-Earth Object Search at the Anderson Mesa Station.
Douglas N. C. Lin (b. 1949) is a theoretical astrophysicist at the University of California, Santa Cruz. He also served as founding director of the Kavli Institute for Astronomy & Astrophysics at Peking University. He has modeled the formation, structure, and evolution of galaxies, globular clusters, stars and planets.
NOTE: some special characters may not display properly (any characters within {} are an attempt to place the proper accent above a character)
Reference: MPC batch dated 2015-09-28Last Updated: 2015-10-05
Ephemeris | Orbit Diagram | Orbital Elements | Mission Design | Physical Parameters | Discovery Circumstances ]
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