| 
        630 Euphemia (2005)
         | 
       
      
         | 
        MPC Designation: | 
        1907 XW | 
       
      
        | Lightcurves  | 
        Period (h): | 
        350. ± 50. | 
       
      
         | 
        Amplitude (mag): | 
        0.45 ± 0.05 | 
       
      
         | 
        Equipment: | 
          Filter: C MagBand: R Telescope: 0.35m f/9.1 SCT Camera:    FLI 1001E Exposure:  150   | 
       
      
         | 
        Obs. Details | 
        Date              E Mag   Phase  PABL   PABB 2005-04-01 08:00  14.32    9.9  185.7   18.4 2005-04-02 09:00  14.34   10.1  185.7   18.4 2005-04-03 09:00  14.35   10.2  185.8   18.4 2005-04-04 09:00  14.36   10.4  185.8   18.4 2005-04-07 09:00  14.40   11.0  185.9   18.4 2005-04-09 09:00  14.43   11.5  186.0   18.4 2005-04-12 09:00  14.48   12.3  186.1   18.3
  | 
       
      
         | 
        Data Points: | 
        624 | 
       
      
         | 
         | 
         | 
       
      
         | 
        Discovered: | 
        1907-03-07  Heidelberg  A. Kopff | 
       
      
         | 
        Family/Group: | 
        Eunomia | 
       
      
         | 
        Taxonomic Class: | 
        S (Assumed) | 
       
      
         | 
        Published: | 
        MPB 38, pending | 
       
      
         | 
         | 
         | 
       
      
         | 
        NOTES:  | 
        Unless otherwise stated, the "Reduced Magnitudes" in the plots are
            Cousins R, based on 2MASS to BVRI conversions (Warner, MPB 34, 113-119)Period in MPB 32, 90-92, was 79.18. Measured images using Comp Star Selector in MPO Canopus and found the new, much longer solution.
The tumbling damping time for this period is > 4.5 Gyr (see Pravec et al., 2005). No obvious signs of tumbling were found but since the data set did not fully cover the curve at least once and start into a second cycle, the lack of evidence is not proof one way or the other. This is rated PAR = 0. | 
       
      
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        Contents © 2011 Brian D. Warner / Palmer Divide Observatory  | 
       
     
       
    
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