|
3854 George (2005)
|
|
MPC Designation: |
1983 EA |
Lightcurves |
Period (h): |
3.3398 ± 0.0002 |
|
Amplitude (mag): |
0.14 ± 0.02 |
|
Equipment: |
Filter: C MagBand: R Telescope: 0.35m f/10 SCT Camera: SBIG ST-9E Exposure: 240 |
|
Obs. Details |
Date E Mag Phase PABL PABB 2005-10-25 04:00 15.37 11.7 24.3 13.3 2005-10-26 04:00 15.39 12.2 24.3 13.5 2005-10-27 04:00 15.41 12.8 24.3 13.8 2005-11-01 04:00 15.54 15.6 24.5 15.0 2005-11-02 04:00 15.56 16.2 24.5 15.2 2005-11-03 04:00 15.59 16.7 24.6 15.4 2005-11-04 04:00 15.62 17.3 24.7 15.7 2005-11-06 04:00 15.67 18.4 24.8 16.1 2005-11-08 04:00 15.73 19.6 24.9 16.5 2005-11-10 04:00 15.78 20.6 25.1 16.9
|
|
Data Points: |
656 |
|
|
|
|
Discovered: |
1983-03-13 Palomar C. S. Shoemaker |
|
Family/Group: |
Hungaria |
|
Taxonomic Class: |
ES (Assumed) |
|
Published: |
MPB 33, 34-35 |
|
|
|
|
NOTES: |
Unless otherwise stated, the "Reduced Magnitudes" in the plots are
Cousins R, based on 2MASS to BVRI conversions (Warner, MPB 34, 113-119)A copule of nights show deviations similar to those of mutual events due to a satellite. However, barring additional confirmation, this can only be regarded as a good target for follow up. |
|
Contents © 2011 Brian D. Warner / Palmer Divide Observatory |
|
|