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154029 2002 CY46 (2010)
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MPC Designation: |
2002 CY46 |
Lightcurves |
Period (h): |
2.554 ± 0.001 |
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Amplitude (mag): |
0.07 ± 0.01 |
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Equipment: |
Filter: C MagBand: r Telescope: 0.35m f/6.8 SCT Camera: SBIG ST-9XE Exposure: 60 |
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Obs. Details |
Date E Mag Phase PABL PABB 2010-09-02 09:25 14.64 45.3 12.5 2.9 2010-09-02 10:25 14.64 45.3 12.5 3.0 2010-09-02 11:00 14.64 45.3 12.5 3.1 2010-09-03 05:22 14.64 45.2 12.2 5.3 2010-09-03 06:15 14.64 45.2 12.1 5.5 2010-09-03 06:50 14.64 45.2 12.1 5.5 2010-09-03 07:30 14.64 45.2 12.1 5.6 2010-09-03 08:20 14.64 45.2 12.1 5.7 2010-09-03 09:20 14.64 45.2 12.1 5.8 2010-09-03 10:15 14.64 45.2 12.1 5.9 2010-09-03 11:15 14.64 45.2 12.0 6.0 2010-09-04 04:10 14.64 45.1 11.7 8.0 2010-09-04 05:00 14.64 45.1 11.6 8.1 2010-09-04 06:25 14.64 45.1 11.6 8.3 2010-09-04 06:50 14.64 45.1 11.6 8.3 2010-09-04 07:15 14.63 45.1 11.6 8.4 2010-09-04 07:40 14.63 45.1 11.6 8.4 2010-09-04 08:10 14.63 45.1 11.6 8.5 2010-09-04 08:30 14.63 45.1 11.6 8.5 2010-09-04 09:00 14.63 45.1 11.5 8.6 2010-09-04 09:25 14.63 45.1 11.5 8.6 2010-09-04 10:05 14.63 45.1 11.5 8.7 2010-09-04 10:50 14.63 45.1 11.5 8.8 2010-09-04 11:10 14.63 45.1 11.5 8.8 2010-09-05 06:10 14.63 45.0 11.0 11.0 2010-09-05 06:30 14.63 45.0 11.0 11.0 2010-09-05 07:15 14.63 45.0 11.0 11.1 2010-09-05 08:05 14.63 45.0 10.9 11.2 2010-09-05 09:00 14.63 45.0 10.9 11.3 2010-09-05 09:55 14.63 45.0 10.9 11.4 2010-09-05 11:10 14.63 45.0 10.9 11.5 2010-09-06 03:40 14.63 44.9 10.4 13.3 2010-09-06 04:00 14.63 44.9 10.4 13.3 2010-09-06 04:20 14.63 44.9 10.4 13.3 2010-09-06 04:40 14.63 44.9 10.4 13.4 2010-09-06 05:10 14.63 44.9 10.4 13.4 2010-09-06 05:50 14.63 44.9 10.3 13.5 2010-09-06 06:30 14.63 44.9 10.3 13.6 2010-09-06 09:00 14.63 44.9 10.3 13.8 2010-09-06 09:40 14.63 44.9 10.3 13.9 2010-09-06 10:00 14.63 44.9 10.2 13.9 2010-09-06 10:40 14.63 44.9 10.2 14.0 2010-09-06 11:00 14.63 44.9 10.2 14.0
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Data Points: |
1052 |
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Discovered: |
2002-02-11 Socorro LINEAR |
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Family/Group: |
NEA |
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Taxonomic Class: |
S (Assumed) |
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Published: |
MPB 38, 32-33 |
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NOTES: |
Unless otherwise stated, the "Reduced Magnitudes" in the plots are
Cousins R, based on 2MASS to BVRI conversions (Warner, MPB 34, 113-119) |
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Contents © 2011 Brian D. Warner / Palmer Divide Observatory |