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2010 RC130 (2010)
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MPC Designation: |
2010 RC130 |
| Lightcurves |
Period (h): |
2.8915 ± 0.0005 |
|
Amplitude (mag): |
1.00 ± 0.03 |
|
Equipment: |
Filter: C
MagBand: R
Telescope: 0.35m f/9.1 SCT
Camera: SBIG STL-1001E
Exposure: 120 |
|
Obs. Details |
Date E Mag Phase PABL PABB
2010-09-29 03:20 16.24 23.8 354.2 6.0
2010-09-29 05:20 16.22 23.6 354.3 5.9
2010-09-29 07:00 16.20 23.4 354.4 5.8
2010-09-30 02:45 15.97 21.0 356.1 4.3
2010-09-30 05:00 15.95 20.7 356.3 4.1
2010-09-30 06:30 15.93 20.5 356.4 4.0
2010-09-30 08:00 15.91 20.3 356.6 3.8
2010-10-01 02:45 15.69 17.7 358.4 2.2
2010-10-01 04:00 15.67 17.5 358.5 2.1
2010-10-01 05:30 15.65 17.3 358.7 1.9
2010-10-01 07:00 15.63 17.1 358.8 1.8
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Data Points: |
310 |
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Discovered: |
|
|
Family/Group: |
NEA |
|
Taxonomic Class: |
S (Assumed) |
|
Published: |
MPB 38, pending |
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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)Discovered to be a tumbler by B. Skiff at Lowell Observatory with analysis by P. Pravec. The two periods are 2.8915 and 1.7378 h. These have almost an exact 3:5 beat frequency with 8.695 h, which is the period used to plot the PDO data. This lead to initially incorrect interpretation of a highly complex lightcurve. However, no physical body can produce this curve at the relatively low phase angle. |
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Contents © 2011 Brian D. Warner / Palmer Divide Observatory |
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