|
218144 2002 RL66 (2009)
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MPC Designation: |
2002 RL66 |
| Lightcurves |
Period (h): |
588. ± 10. |
|
Amplitude (mag): |
0.25 ± 0.02 |
|
Equipment: |
Filter: C
MagBand: R
Telescope: 0.35m f/9.1 SCT
Camera: SBIG STL-1001E
Exposure: 240 |
|
Obs. Details |
Date E Mag Phase PABL PABB
2009-11-18 07:00 16.20 27.3 76.4 26.9
2009-11-19 07:00 16.19 27.3 76.7 27.2
2009-11-20 07:00 16.17 27.2 76.9 27.5
2009-11-21 07:00 16.16 27.2 77.2 27.9
2009-11-22 07:00 16.15 27.2 77.5 28.2
2009-11-23 07:00 16.14 27.2 77.8 28.5
2009-11-24 07:00 16.13 27.2 78.0 28.9
2009-11-25 07:00 16.12 27.2 78.3 29.2
2009-11-26 07:00 16.11 27.2 78.6 29.5
2009-11-27 07:00 16.11 27.3 78.9 29.8
2009-11-28 07:00 16.10 27.3 79.1 30.1
2009-11-30 07:00 16.09 27.4 79.7 30.7
2009-12-01 07:00 16.09 27.5 79.9 30.9
2009-12-10 07:00 16.08 28.3 82.3 33.2
2009-12-11 07:00 16.08 28.5 82.6 33.5
2010-01-09 07:00 16.33 32.7 91.6 36.8
2010-01-10 07:00 16.34 32.8 91.9 36.9
2010-01-11 07:00 16.35 33.0 92.3 36.9
2010-02-13 07:00 16.82 35.9 106.6 34.0
|
|
Data Points: |
1348 |
|
|
|
|
Discovered: |
2002-09-06 Socorro LINEAR |
|
Family/Group: |
Mars-crosser |
|
Taxonomic Class: |
S (Assumed) |
|
Published: |
MPB 37, 109-11
MPB 37, 54-64 |
|
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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)Collaboration with P. Pravec, P. Kusnirak, A.W. Harris.
This was the first of at least two asteroids found to have a very long period with a short-period, low-amplitude curve superimposed on the data. |
|
Contents © 2011 Brian D. Warner / Palmer Divide Observatory |
