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76818 2000 RG79 (2005)
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MPC Designation: |
2000 RG79 |
| Lightcurves |
Period (h): |
3.1664 ± 0.0001 |
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Amplitude (mag): |
0.14 ± 0.02 |
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Equipment: |
Filter: C
MagBand: R
Telescope: 0.35m f/10 SCT
Camera: SBIG ST-9E
Exposure: 120 |
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Obs. Details |
Date E Mag Phase PABL PABB
2005-08-07 04:00 15.82 17.3 334.9 16.0
2005-08-08 04:00 15.79 16.9 334.9 16.2
2005-08-09 04:00 15.77 16.6 335.0 16.4
2005-08-16 04:00 15.64 14.8 335.5 17.6
2005-08-17 04:00 15.62 14.5 335.6 17.8
2005-08-18 04:00 15.61 14.3 335.6 18.0
2005-08-22 04:00 15.56 13.8 335.8 18.6
2005-08-23 04:00 15.55 13.7 335.9 18.8
2005-08-24 04:00 15.54 13.7 335.9 18.9
2005-08-25 04:00 15.54 13.6 336.0 19.0
2005-08-26 04:00 15.54 13.6 336.0 19.2
2005-08-27 04:00 15.53 13.6 336.0 19.3
2005-08-28 04:00 15.53 13.7 336.1 19.5
2005-08-29 04:00 15.53 13.8 336.1 19.6
2005-08-30 20:00 15.54 13.9 336.2 19.8
2005-08-31 00:00 15.54 13.9 336.2 19.8
2005-09-11 04:00 15.64 16.6 336.8 21.1
2005-09-12 04:00 15.66 16.9 336.8 21.1
2005-09-13 04:00 15.68 17.3 336.9 21.2
2005-09-15 04:00 15.71 17.9 337.0 21.4
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Data Points: |
1044 |
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Discovered: |
2000-09-08 Socorro LINEAR |
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Family/Group: |
Hungaria |
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Taxonomic Class: |
ES (Assumed) |
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Published: |
MPB 38, pending
IAUC 8592 |
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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)PDO binary discovery in collaboration with Petr Pravec's Binary Asteroid Survey group. Only PDO data are shown.
The "dips" orbital curve are due to occultations and/or eclipses involving the satellite. The "bowing" in the orbital curve is the result of the elongated satellite rotating at the same rate as the orbital period, i.e., it is tidally locked to its orbit. |
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Contents © 2011 Brian D. Warner / Palmer Divide Observatory |
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