|
1177 Gonnessia (2002)
|
|
MPC Designation: |
1930 WA |
| Lightcurves |
Period (h): |
82. ± 5. |
|
Amplitude (mag): |
0.25 ± 0.10 |
|
Equipment: |
Filter: C
MagBand: R
Telescope: 0.5m f/8.1 R/C
Camera: FLI IMG-1001E
Exposure: 45 |
|
Obs. Details |
Date E Mag Phase PABL PABB
2002-07-13 06:00 14.57 8.4 311.6 14.9
2002-07-14 06:00 14.55 8.2 311.6 15.0
2002-07-15 06:30 14.54 8.0 311.6 15.0
2002-07-16 06:00 14.53 7.8 311.6 15.1
2002-07-18 05:30 14.50 7.4 311.6 15.2
|
|
Data Points: |
205 |
|
|
|
|
Discovered: |
1930-11-24 Algiers L. Boyer |
|
Family/Group: |
MB-Outer |
|
Taxonomic Class: |
XFU |
|
Published: |
MPB 38, pending |
|
|
|
|
NOTES: |
Unless otherwise stated, the "Reduced Magnitudes" in the plots are
Cousins R, based on 2MASS to BVRI conversions (Warner, MPB 34, 113-119)MPB 30, 33-35: P = 6.81, A = 0.11, U = 2
Behrned reports P > 10 h (U = 1).
Remeasured data set indicates a long period. If the assumption is that the full height of the curve has been captured, then the period is on the order of 300 h (bimodal solution). If, as is often the case for very slow rotators, the amplitude is much more, the period is more on the order of 800-1000 h. |
|
Contents © 2011 Brian D. Warner / Palmer Divide Observatory |
|
|
