|
14395 Tommorgan (2012)
|
|
MPC Designation: |
1990 TN3 |
| Lightcurves |
Period (h): |
35.5 ± 0.5 |
|
Amplitude (mag): |
0.61 ± 0.05 |
|
Equipment: |
Filter: C
MagBand: V
Telescope: 0.30m f/9.6 SCT
Camera: ST-9XE
Exposure: 240 |
|
Obs. Details |
Date E Mag Phase PABL PABB
2012-11-05 07:00 16.54 9.3 38.7 11.5
2012-11-06 07:00 16.56 9.7 38.8 11.7
2012-11-07 07:00 16.58 10.2 38.8 11.9
2012-11-08 07:00 16.60 10.6 38.8 12.1
2012-11-12 07:00 16.70 12.7 39.1 12.9
2012-11-13 07:00 16.72 13.2 39.1 13.1
2012-11-14 07:00 16.75 13.7 39.2 13.3
2012-11-15 07:00 16.77 14.2 39.3 13.5
2012-11-16 07:00 16.80 14.8 39.4 13.7
2012-11-17 07:00 16.83 15.3 39.4 13.9
2012-11-18 07:00 16.85 15.8 39.5 14.1
2012-11-19 07:00 16.88 16.4 39.6 14.2
2012-11-20 07:00 16.91 16.9 39.7 14.4
2012-11-21 07:00 16.93 17.4 39.8 14.6
2012-11-22 07:00 16.96 17.9 39.9 14.7
2012-11-24 07:00 17.02 18.9 40.1 15.0
2012-11-25 07:00 17.05 19.4 40.3 15.2
2012-12-04 07:00 17.30 23.3 41.6 16.4
2012-12-07 07:00 17.38 24.4 42.2 16.7
|
|
Data Points: |
963 |
|
|
|
|
Discovered: |
1990-10-15 Palomar E. F. Helin |
|
Family/Group: |
Hungaria |
|
Taxonomic Class: |
ES (Assumed) |
|
Published: |
MPB 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)A tumbler. The period given is the dominant one. Petr Pravec found a second period of 40.4 h. However, it is not a unique solution. |
|
Contents © 2013 Brian D. Warner / Palmer Divide Observatory |
