|
2577 Litva (2009)
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MPC Designation: |
1975 EE3 |
| Lightcurves |
Period (h): |
2.81258 ± 0.00002 |
|
Amplitude (mag): |
0.24 ± 0.02 |
|
Equipment: |
Filter: C
MagBand: R
Telescope: 0.5m f/8.1 R/C
Camera: SBIG STL-1001E
Exposure: 180 |
|
Obs. Details |
Date E Mag Phase PABL PABB
2009-02-28 06:00 14.88 21.6 141.1 -21.4
2009-03-01 06:00 14.90 21.8 141.2 -21.1
2009-03-02 05:00 14.91 22.0 141.3 -20.8
2009-03-05 00:00 14.97 22.7 141.8 -20.0
2009-03-05 06:00 14.97 22.8 141.8 -19.9
2009-03-06 06:00 14.99 23.0 141.9 -19.6
2009-03-08 05:00 15.04 23.5 142.3 -19.0
2009-03-10 06:00 15.08 24.1 142.6 -18.4
2009-03-12 06:00 15.13 24.6 143.0 -17.7
2009-03-14 06:00 15.18 25.2 143.4 -17.1
2009-03-14 07:00 15.18 25.2 143.4 -17.1
2009-03-15 06:00 15.21 25.5 143.6 -16.8
2009-03-16 05:00 15.23 25.8 143.8 -16.5
2009-03-17 05:00 15.26 26.1 144.0 -16.2
2009-03-19 05:00 15.31 26.6 144.5 -15.6
2009-03-21 05:00 15.36 27.2 144.9 -14.9
2009-03-22 05:00 15.39 27.5 145.2 -14.7
|
|
Data Points: |
941 |
|
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|
|
Discovered: |
1975-03-12 Nauchnyj N. S. Chernykh |
|
Family/Group: |
Hungaria |
|
Taxonomic Class: |
EU |
|
Published: |
MPB 36, 165-166
CBET 1715 |
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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.
This shows three periods: the rotation of the primary, the rotation of the secondary, and the orbital period via mutual events (occultations and/or eclipses). |
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Contents © 2011 Brian D. Warner / Palmer Divide Observatory |
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