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Asteroid | P |
![]() |
A | a/b | D |
[h] | [h] | [mag] | [km] | ||
2007 CX50 | 1.45 | ![]() |
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0.035 |
2007 EO | 2.4 | ![]() |
![]() |
![]() |
0.082 |
2007 GU1 | 4.5 | ![]() |
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0.030 |
2007 HL4 | 1.48 | ![]() |
0.55 | ![]() |
0.043 |
2007 RE2 | 1.0 | ![]() |
0.5 | ![]() |
0.081 |
2007 UC2 | 0.527 | ![]() |
0.40 | ![]() |
0.075 |
2007 RY9 | 1.2 | ![]() |
0.60 | ![]() |
0.062 |
2007 TS24 | 1.0 | ![]() |
1.3 | ![]() |
0.039 |
2007 UG6 | 1.82 | ![]() |
0.8 | ![]() |
0.073 |
2007 XN16 | 1.7 | ![]() |
1.4 | ![]() |
0.023 |
2008 CP116 | 0.330 | ![]() |
0.15 | ![]() |
0.082 |
Possible NPA rotation asteroid | |||||
2007 RQ12 | 0.23 | -- | 1.9 | ![]() |
0.059 |
Notes. P is the synodic period of rotation,
is its systematic uncertainty (maximal error), A is the peak-to-peak lightcurve amplitude, a/b is the
elongation of the asteroid and D denotes its effective diameter computed
with the geometric albedo
.
(a) The quoted uncertainty is the standard deviation .
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