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Asteroids
No./Name
Spin Vector Solutions
λ
0° — 360°
0° — 360°
β
-90° — 90°
-90° — 90°
Sidereal Period
period
Ellipsoidal Model
a
⁄
b
b
⁄
c
Methods
OR
AND
A
Amplitudes of lightcurves
B
ADAM - All-Data Asteroid Modelling algorithm (optical lc + radar data + stellar occ. + disc resolved images)
C
Close observations from spacecraft during fly-by or rendezvous
D
Individual data-points of photometric lightcurves
E
Epochs (e.g. times of lightcurve extrema)
F
Fourier coefficients of photometric lightcurves
I
Infrared pre- and post-opposition differences
K
KOALA algorithm (optical lc + stellar occ. + disc resolved images)
L
Lightcurve inversion based on lightcurves
L*
Lightcurve inversion based on lightcurves and sparse data
L**
Lightcurve inversion based on sparse data only
M
Magnitudes (usually at maximum light)
O
Occultation observations
P
Infrared polarimetry
R
Radar observations
S
Surface resolved (e.g. speckle data, adaptive optics)
T
Thermophysical modelling
V
Visual position angles
X
Radar speckles
Z
Zero and non-zero amplitude apparitions imply pole-on view in former case
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