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Explore dimensions and poles of Ceres and Vesta through advanced imaging techniques like STAs and AO, shedding light on their intriguing characteristics.
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Rotational Poles and Dimensions of Ceres and Vestaand three STEAs Jack Drummond Starfire Optical Range Air Force Research Lab
Fits are Made in the Fourier Plane Image = E סּ L ₣ (Image) = K0 2J1(x)/x
Ceres Dimensions This work Thomas et al a=b=α= 480±1 km 487.3±1.5 km c=[β2-a2 sin(θ)2]½ / cos(θ)= 448±1 km 454.7±1.5 km
Lightcurves HST SI AO
Weighted Mean Vesta This Work (n=4) Thomas et al a = 562±2 km 578±10 km b = 543±2 km 560±10 km c = 458±4 km 458±10 km RA = 325° 301° Dec= +55° +41° Error radius = 6.7° 5°
STEAs(Standard Triaxial Ellipsoid Asteroids) a Al Conrad, Bill Merline, Christophe Dumas, Drummond et al. 2007, Icarus in press: ‘Direct measurement of the size, shape, and pole of 511 Davida with Keck AO in a single night’ b Merline et al. 2007, In prep: ‘Direct measurement of the size, shape, and pole of 52 Europa with Keck AO in a single night’ c Drummond and Julian Christou 2007, Icarus submitted: ‘Triaxial Ellipsoid Dimensions and Rotational Poles of Seven Asteroids from Lick Observatory Adaptive Optics Images, and of Ceres’