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Rotational Poles and Dimensions of Ceres and Vesta and three STEAs
Jack Drummond Starfire Optical Range Air Force Research Lab
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Rotating 3x2x1 Asteroid
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Fits are Made in the Fourier Plane
Image = E סּ L ₣ (Image) = K0 2J1(x)/x
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Juno Fit Diagnostics Shane 3 m at 2.1μm
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Davida Fit Diagnostics Keck 10 m at 2.1μm
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Ceres(λ=5550) December 2003 HST
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Ceres Oblate Spheroid Observations
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Ceres’ Pole
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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 ±1.5 km
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Vesta October 1997 HST
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Vesta Triaxial Results
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Vesta: AO on Lick 3 m
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Vesta Resolved
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HST Lightcurves SI AO
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Weighted Mean Vesta This Work (n=4) Thomas et al
a = 562±2 km ±10 km b = 543±2 km ±10 km c = 458±4 km ±10 km RA = 325° ° Dec= +55° ° Error radius = 6.7° °
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511 Davida with AO at Keck
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511 Davida with AO at Keck
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511 Davida with AO at Keck
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Davida Edge Features
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52 Europa with AO at Keck
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52 Europa with AO at Keck
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52 Europa with AO at Keck
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2 Pallas with AO at Keck
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Pallas Pole on Ecliptic Globe
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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’
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