Physics – Optics
Scientific paper
Oct 2000
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000dps....32.0805c&link_type=abstract
American Astronomical Society, DPS Meeting #32, #08.05; Bulletin of the American Astronomical Society, Vol. 32, p.1003
Physics
Optics
Scientific paper
Being the biggest asteroid with a reasonably intact basaltic crust, 4 Vesta is a pivotal object to the understanding of the early history of the Solar System. Attempts to map the mineralogical variations on its surface include earth-based spectroscopy on the 0.8-2.5μ m range as well as disk-resolved observations with the HST between 0.4-1.0μ m and JHK imaging with adaptive optics with the Keck Telescope. However,the observations of 4 Vesta during the 1997 opposition with the HST/NICMOS are the first to combine spatial resolution and full rotational coverage with a set of filters that covers the most mineralogically relevant spectral features of HED assemblages. The NICMOS data were all acquired within a 5-day interval, with Vesta's sub-earth latitude varying from -2.8 to -3.5o. Narrow-band filters centered on 0.9536, 1.1298, 1.606, 1.8986 and 2.1641 μ m and medium-band filters on 1.4556 and 2.2181 μ m were used. For each filter, full rotational coverage was obtained, with increments of ~ 20o of longitude. The resulting 144 frames were initially reduced with CALNICA and then PSF-calibrated with the Iterative Blind Deconvolution algorithm. This algorithm, coded on the program IDAC, performs PSF deconvolution through the physically constrained iterative minimization of an error metric. The high signal-to-noise of the data allowed us to achieve super-resolution. Here we compare the first results of the deconvolution with previous results on the surface mineralogy of 4 Vesta. Further developments of this work will lead to the first mineralogical map of 4 Vesta on the 0.95-2.2μ m range. J. Carvano was supported by a CNPq fellowship.
Binzel Richard
Carvano Jorge M.
Drummond Jack
Gaffey M.
Hege Keith
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