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University of Central Florida

Faculty Bibliography 2010s

2013

Minor planets

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Physical Properties Of B-Type Asteroids From Wise Data, V. Alí-Lagoa, J. De León, J. Licandro, M. Delbó, H. Campins, N. Pinilla-Alonso, M. S. Kelley Jan 2013

Physical Properties Of B-Type Asteroids From Wise Data, V. Alí-Lagoa, J. De León, J. Licandro, M. Delbó, H. Campins, N. Pinilla-Alonso, M. S. Kelley

Faculty Bibliography 2010s

Aims. Our aim is to obtain more information about the physical nature of B-type asteroids and extend previous work by studying their physical properties as derived from fitting an asteroid thermal model to their NASA's Wide-field Infrared Survey Explorer (WISE) data. We also examine the Pallas collisional family, a B-type family with a moderately high albedo in contrast to the large majority of B-types. Methods. We applied a combination of the near-Earth asteroid thermal model and a model of the reflected sunlight to WISE asteroid data in order to derive up to four parameters: effective diameter (D), the so-called infrared …


Additional Spectra Of Asteroid 1996 Fg3, Backup Target Of The Esa Marcopolo-R Mission (Research Note), J. De León, V. Lorenzi, V. Alí-Lagoa, J. Licandro, N. Pinilla-Alonso, H. Campins Jan 2013

Additional Spectra Of Asteroid 1996 Fg3, Backup Target Of The Esa Marcopolo-R Mission (Research Note), J. De León, V. Lorenzi, V. Alí-Lagoa, J. Licandro, N. Pinilla-Alonso, H. Campins

Faculty Bibliography 2010s

Context. Near-Earth binary asteroid (175706) 1996 FG(3) is the current backup target of the ESA MarcoPolo-R mission, selected for the study phase of ESA M3 missions. It is a primitive (C-type) asteroid that shows significant variation in its visible and near-infrared spectra. Aims. Here we present new visible and near-infrared spectra of 1996 FG(3). We compare our new data with other published spectra, analysing the variation in the spectral slope. The asteroid will not be observable again over the next three years at least. Methods. We obtained visible and near-infrared spectra using DOLORES and NICS instruments, respectively, at the Telescopio …