Author/Authors :
Binzel، نويسنده , , Richard P. and Rivkin، نويسنده , , Andrew S. and Thomas، نويسنده , , Cristina A. and Vernazza، نويسنده , , Pierre and Burbine، نويسنده , , Thomas H. and DeMeo، نويسنده , , Francesca E. and Bus، نويسنده , , Schelte J. and Tokunaga، نويسنده , , Alan T. and Birlan، نويسنده , , Mirel، نويسنده ,
Abstract :
The known close approach of Asteroid (99942) Apophis in April 2029 provides the opportunity for the case study of a potentially hazardous asteroid in advance of its encounter. The visible to near-infrared (0.55 to 2.45 μm) reflectance spectrum of Apophis is compared and modeled with respect to the spectral and mineralogical characteristics of likely meteorite analogs. Apophis is found to be an Sq-class asteroid that most closely resembles LL ordinary chondrite meteorites in terms of spectral characteristics and interpreted olivine and pyroxene abundances, although we cannot rule out some degree of partial melting. A meteorite analog allows some estimates and conjectures of Apophisʹ possible range of physical properties such as the grain density and micro-porosity of its constituent material. Composition and size similarities of Apophis with (25143) Itokawa suggest a total porosity of 40% as a “current best guess” for Apophis. Applying these parameters to Apophis yields a mass estimate of 2 × 10 10 kg with a corresponding energy estimate of 375 Mt for its potential hazard. Substantial unknowns, most notably the total porosity, allow uncertainties in these mass and energy estimates to be as large as factors of two or three.
