Ellipsoidal geometry in asteroid thermal models - The standard radiometric model

Astronomy and Astrophysics – Astronomy

Scientific paper

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Asteroids, Astronomical Models, Ellipsoids, Radiometric Correction, Albedo, Heat Flux, Light Curve, Asteroids, Geometry, Thermal Properties, Models, Radiometry, Ellipicity, Shape, Flux, Temperture, Wavelengths, Obliquity, Diurnal Variations, Size, Albedo, Comparisons, Diameter, Infrared, Amplitude, Calculations, Diagrams, Lightcurves, Data

Scientific paper

This paper reports results of the incorporation of ellipsoidal geometry into the standard radiometric model for asteroids. The results derived suggest that radiometric measurements of highly nonspherical, low-obliquity asteroids interpreted with spherical models result in systematically smaller diameters and higher albedos. In addition, nonspherical shape can also result in a systematic difference in the diameter of a particular asteroid derived from separate 10- and 20-μm flux measurements interpreted with spherical models. Thermal-infrared diurnal lightcurves calculated for ellipsoids have amplitudes that depend on wavelength as well as projected area, and phase curves calculated for ellipsoids are indistinguishable from those calculated for spheres.

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