Comparing the NEATM with a Rotating, Cratered Thermophysical Asteroid Model

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dc.creatorWright, Edward L.
dc.date2007-03-05
dc.date2007-04-12
dc.date.accessioned2026-07-07T07:56:12Z
dc.date.available2026-07-07T07:56:12Z
dc.descriptionA cratered asteroid acts somewhat like a retroflector, sending light and infrared radiation back toward the Sun, while thermal inertia in a rotating asteroid causes the infrared radiation to peak over the ``afternoon'' part. In this paper a rotating, cratered asteroid model is described, and used to generate infrared fluxes which are then interpreted using the Near Earth Asteroid Thermal Model (NEATM). Even though the rotating, cratered model depends on three parameters not available to the NEATM (the dimensionless thermal inertia parameter and pole orientation), the NEATM gives diameter estimates that are accurate to 10 percent RMS for phase angles less than 60 degrees. For larger phase angles, such as back-lit asteroids, the infrared flux depends more strongly on these unknown parameters, so the diameter errors are larger. These results are still true for the non-spherical shapes typical of small Near Earth objects.
dc.description9 pages LaTex with 18 Postscript figures. Extended to allow for non-spherical shapes and rotational lightcurves
dc.identifierhttps://arxiv.org/abs/astro-ph/0703085
dc.identifierhttp://arxiv.org/abs/astro-ph/0703085
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/127221
dc.subjectAstrophysics
dc.titleComparing the NEATM with a Rotating, Cratered Thermophysical Asteroid Model
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