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arXiv · 1906.07284

Spitzer Albedos of Near-Earth Objects

Annika Gustafsson·David E. Trilling·Michael Mommert·Andrew McNeill·Joseph L. Hora·Howard A. Smith·Stephan Hellmich·Stefano Mottola·Alan W. Harris
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Abstract

Thermal infrared observations are the most effective way to measure asteroid diameter and albedo for a large number of near-Earth objects. Major surveys like NEOWISE, NEOSurvey, ExploreNEOs, and NEOLegacy find a small fraction of high albedo objects that do not have clear analogs in the current meteorite population. About 8% of Spitzer-observed near-Earth objects have nominal albedo solutions greater than 0.5. This may be a result of lightcurve variability leading to an incorrect estimate of diameter or inaccurate absolute visual magnitudes. For a sample of 23 high albedo NEOs we do not find that their shapes are significantly different from the McNeill et al. (2019) near-Earth object shape distribution. We performed a Monte Carlo analysis on 1505 near-Earth objects observed by Spitzer, sampling the visible and thermal fluxes of all targets to determine the likelihood of obtaining a high albedo erroneously. Implementing the McNeill shape distribution for near-Earth objects, we provide an upper-limit on the geometric albedo of 0.5+/-0.1 for the near-Earth population.

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Annika Gustafsson, David E. Trilling, Michael Mommert, Andrew McNeill, Joseph L. Hora, Howard A. Smith, Stephan Hellmich, Stefano Mottola, Alan W. Harris. 2019-06-17. Spitzer Albedos of Near-Earth Objects. https://doi.org/10.3847/1538-3881%2Fab29ea

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