The paper proposes a statistical test for asteroid surface color heterogeneity from sparse multiband photometry and evaluates its performance and sensitivity to model errors through Monte Carlo simulations of synthetic asteroids.
year = 2010, month = oct, volume =
2 Pith papers cite this work. Polarity classification is still indexing.
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astro-ph.EP 2years
2026 2representative citing papers
Derives pole at (276.79°, -21.43°), 28.4517 min period, S-type classification, ~27.4 m size, and thermal inertia 163 J m^{-2} K^{-1} s^{-1/2} for Kamo'oalewa from light curves and a fitted Yarkovsky A2 value.
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Prospects for detecting surface color heterogeneity on asteroid surfaces from sparse multiband photometric survey data
The paper proposes a statistical test for asteroid surface color heterogeneity from sparse multiband photometry and evaluates its performance and sensitivity to model errors through Monte Carlo simulations of synthetic asteroids.
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Physical Characteristics of the Asteroid (469219) Kamo'oalewa as a target of the Chinese Tianwen-2 mission
Derives pole at (276.79°, -21.43°), 28.4517 min period, S-type classification, ~27.4 m size, and thermal inertia 163 J m^{-2} K^{-1} s^{-1/2} for Kamo'oalewa from light curves and a fitted Yarkovsky A2 value.