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- W2183194711 abstract "The Hungaria asteroids are small (D 24 h), and that the percentage of binary asteroids within the two groups is also similar. Our efforts have now turned to looking at the spin axis pole distribution of the Hungarias, e.g., to determine if that distribution is isotropic or, as Slivan [5] found for the Koronis family, there are distinct “clumps” or trends within the distribution. We report on our initial analysis that is based on the combination of dense and sparse lightcurve data (see Durech et al. [1] for a discussion regarding the differences between dense and sparse data sets). So far, our analysis is inconclusive due to the fact that there are too few Hungarias with sufficient lightcurve data to determine reliable pole solutions. We conclude by discussing the reasons why this is the case and our plans to overcome this deficiency." @default.
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- W2183194711 date "2011-10-01" @default.
- W2183194711 modified "2023-09-24" @default.
- W2183194711 title "Spin Axis Pole Distribution of the Hungaria Asteroids: An Initial Look" @default.
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