Abstract
(Left) Arecibo radar image of Dione Regio on Venus. White arrows indicate radar-bright features that potentially represent debris from previous volcanic eruptions (Campbell et al. 2017). (Right) Goldstone Solar System Radar image of the near-Earth asteroid (NEA) 2017 BQ 6 showing sharp facets on this object. NEAs display a range of surface features, from which evolution and collisional processes can be constrained, and are important to characterize for planetary defense.
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CITATION STYLE
Lazio, J., Virkki, A. K., Pinilla-Alonso, N., Benner, L. A. M., Brozovic, M., Butler, B. J., … Venditti, F. C. F. (2021). The Next-Generation Ground-Based Planetary Radar. Bulletin of the AAS, 53(4). https://doi.org/10.3847/25c2cfeb.9c808c46
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