The Spectrum of Comet Bester (1947k).
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The properties expected for small collisional rubble piles should be compared to those of comet 67P; (1) a low bulk density ρ bulk = 535 ± 35 kg m −3 and high porosity of ∼70%;
Compact grouping of rotational transitions due to the small asymmetry (κ = −0.9986), torsional splittings due to internal rotation of the CH 3 group, and relatively large
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Key words: Comet analog; Radar Tomography; Imaging; Internal structure; Bistatic configuration; Electromagnetic wave; Microwave
