作者: David J. Tholen , B. Zellner
DOI: 10.1016/0019-1035(84)90041-1
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摘要: Abstract Multicolor photometry was obtained of satellites J6 Himalia, J7 Elara, and J10 Lysithea in the prograde cloud outer Jovian satellites, J8 Pasiphae, J9 Sinope, J11 Carme retrograde cloud. Our data for are fragmentary; otherwise, all look like C-class asteroids, except J11, which shows a remarkable brightness ultraviolet. The absence D-class spectra among suggests that they were not derived from same population as outer-belt Trojan asteroid populations.