Anderson, J. D.; Rappaport, N. J.; Giampieri, G.; et.al. Gravity field and interior structure of Rhea. Physics of the Earth and Planetary Interiors. 2003, 136: 201–213. doi:10.1016/S0031-9201(03)00035-9.引文使用过时参数coauthors (帮助)
More precisely, 0.3911 ± 0.0045 kg·m². Schubert, G.; Anderson, J. D.; Palguta, J.; Travis, B. J. Internal Structure of Rhea and Enceladus. American Geophysical Union, Fall Meeting 2006, abstract #P31D-06. December 2006, 319: 1380. PMID 18323452. doi:10.1126/science.1151524.引文使用过时参数coauthors (帮助)
Anderson, J. D.; Schubert, J. Saturn's satellite Rhea is a homogeneous mix of rock and ice. Geophysical Research Letters. 2007, 34: L02202. doi:10.1029/2006GL028100.引文使用过时参数coauthors (帮助)
The moons more massive than Rhea are: Earth Moon, The 4 Galilean moons, Titan, Triton, Titania, and Oberon. See JPLSSD. (页面存档备份,存于互联网档案馆)
nih.gov
ncbi.nlm.nih.gov
More precisely, 0.3911 ± 0.0045 kg·m². Schubert, G.; Anderson, J. D.; Palguta, J.; Travis, B. J. Internal Structure of Rhea and Enceladus. American Geophysical Union, Fall Meeting 2006, abstract #P31D-06. December 2006, 319: 1380. PMID 18323452. doi:10.1126/science.1151524.引文使用过时参数coauthors (帮助)