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Formation of Planets around M
- Bondi radius (Rb=GMp /cs2) Hill's radius (Rh=(Mp/3M* )1/3 a) Disk thickness (H=csa/Vk) ... If Rb Rh, , a large decline in r ( ve r gradient) would be needed ...
Bondi radius (Rb=GMp /cs2) Hill's radius (Rh=(Mp/3M* )1/3 a) Disk thickness (H=csa/Vk) ... If Rb Rh, , a large decline in r ( ve r gradient) would be needed ...
| PowerPoint PPT presentation | free to view
Eduplex Concept Overview $15Myr., 10year Institute
| PowerPoint PPT presentation | free to view
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