𝔖 Bobbio Scriptorium
✦   LIBER   ✦

Hydromagnetic dynamo in the cores of Uranus and Neptune

✍ Scribed by Torbett, M.; Smoluchowski, R.


Book ID
109719102
Publisher
Nature Publishing Group
Year
1980
Tongue
English
Weight
335 KB
Volume
286
Category
Article
ISSN
0028-0836

No coin nor oath required. For personal study only.


πŸ“œ SIMILAR VOLUMES


On the accretion of Uranus and Neptune
✍ A. Brunini; M.D. Melita πŸ“‚ Article πŸ“… 2002 πŸ› John Wiley and Sons 🌐 English βš– 85 KB
Detecting the signatures of Uranus and N
✍ Stephen R. Kane πŸ“‚ Article πŸ“… 2011 πŸ› Elsevier Science 🌐 English βš– 444 KB

With more than 15 years since the first radial velocity discovery of a planet orbiting a Sun-like star, the time baseline for radial velocity surveys is now extending out beyond the orbit of Jupiter analogs. The sensitivity to exoplanet orbital periods beyond that of Saturn orbital radii however is

The Moons of Uranus, Neptune and Pluto
✍ Brown, Robert Hamilton; Cruikshank, Dale P. πŸ“‚ Article πŸ“… 1985 πŸ› Nature Publishing Group 🌐 English βš– 731 KB
Forming Jupiter, Saturn, Uranus and Nept
✍ Omar G. Benvenuto; Andrea Fortier; AdriΓ‘n Brunini πŸ“‚ Article πŸ“… 2009 πŸ› Elsevier Science 🌐 English βš– 270 KB

Giant planet formation process is still not completely understood. The current most accepted paradigm, the core instability model, explains several observed properties of the Solar System's giant planets but, to date, has faced difficulties to account for a formation time shorter than the observatio